[{"publication_identifier":{"issn":["2041-8205"],"eissn":["2041-8213"]},"doi":"10.3847/2041-8213/ac6585","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"article_number":"L20","date_updated":"2024-04-02T07:25:50Z","date_published":"2022-05-30T00:00:00Z","author":[{"first_name":"Harvey B.","last_name":"Richer","full_name":"Richer, Harvey B."},{"first_name":"Roger E.","full_name":"Cohen, Roger E.","last_name":"Cohen"},{"first_name":"Jeremy","full_name":"Heyl, Jeremy","last_name":"Heyl"},{"first_name":"Jason","last_name":"Kalirai","full_name":"Kalirai, Jason"},{"id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d","full_name":"Caiazzo, Ilaria","last_name":"Caiazzo","first_name":"Ilaria","orcid":"0000-0002-4770-5388"},{"first_name":"Matteo","last_name":"Correnti","full_name":"Correnti, Matteo"},{"full_name":"Cummings, Jeffrey","last_name":"Cummings","first_name":"Jeffrey"},{"first_name":"Paul","full_name":"Goudfrooij, Paul","last_name":"Goudfrooij"},{"full_name":"Hansen, Bradley M. S.","last_name":"Hansen","first_name":"Bradley M. S."},{"first_name":"Molly","full_name":"Peeples, Molly","last_name":"Peeples"},{"first_name":"Elena","full_name":"Sabbi, Elena","last_name":"Sabbi"},{"full_name":"Tremblay, Pier-Emmanuel","last_name":"Tremblay","first_name":"Pier-Emmanuel"},{"first_name":"Benjamin","last_name":"Williams","full_name":"Williams, Benjamin"}],"month":"05","oa_version":"Published Version","scopus_import":"1","language":[{"iso":"eng"}],"external_id":{"arxiv":["2203.11264"]},"oa":1,"citation":{"ista":"Richer HB, Cohen RE, Heyl J, Kalirai J, Caiazzo I, Correnti M, Cummings J, Goudfrooij P, Hansen BMS, Peeples M, Sabbi E, Tremblay P-E, Williams B. 2022. When do stars go boom? The Astrophysical Journal Letters. 931(2), L20.","ama":"Richer HB, Cohen RE, Heyl J, et al. When do stars go boom? <i>The Astrophysical Journal Letters</i>. 2022;931(2). doi:<a href=\"https://doi.org/10.3847/2041-8213/ac6585\">10.3847/2041-8213/ac6585</a>","chicago":"Richer, Harvey B., Roger E. Cohen, Jeremy Heyl, Jason Kalirai, Ilaria Caiazzo, Matteo Correnti, Jeffrey Cummings, et al. “When Do Stars Go Boom?” <i>The Astrophysical Journal Letters</i>. American Astronomical Society, 2022. <a href=\"https://doi.org/10.3847/2041-8213/ac6585\">https://doi.org/10.3847/2041-8213/ac6585</a>.","apa":"Richer, H. B., Cohen, R. E., Heyl, J., Kalirai, J., Caiazzo, I., Correnti, M., … Williams, B. (2022). When do stars go boom? <i>The Astrophysical Journal Letters</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/2041-8213/ac6585\">https://doi.org/10.3847/2041-8213/ac6585</a>","ieee":"H. B. Richer <i>et al.</i>, “When do stars go boom?,” <i>The Astrophysical Journal Letters</i>, vol. 931, no. 2. American Astronomical Society, 2022.","short":"H.B. Richer, R.E. Cohen, J. Heyl, J. Kalirai, I. Caiazzo, M. Correnti, J. Cummings, P. Goudfrooij, B.M.S. Hansen, M. Peeples, E. Sabbi, P.-E. Tremblay, B. Williams, The Astrophysical Journal Letters 931 (2022).","mla":"Richer, Harvey B., et al. “When Do Stars Go Boom?” <i>The Astrophysical Journal Letters</i>, vol. 931, no. 2, L20, American Astronomical Society, 2022, doi:<a href=\"https://doi.org/10.3847/2041-8213/ac6585\">10.3847/2041-8213/ac6585</a>."},"year":"2022","date_created":"2024-03-26T10:28:48Z","article_type":"original","quality_controlled":"1","title":"When do stars go boom?","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","status":"public","intvolume":"       931","_id":"15210","abstract":[{"lang":"eng","text":"The maximum mass of a star that can produce a white dwarf (WD) is an important astrophysical quantity. One of the best approaches to establishing this limit is to search for WDs in young star clusters in which only massive stars have had time to evolve and where the mass of the progenitor can be established from the cooling time of the WD together with the age of the cluster. Searches in young Milky Way clusters have not thus far yielded WD members more massive than about 1.1 M⊙, well below the Chandrasekhar mass of 1.38 M⊙, nor progenitors with masses in excess of about 6 M⊙. However, the hunt for potentially massive WDs that escaped their cluster environs is yielding interesting candidates. To expand the cluster sample further, we used HST to survey four young and massive star clusters in the Magellanic Clouds for bright WDs that could have evolved from stars as massive as 10 M⊙. We located five potential WD candidates in the oldest of the four clusters examined, the first extragalactic single WDs thus far discovered. As these hot WDs are very faint at optical wavelengths, final confirmation will likely have to await spectroscopy with 30 m class telescopes."}],"main_file_link":[{"url":"https://doi.org/10.3847/2041-8213/ac6585","open_access":"1"}],"arxiv":1,"publication_status":"published","type":"journal_article","day":"30","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"volume":931,"publisher":"American Astronomical Society","publication":"The Astrophysical Journal Letters","extern":"1","issue":"2","article_processing_charge":"No"},{"_id":"15211","intvolume":"       605","pmid":1,"abstract":[{"lang":"eng","text":"Over a dozen millisecond pulsars are ablating low-mass companions in close binary systems. In the original ‘black widow’, the eight-hour orbital period eclipsing pulsar PSR J1959+2048 (PSR B1957+20)1, high-energy emission originating from the pulsar2 is irradiating and may eventually destroy3 a low-mass companion. These systems are not only physical laboratories that reveal the interesting results of exposing a close companion star to the relativistic energy output of a pulsar, but are also believed to harbour some of the most massive neutron stars4, allowing for robust tests of the neutron star equation of state. Here we report observations of ZTF J1406+1222, a wide hierarchical triple hosting a 62-minute orbital period black widow candidate, the optical flux of which varies by a factor of more than ten. ZTF J1406+1222 pushes the boundaries of evolutionary models5, falling below the 80-minute minimum orbital period of hydrogen-rich systems. The wide tertiary companion is a rare low-metallicity cool subdwarf star, and the system has a Galactic halo orbit consistent with passing near the Galactic Centre, making it a probe of formation channels, neutron star kick physics6 and binary evolution."}],"status":"public","main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/2205.02278"}],"arxiv":1,"publication_status":"published","type":"journal_article","volume":605,"page":"41-45","keyword":["Multidisciplinary"],"day":"04","issue":"7908","publication":"Nature","extern":"1","publisher":"Springer Nature","article_processing_charge":"No","oa":1,"citation":{"mla":"Burdge, Kevin B., et al. “A 62-Minute Orbital Period Black Widow Binary in a Wide Hierarchical Triple.” <i>Nature</i>, vol. 605, no. 7908, Springer Nature, 2022, pp. 41–45, doi:<a href=\"https://doi.org/10.1038/s41586-022-04551-1\">10.1038/s41586-022-04551-1</a>.","short":"K.B. Burdge, T.R. Marsh, J. Fuller, E.C. Bellm, I. Caiazzo, D. Chakrabarty, M.W. Coughlin, K. De, V.S. Dhillon, M.J. Graham, P. Rodríguez-Gil, A.D. Jaodand, D.L. Kaplan, E. Kara, A.K.H. Kong, S.R. Kulkarni, K.-L. Li, S.P. Littlefair, W.A. Majid, P. Mróz, A.B. Pearlman, E.S. Phinney, J. van Roestel, R.A. Simcoe, I. Andreoni, A.J. Drake, R.G. Dekany, D.A. Duev, E.C. Kool, A.A. Mahabal, M.S. Medford, R. Riddle, T.A. Prince, Nature 605 (2022) 41–45.","ieee":"K. B. Burdge <i>et al.</i>, “A 62-minute orbital period black widow binary in a wide hierarchical triple,” <i>Nature</i>, vol. 605, no. 7908. Springer Nature, pp. 41–45, 2022.","ista":"Burdge KB, Marsh TR, Fuller J, Bellm EC, Caiazzo I, Chakrabarty D, Coughlin MW, De K, Dhillon VS, Graham MJ, Rodríguez-Gil P, Jaodand AD, Kaplan DL, Kara E, Kong AKH, Kulkarni SR, Li K-L, Littlefair SP, Majid WA, Mróz P, Pearlman AB, Phinney ES, Roestel J van, Simcoe RA, Andreoni I, Drake AJ, Dekany RG, Duev DA, Kool EC, Mahabal AA, Medford MS, Riddle R, Prince TA. 2022. A 62-minute orbital period black widow binary in a wide hierarchical triple. Nature. 605(7908), 41–45.","ama":"Burdge KB, Marsh TR, Fuller J, et al. A 62-minute orbital period black widow binary in a wide hierarchical triple. <i>Nature</i>. 2022;605(7908):41-45. doi:<a href=\"https://doi.org/10.1038/s41586-022-04551-1\">10.1038/s41586-022-04551-1</a>","chicago":"Burdge, Kevin B., Thomas R. Marsh, Jim Fuller, Eric C. Bellm, Ilaria Caiazzo, Deepto Chakrabarty, Michael W. Coughlin, et al. “A 62-Minute Orbital Period Black Widow Binary in a Wide Hierarchical Triple.” <i>Nature</i>. Springer Nature, 2022. <a href=\"https://doi.org/10.1038/s41586-022-04551-1\">https://doi.org/10.1038/s41586-022-04551-1</a>.","apa":"Burdge, K. B., Marsh, T. R., Fuller, J., Bellm, E. C., Caiazzo, I., Chakrabarty, D., … Prince, T. A. (2022). A 62-minute orbital period black widow binary in a wide hierarchical triple. <i>Nature</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s41586-022-04551-1\">https://doi.org/10.1038/s41586-022-04551-1</a>"},"date_created":"2024-03-26T10:29:26Z","year":"2022","quality_controlled":"1","article_type":"original","title":"A 62-minute orbital period black widow binary in a wide hierarchical triple","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2024-04-02T07:26:19Z","date_published":"2022-05-04T00:00:00Z","author":[{"full_name":"Burdge, Kevin B.","last_name":"Burdge","first_name":"Kevin B."},{"first_name":"Thomas R.","last_name":"Marsh","full_name":"Marsh, Thomas R."},{"full_name":"Fuller, Jim","last_name":"Fuller","first_name":"Jim"},{"first_name":"Eric C.","full_name":"Bellm, Eric C.","last_name":"Bellm"},{"first_name":"Ilaria","orcid":"0000-0002-4770-5388","id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d","full_name":"Caiazzo, Ilaria","last_name":"Caiazzo"},{"full_name":"Chakrabarty, Deepto","last_name":"Chakrabarty","first_name":"Deepto"},{"full_name":"Coughlin, Michael W.","last_name":"Coughlin","first_name":"Michael W."},{"last_name":"De","full_name":"De, Kishalay","first_name":"Kishalay"},{"first_name":"V. S.","last_name":"Dhillon","full_name":"Dhillon, V. S."},{"last_name":"Graham","full_name":"Graham, Matthew J.","first_name":"Matthew J."},{"full_name":"Rodríguez-Gil, Pablo","last_name":"Rodríguez-Gil","first_name":"Pablo"},{"first_name":"Amruta D.","full_name":"Jaodand, Amruta D.","last_name":"Jaodand"},{"first_name":"David L.","full_name":"Kaplan, David L.","last_name":"Kaplan"},{"full_name":"Kara, Erin","last_name":"Kara","first_name":"Erin"},{"first_name":"Albert K. H.","last_name":"Kong","full_name":"Kong, Albert K. H."},{"last_name":"Kulkarni","full_name":"Kulkarni, S. R.","first_name":"S. R."},{"first_name":"Kwan-Lok","last_name":"Li","full_name":"Li, Kwan-Lok"},{"full_name":"Littlefair, S. P.","last_name":"Littlefair","first_name":"S. P."},{"full_name":"Majid, Walid A.","last_name":"Majid","first_name":"Walid A."},{"last_name":"Mróz","full_name":"Mróz, Przemek","first_name":"Przemek"},{"first_name":"Aaron B.","last_name":"Pearlman","full_name":"Pearlman, Aaron B."},{"first_name":"E. S.","full_name":"Phinney, E. S.","last_name":"Phinney"},{"last_name":"Roestel","full_name":"Roestel, Jan van","first_name":"Jan van"},{"first_name":"Robert A.","last_name":"Simcoe","full_name":"Simcoe, Robert A."},{"last_name":"Andreoni","full_name":"Andreoni, Igor","first_name":"Igor"},{"last_name":"Drake","full_name":"Drake, Andrew J.","first_name":"Andrew J."},{"last_name":"Dekany","full_name":"Dekany, Richard G.","first_name":"Richard G."},{"full_name":"Duev, Dmitry A.","last_name":"Duev","first_name":"Dmitry A."},{"full_name":"Kool, Erik C.","last_name":"Kool","first_name":"Erik C."},{"full_name":"Mahabal, Ashish A.","last_name":"Mahabal","first_name":"Ashish A."},{"first_name":"Michael S.","full_name":"Medford, Michael S.","last_name":"Medford"},{"last_name":"Riddle","full_name":"Riddle, Reed","first_name":"Reed"},{"first_name":"Thomas A.","full_name":"Prince, Thomas A.","last_name":"Prince"}],"month":"05","oa_version":"Preprint","scopus_import":"1","language":[{"iso":"eng"}],"external_id":{"pmid":["35508781"],"arxiv":["2205.02278"]},"publication_identifier":{"eissn":["1476-4687"],"issn":["0028-0836"]},"doi":"10.1038/s41586-022-04551-1"},{"publication_identifier":{"eissn":["1365-2966"],"issn":["0035-8711"]},"doi":"10.1093/mnras/stac458","scopus_import":"1","oa_version":"Preprint","month":"02","external_id":{"arxiv":["2110.00598"]},"language":[{"iso":"eng"}],"date_updated":"2024-04-02T07:26:50Z","author":[{"full_name":"Fleury, Leesa","last_name":"Fleury","first_name":"Leesa"},{"orcid":"0000-0002-4770-5388","first_name":"Ilaria","id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d","full_name":"Caiazzo, Ilaria","last_name":"Caiazzo"},{"last_name":"Heyl","full_name":"Heyl, Jeremy","first_name":"Jeremy"}],"date_published":"2022-02-21T00:00:00Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","title":"The cooling of massive white dwarfs from <i>Gaia</i> EDR3","citation":{"mla":"Fleury, Leesa, et al. “The Cooling of Massive White Dwarfs from <i>Gaia</i> EDR3.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 511, no. 4, Oxford University Press, 2022, pp. 5984–93, doi:<a href=\"https://doi.org/10.1093/mnras/stac458\">10.1093/mnras/stac458</a>.","ieee":"L. Fleury, I. Caiazzo, and J. Heyl, “The cooling of massive white dwarfs from <i>Gaia</i> EDR3,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 511, no. 4. Oxford University Press, pp. 5984–5993, 2022.","short":"L. Fleury, I. Caiazzo, J. Heyl, Monthly Notices of the Royal Astronomical Society 511 (2022) 5984–5993.","apa":"Fleury, L., Caiazzo, I., &#38; Heyl, J. (2022). The cooling of massive white dwarfs from <i>Gaia</i> EDR3. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stac458\">https://doi.org/10.1093/mnras/stac458</a>","chicago":"Fleury, Leesa, Ilaria Caiazzo, and Jeremy Heyl. “The Cooling of Massive White Dwarfs from <i>Gaia</i> EDR3.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2022. <a href=\"https://doi.org/10.1093/mnras/stac458\">https://doi.org/10.1093/mnras/stac458</a>.","ama":"Fleury L, Caiazzo I, Heyl J. The cooling of massive white dwarfs from <i>Gaia</i> EDR3. <i>Monthly Notices of the Royal Astronomical Society</i>. 2022;511(4):5984-5993. doi:<a href=\"https://doi.org/10.1093/mnras/stac458\">10.1093/mnras/stac458</a>","ista":"Fleury L, Caiazzo I, Heyl J. 2022. The cooling of massive white dwarfs from <i>Gaia</i> EDR3. Monthly Notices of the Royal Astronomical Society. 511(4), 5984–5993."},"oa":1,"quality_controlled":"1","article_type":"original","date_created":"2024-03-26T10:31:05Z","year":"2022","volume":511,"page":"5984-5993","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"day":"21","type":"journal_article","article_processing_charge":"No","issue":"4","publication":"Monthly Notices of the Royal Astronomical Society","extern":"1","publisher":"Oxford University Press","main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/2110.00598"}],"abstract":[{"lang":"eng","text":"We determine the distribution of cooling ages of massive Gaia EDR3 white dwarfs identified with over 90 per cent probability within 200 pc and with mass in the range 0.95–1.25 M⊙. Using three sets of publicly available models, we consider sub-samples of these white dwarfs sorted into three equally spaced mass bins. Under the assumption of a constant white dwarf formation rate, we find an excess of white dwarfs, both along the Q branch and below it, corresponding respectively to stars that are in the process of freezing and those that are completely frozen. We compare the cooling age distributions for each of these bins to the recently determined time-varying star formation rate of Gaia DR2 main sequence stars. For white dwarfs in the two lightest mass bins, spanning the mass range 0.95–1.15 M⊙, we find that the cumulative cooling age distribution is statistically consistent with the expectation from the star formation rate. For white dwarfs in the heaviest mass bin, 1.15–1.25 M⊙, we find that their cumulative distribution is inconsistent with the star formation rate for all of the models considered; instead, we find that their cooling age distribution is well fitted by a linear combination of the distribution expected for single stellar evolution products and the distribution expected for double white dwarf merger products when approximately 40–50 per cent of the 1.15–1.25 M⊙ white dwarfs that formed over the past 4 Gyr are produced through double white dwarf mergers."}],"_id":"15212","intvolume":"       511","status":"public","publication_status":"published","arxiv":1},{"date_updated":"2024-04-02T07:27:20Z","author":[{"first_name":"David R.","full_name":"Miller, David R.","last_name":"Miller"},{"first_name":"Ilaria","orcid":"0000-0002-4770-5388","id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d","full_name":"Caiazzo, Ilaria","last_name":"Caiazzo"},{"full_name":"Heyl, Jeremy","last_name":"Heyl","first_name":"Jeremy"},{"first_name":"Harvey B.","last_name":"Richer","full_name":"Richer, Harvey B."},{"last_name":"Tremblay","full_name":"Tremblay, Pier-Emmanuel","first_name":"Pier-Emmanuel"}],"date_published":"2022-02-21T00:00:00Z","scopus_import":"1","oa_version":"Published Version","month":"02","external_id":{"arxiv":["2110.09668"]},"language":[{"iso":"eng"}],"publication_identifier":{"eissn":["2041-8213"],"issn":["2041-8205"]},"doi":"10.3847/2041-8213/ac50a5","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"article_number":"L24","main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/2041-8213/ac50a5"}],"status":"public","_id":"15213","abstract":[{"text":"We searched through the entire Gaia EDR3 candidate white dwarf catalog for stars with proper motions and positions that are consistent with them having escaped from the Alpha Persei cluster within the past 81 Myr, the age of the cluster. In this search we found five candidate white dwarf escapees from Alpha Persei and obtained spectra for all of them. We confirm that three are massive white dwarfs sufficiently young to have originated in the cluster. All these are more massive than any white dwarf previously associated with a cluster using Gaia astrometry, and possess some of the most massive progenitors. In particular, the white dwarf Gaia EDR3 4395978097863572, which lies within 25 pc of the cluster center, has a mass of about 1.20 solar masses and evolved from an 8.5 solar-mass star, pushing the upper limit for white dwarf formation from a single massive star, while still leaving a substantial gap between the resulting white dwarf mass and the Chandrasekhar mass.","lang":"eng"}],"intvolume":"       926","publication_status":"published","arxiv":1,"day":"21","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"volume":926,"type":"journal_article","article_processing_charge":"No","publisher":"American Astronomical Society","issue":"2","extern":"1","publication":"The Astrophysical Journal Letters","citation":{"mla":"Miller, David R., et al. “The Ultramassive White Dwarfs of the Alpha Persei Cluster.” <i>The Astrophysical Journal Letters</i>, vol. 926, no. 2, L24, American Astronomical Society, 2022, doi:<a href=\"https://doi.org/10.3847/2041-8213/ac50a5\">10.3847/2041-8213/ac50a5</a>.","short":"D.R. Miller, I. Caiazzo, J. Heyl, H.B. Richer, P.-E. Tremblay, The Astrophysical Journal Letters 926 (2022).","ieee":"D. R. Miller, I. Caiazzo, J. Heyl, H. B. Richer, and P.-E. Tremblay, “The ultramassive white dwarfs of the Alpha Persei cluster,” <i>The Astrophysical Journal Letters</i>, vol. 926, no. 2. American Astronomical Society, 2022.","ama":"Miller DR, Caiazzo I, Heyl J, Richer HB, Tremblay P-E. The ultramassive white dwarfs of the Alpha Persei cluster. <i>The Astrophysical Journal Letters</i>. 2022;926(2). doi:<a href=\"https://doi.org/10.3847/2041-8213/ac50a5\">10.3847/2041-8213/ac50a5</a>","ista":"Miller DR, Caiazzo I, Heyl J, Richer HB, Tremblay P-E. 2022. The ultramassive white dwarfs of the Alpha Persei cluster. The Astrophysical Journal Letters. 926(2), L24.","apa":"Miller, D. R., Caiazzo, I., Heyl, J., Richer, H. B., &#38; Tremblay, P.-E. (2022). The ultramassive white dwarfs of the Alpha Persei cluster. <i>The Astrophysical Journal Letters</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/2041-8213/ac50a5\">https://doi.org/10.3847/2041-8213/ac50a5</a>","chicago":"Miller, David R., Ilaria Caiazzo, Jeremy Heyl, Harvey B. Richer, and Pier-Emmanuel Tremblay. “The Ultramassive White Dwarfs of the Alpha Persei Cluster.” <i>The Astrophysical Journal Letters</i>. American Astronomical Society, 2022. <a href=\"https://doi.org/10.3847/2041-8213/ac50a5\">https://doi.org/10.3847/2041-8213/ac50a5</a>."},"oa":1,"article_type":"original","quality_controlled":"1","year":"2022","date_created":"2024-03-26T10:31:25Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","title":"The ultramassive white dwarfs of the Alpha Persei cluster"},{"date_updated":"2024-04-02T07:27:52Z","date_published":"2022-02-18T00:00:00Z","author":[{"last_name":"Heyl","full_name":"Heyl, Jeremy","first_name":"Jeremy"},{"orcid":"0000-0002-4770-5388","first_name":"Ilaria","last_name":"Caiazzo","full_name":"Caiazzo, Ilaria","id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d"},{"first_name":"Harvey B.","full_name":"Richer, Harvey B.","last_name":"Richer"}],"month":"02","scopus_import":"1","oa_version":"Published Version","language":[{"iso":"eng"}],"external_id":{"arxiv":["2110.03837"]},"publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"doi":"10.3847/1538-4357/ac45fc","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"article_number":"132","_id":"15214","intvolume":"       926","abstract":[{"text":"We search through an eight million cubic parsec volume surrounding the Pleiades star cluster and the Sun to identify both the current and past members of the Pleiades cluster within the Gaia EDR3 data set. We find nearly 1300 current cluster members and 289 former cluster candidates. Many of these candidates lie well in front of or behind the cluster from our point of view, so formerly they were considered cluster members, but their parallaxes put them more than 10 pc from the center of the cluster today. Over the past 100 Myr we estimate that the cluster has lost twenty percent of its mass including two massive white dwarf stars and the α2 Canum Venaticorum type variable star, 41 Tau. All three white dwarfs associated with the cluster are massive (1.01–1.06 M⊙) and have progenitors with main-sequence masses of about six solar masses. Although we did not associate any giant stars with the cluster, the cooling time of the oldest white dwarf of 60 Myr gives a firm lower limit on the age of the cluster.","lang":"eng"}],"status":"public","main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/1538-4357/ac45fc"}],"arxiv":1,"publication_status":"published","type":"journal_article","volume":926,"keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"day":"18","extern":"1","publication":"The Astrophysical Journal","issue":"2","publisher":"American Astronomical Society","article_processing_charge":"No","oa":1,"citation":{"apa":"Heyl, J., Caiazzo, I., &#38; Richer, H. B. (2022). Reconstructing the Pleiades with Gaia EDR3. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/ac45fc\">https://doi.org/10.3847/1538-4357/ac45fc</a>","chicago":"Heyl, Jeremy, Ilaria Caiazzo, and Harvey B. Richer. “Reconstructing the Pleiades with Gaia EDR3.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2022. <a href=\"https://doi.org/10.3847/1538-4357/ac45fc\">https://doi.org/10.3847/1538-4357/ac45fc</a>.","ama":"Heyl J, Caiazzo I, Richer HB. Reconstructing the Pleiades with Gaia EDR3. <i>The Astrophysical Journal</i>. 2022;926(2). doi:<a href=\"https://doi.org/10.3847/1538-4357/ac45fc\">10.3847/1538-4357/ac45fc</a>","ista":"Heyl J, Caiazzo I, Richer HB. 2022. Reconstructing the Pleiades with Gaia EDR3. The Astrophysical Journal. 926(2), 132.","ieee":"J. Heyl, I. Caiazzo, and H. B. Richer, “Reconstructing the Pleiades with Gaia EDR3,” <i>The Astrophysical Journal</i>, vol. 926, no. 2. American Astronomical Society, 2022.","short":"J. Heyl, I. Caiazzo, H.B. Richer, The Astrophysical Journal 926 (2022).","mla":"Heyl, Jeremy, et al. “Reconstructing the Pleiades with Gaia EDR3.” <i>The Astrophysical Journal</i>, vol. 926, no. 2, 132, American Astronomical Society, 2022, doi:<a href=\"https://doi.org/10.3847/1538-4357/ac45fc\">10.3847/1538-4357/ac45fc</a>."},"date_created":"2024-03-26T10:31:44Z","year":"2022","quality_controlled":"1","article_type":"original","title":"Reconstructing the Pleiades with Gaia EDR3","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87"},{"publication_status":"published","status":"public","pmid":1,"_id":"15268","intvolume":"        90","abstract":[{"lang":"eng","text":"Apolipoprotein A‐I (apoA‐I) has a key function in the reverse cholesterol transport. However, aggregation of apoA‐I single point mutants can lead to hereditary amyloid pathology. Although several studies have tackled the biophysical and structural consequences introduced by these mutations, there is little information addressing the relationship between the evolutionary and structural features that contribute to the amyloid behavior of apoA‐I. We combined evolutionary studies, in silico mutagenesis and molecular dynamics (MD) simulations to provide a comprehensive analysis of the conservation and pathogenic role of the aggregation‐prone regions (APRs) present in apoA‐I. Sequence analysis demonstrated that among the four amyloidogenic regions described for human apoA‐I, only two (APR1 and APR4) are evolutionary conserved across different species of Sarcopterygii. Moreover, stability analysis carried out with the FoldX engine showed that APR1 contributes to the marginal stability of apoA‐I. Structural properties of full‐length apoA‐I models suggest that aggregation is avoided by placing APRs into highly packed and rigid portions of its native fold. Compared to silent variants extracted from the gnomAD database, the thermodynamic and pathogenic impact of amyloid mutations showed evidence of a higher destabilizing effect. MD simulations of the amyloid variant G26R evidenced the partial unfolding of the alpha‐helix bundle with the concomitant exposure of APR1 to the solvent, suggesting an insight into the early steps involved in its aggregation. Our findings highlight APR1 as a relevant component for apoA‐I structural integrity and emphasize a destabilizing effect of amyloid variants that leads to the exposure of this region."}],"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1101/2020.09.18.304337"}],"publisher":"Wiley","issue":"1","publication":"Proteins: Structure, Function, and Bioinformatics","article_processing_charge":"No","type":"journal_article","page":"258-269","day":"01","keyword":["Molecular Biology","Biochemistry","Structural Biology"],"volume":90,"year":"2022","date_created":"2024-04-03T07:49:53Z","article_type":"original","corr_author":"1","quality_controlled":"1","oa":1,"citation":{"short":"R.A. Gisonno, T. Masson, N.A. Ramella, E.E. Barrera, V. Romanowski, M.A. Tricerri, Proteins: Structure, Function, and Bioinformatics 90 (2022) 258–269.","ieee":"R. A. Gisonno, T. Masson, N. A. Ramella, E. E. Barrera, V. Romanowski, and M. A. Tricerri, “Evolutionary and structural constraints influencing apolipoprotein A‐I amyloid behavior,” <i>Proteins: Structure, Function, and Bioinformatics</i>, vol. 90, no. 1. Wiley, pp. 258–269, 2022.","mla":"Gisonno, Romina A., et al. “Evolutionary and Structural Constraints Influencing Apolipoprotein A‐I Amyloid Behavior.” <i>Proteins: Structure, Function, and Bioinformatics</i>, vol. 90, no. 1, Wiley, 2022, pp. 258–69, doi:<a href=\"https://doi.org/10.1002/prot.26217\">10.1002/prot.26217</a>.","chicago":"Gisonno, Romina A., Tomas Masson, Nahuel A. Ramella, Exequiel E. Barrera, Víctor Romanowski, and M. Alejandra Tricerri. “Evolutionary and Structural Constraints Influencing Apolipoprotein A‐I Amyloid Behavior.” <i>Proteins: Structure, Function, and Bioinformatics</i>. Wiley, 2022. <a href=\"https://doi.org/10.1002/prot.26217\">https://doi.org/10.1002/prot.26217</a>.","apa":"Gisonno, R. A., Masson, T., Ramella, N. A., Barrera, E. E., Romanowski, V., &#38; Tricerri, M. A. (2022). Evolutionary and structural constraints influencing apolipoprotein A‐I amyloid behavior. <i>Proteins: Structure, Function, and Bioinformatics</i>. Wiley. <a href=\"https://doi.org/10.1002/prot.26217\">https://doi.org/10.1002/prot.26217</a>","ista":"Gisonno RA, Masson T, Ramella NA, Barrera EE, Romanowski V, Tricerri MA. 2022. Evolutionary and structural constraints influencing apolipoprotein A‐I amyloid behavior. Proteins: Structure, Function, and Bioinformatics. 90(1), 258–269.","ama":"Gisonno RA, Masson T, Ramella NA, Barrera EE, Romanowski V, Tricerri MA. Evolutionary and structural constraints influencing apolipoprotein A‐I amyloid behavior. <i>Proteins: Structure, Function, and Bioinformatics</i>. 2022;90(1):258-269. doi:<a href=\"https://doi.org/10.1002/prot.26217\">10.1002/prot.26217</a>"},"title":"Evolutionary and structural constraints influencing apolipoprotein A‐I amyloid behavior","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_published":"2022-01-01T00:00:00Z","author":[{"first_name":"Romina A.","full_name":"Gisonno, Romina A.","last_name":"Gisonno"},{"first_name":"Tomas","orcid":"0000-0002-2634-6283","full_name":"Masson, Tomas","last_name":"Masson","id":"93ac43e8-8599-11eb-9b86-f6efb0a4c207"},{"full_name":"Ramella, Nahuel A.","last_name":"Ramella","first_name":"Nahuel A."},{"full_name":"Barrera, Exequiel E.","last_name":"Barrera","first_name":"Exequiel E."},{"first_name":"Víctor","full_name":"Romanowski, Víctor","last_name":"Romanowski"},{"last_name":"Tricerri","full_name":"Tricerri, M. Alejandra","first_name":"M. Alejandra"}],"date_updated":"2024-10-09T21:08:44Z","language":[{"iso":"eng"}],"external_id":{"pmid":["34414600"]},"month":"01","oa_version":"Preprint","doi":"10.1002/prot.26217","publication_identifier":{"issn":["0887-3585"],"eissn":["1097-0134"]},"department":[{"_id":"MaJö"}]},{"publication_status":"published","abstract":[{"lang":"eng","text":"A versatile, scalable, room temperature and surfactant-free route for the synthesis of metal chalcogenide nanoparticles in aqueous solution is detailed here for the production of PbS and Cu-doped PbS nanoparticles. Subsequently, nanoparticles are annealed in a reducing atmosphere to remove surface oxide, and consolidated into dense polycrystalline materials by means of spark plasma sintering. By characterizing the transport properties of the sintered material, we observe the annealing step and the incorporation of Cu to play a key role in promoting the thermoelectric performance of PbS. The presence of Cu allows improving the electrical conductivity by increasing the charge carrier concentration and simultaneously maintaining a large charge carrier mobility, which overall translates into record power factors at ambient temperature, 2.3 mWm-1K−2. Simultaneously, the lattice thermal conductivity decreases with the introduction of Cu, leading to a record high ZT = 0.37 at room temperature and ZT = 1.22 at 773 K. Besides, a record average ZTave = 0.76 is demonstrated in the temperature range 320–773 K for n-type Pb0.955Cu0.045S."}],"_id":"10566","intvolume":"       433","status":"public","main_file_link":[{"url":"https://ddd.uab.cat/pub/artpub/2022/270830/10.1016j.cej.2021.133837.pdf","open_access":"1"}],"publication":"Chemical Engineering Journal","publisher":"Elsevier","article_processing_charge":"No","type":"journal_article","volume":433,"day":"01","date_created":"2021-12-19T23:01:33Z","year":"2022","corr_author":"1","quality_controlled":"1","article_type":"original","oa":1,"citation":{"short":"M. Li, Y. Liu, Y. Zhang, C. Chang, T. Zhang, D. Yang, K. Xiao, J. Arbiol, M. Ibáñez, A. Cabot, Chemical Engineering Journal 433 (2022).","ieee":"M. Li <i>et al.</i>, “Room temperature aqueous-based synthesis of copper-doped lead sulfide nanoparticles for thermoelectric application,” <i>Chemical Engineering Journal</i>, vol. 433. Elsevier, 2022.","mla":"Li, Mengyao, et al. “Room Temperature Aqueous-Based Synthesis of Copper-Doped Lead Sulfide Nanoparticles for Thermoelectric Application.” <i>Chemical Engineering Journal</i>, vol. 433, 133837, Elsevier, 2022, doi:<a href=\"https://doi.org/10.1016/j.cej.2021.133837\">10.1016/j.cej.2021.133837</a>.","apa":"Li, M., Liu, Y., Zhang, Y., Chang, C., Zhang, T., Yang, D., … Cabot, A. (2022). Room temperature aqueous-based synthesis of copper-doped lead sulfide nanoparticles for thermoelectric application. <i>Chemical Engineering Journal</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.cej.2021.133837\">https://doi.org/10.1016/j.cej.2021.133837</a>","chicago":"Li, Mengyao, Yu Liu, Yu Zhang, Cheng Chang, Ting Zhang, Dawei Yang, Ke Xiao, Jordi Arbiol, Maria Ibáñez, and Andreu Cabot. “Room Temperature Aqueous-Based Synthesis of Copper-Doped Lead Sulfide Nanoparticles for Thermoelectric Application.” <i>Chemical Engineering Journal</i>. Elsevier, 2022. <a href=\"https://doi.org/10.1016/j.cej.2021.133837\">https://doi.org/10.1016/j.cej.2021.133837</a>.","ama":"Li M, Liu Y, Zhang Y, et al. Room temperature aqueous-based synthesis of copper-doped lead sulfide nanoparticles for thermoelectric application. <i>Chemical Engineering Journal</i>. 2022;433. doi:<a href=\"https://doi.org/10.1016/j.cej.2021.133837\">10.1016/j.cej.2021.133837</a>","ista":"Li M, Liu Y, Zhang Y, Chang C, Zhang T, Yang D, Xiao K, Arbiol J, Ibáñez M, Cabot A. 2022. Room temperature aqueous-based synthesis of copper-doped lead sulfide nanoparticles for thermoelectric application. Chemical Engineering Journal. 433, 133837."},"title":"Room temperature aqueous-based synthesis of copper-doped lead sulfide nanoparticles for thermoelectric application","ec_funded":1,"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_published":"2022-04-01T00:00:00Z","author":[{"last_name":"Li","full_name":"Li, Mengyao","first_name":"Mengyao"},{"orcid":"0000-0001-7313-6740","first_name":"Yu","id":"2A70014E-F248-11E8-B48F-1D18A9856A87","full_name":"Liu, Yu","last_name":"Liu"},{"first_name":"Yu","full_name":"Zhang, Yu","last_name":"Zhang"},{"orcid":"0000-0002-9515-4277","first_name":"Cheng","last_name":"Chang","id":"9E331C2E-9F27-11E9-AE48-5033E6697425","full_name":"Chang, Cheng"},{"last_name":"Zhang","full_name":"Zhang, Ting","first_name":"Ting"},{"first_name":"Dawei","last_name":"Yang","full_name":"Yang, Dawei"},{"last_name":"Xiao","full_name":"Xiao, Ke","first_name":"Ke"},{"first_name":"Jordi","last_name":"Arbiol","full_name":"Arbiol, Jordi"},{"last_name":"Ibáñez","id":"43C61214-F248-11E8-B48F-1D18A9856A87","full_name":"Ibáñez, Maria","first_name":"Maria","orcid":"0000-0001-5013-2843"},{"first_name":"Andreu","full_name":"Cabot, Andreu","last_name":"Cabot"}],"date_updated":"2025-04-14T07:43:48Z","project":[{"grant_number":"754411","name":"ISTplus - Postdoctoral Fellowships","call_identifier":"H2020","_id":"260C2330-B435-11E9-9278-68D0E5697425"},{"grant_number":"M02889","name":"Bottom-up Engineering for Thermoelectric Applications","_id":"9B8804FC-BA93-11EA-9121-9846C619BF3A"},{"_id":"9B8F7476-BA93-11EA-9121-9846C619BF3A","name":"HighTE: The Werner Siemens Laboratory for the High Throughput Discovery of Semiconductors for Waste Heat Recovery"}],"language":[{"iso":"eng"}],"external_id":{"isi":["000773425200006"]},"month":"04","oa_version":"Submitted Version","scopus_import":"1","doi":"10.1016/j.cej.2021.133837","publication_identifier":{"issn":["1385-8947"]},"acknowledgement":"This work was supported by the European Regional Development Funds. MYL, YZ, DWY and KX thank the China Scholarship Council for scholarship support. YL acknowledges funding from the European Union's Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant agreement No. 754411 and the funding for scientific research startup of Hefei University of Technology (No. 13020-03712021049). MI acknowledges funding from IST Austria and the Werner Siemens Foundation. CC acknowledges funding from the FWF “Lise Meitner Fellowship” grant agreement M 2889-N. TZ has received funding from the CSC-UAB PhD scholarship program. ICN2 acknowledges funding from Generalitat de Catalunya 2017 SGR 327. ICN2 thanks support from the project NANOGEN (PID2020-116093RB-C43), funded by MCIN/ AEI/10.13039/501100011033/. ICN2 is supported by the Severo Ochoa program from Spanish MINECO (Grant No. SEV-2017-0706) and is funded by the CERCA Programme / Generalitat de Catalunya. Part of the present work has been performed in the framework of Universitat Autònoma de Barcelona Materials Science PhD program.","article_number":"133837","department":[{"_id":"MaIb"}],"isi":1},{"publication_status":"published","status":"public","abstract":[{"text":"The synthetic strigolactone (SL) analog, rac-GR24, has been instrumental in studying the role of SLs as well as karrikins because it activates the receptors DWARF14 (D14) and KARRIKIN INSENSITIVE 2 (KAI2) of their signaling pathways, respectively. Treatment with rac-GR24 modifies the root architecture at different levels, such as decreasing the lateral root density (LRD), while promoting root hair elongation or flavonol accumulation. Previously, we have shown that the flavonol biosynthesis is transcriptionally activated in the root by rac-GR24 treatment, but, thus far, the molecular players involved in that response have remained unknown. To get an in-depth insight into the changes that occur after the compound is perceived by the roots, we compared the root transcriptomes of the wild type and the more axillary growth2 (max2) mutant, affected in both SL and karrikin signaling pathways, with and without rac-GR24 treatment. Quantitative reverse transcription (qRT)-PCR, reporter line analysis and mutant phenotyping indicated that the flavonol response and the root hair elongation are controlled by the ELONGATED HYPOCOTYL 5 (HY5) and MYB12 transcription factors, but HY5, in contrast to MYB12, affects the LRD as well. Furthermore, we identified the transcription factors TARGET OF MONOPTEROS 5 (TMO5) and TMO5 LIKE1 as negative and the Mediator complex as positive regulators of the rac-GR24 effect on LRD. Altogether, hereby, we get closer toward understanding the molecular mechanisms that underlay the rac-GR24 responses in the root.","lang":"eng"}],"_id":"10583","pmid":1,"intvolume":"        63","main_file_link":[{"url":"https://doi.org/10.1093/pcp/pcab149","open_access":"1"}],"publisher":"Oxford University Press","issue":"1","publication":"Plant & Cell Physiology","article_processing_charge":"No","type":"journal_article","day":"21","page":"104-119","keyword":["flavonols","MAX2","rac-Gr24","RNA-seq","root development","transcriptional regulation"],"volume":63,"year":"2022","date_created":"2021-12-28T11:44:18Z","article_type":"original","quality_controlled":"1","oa":1,"citation":{"chicago":"Struk, Sylwia, Lukas Braem, Cedrick Matthys, Alan Walton, Nick Vangheluwe, Stan Van Praet, Lingxiang Jiang, et al. “Transcriptional Analysis in the Arabidopsis Roots Reveals New Regulators That Link Rac-GR24 Treatment with Changes in Flavonol Accumulation, Root Hair Elongation and Lateral Root Density.” <i>Plant &#38; Cell Physiology</i>. Oxford University Press, 2022. <a href=\"https://doi.org/10.1093/pcp/pcab149\">https://doi.org/10.1093/pcp/pcab149</a>.","apa":"Struk, S., Braem, L., Matthys, C., Walton, A., Vangheluwe, N., Van Praet, S., … Goormachtig, S. (2022). Transcriptional analysis in the Arabidopsis roots reveals new regulators that link rac-GR24 treatment with changes in flavonol accumulation, root hair elongation and lateral root density. <i>Plant &#38; Cell Physiology</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/pcp/pcab149\">https://doi.org/10.1093/pcp/pcab149</a>","ista":"Struk S, Braem L, Matthys C, Walton A, Vangheluwe N, Van Praet S, Jiang L, Baster P, De Cuyper C, Boyer F-D, Stes E, Beeckman T, Friml J, Gevaert K, Goormachtig S. 2022. Transcriptional analysis in the Arabidopsis roots reveals new regulators that link rac-GR24 treatment with changes in flavonol accumulation, root hair elongation and lateral root density. Plant &#38; Cell Physiology. 63(1), 104–119.","ama":"Struk S, Braem L, Matthys C, et al. Transcriptional analysis in the Arabidopsis roots reveals new regulators that link rac-GR24 treatment with changes in flavonol accumulation, root hair elongation and lateral root density. <i>Plant &#38; Cell Physiology</i>. 2022;63(1):104-119. doi:<a href=\"https://doi.org/10.1093/pcp/pcab149\">10.1093/pcp/pcab149</a>","ieee":"S. Struk <i>et al.</i>, “Transcriptional analysis in the Arabidopsis roots reveals new regulators that link rac-GR24 treatment with changes in flavonol accumulation, root hair elongation and lateral root density,” <i>Plant &#38; Cell Physiology</i>, vol. 63, no. 1. Oxford University Press, pp. 104–119, 2022.","short":"S. Struk, L. Braem, C. Matthys, A. Walton, N. Vangheluwe, S. Van Praet, L. Jiang, P. Baster, C. De Cuyper, F.-D. Boyer, E. Stes, T. Beeckman, J. Friml, K. Gevaert, S. Goormachtig, Plant &#38; Cell Physiology 63 (2022) 104–119.","mla":"Struk, Sylwia, et al. “Transcriptional Analysis in the Arabidopsis Roots Reveals New Regulators That Link Rac-GR24 Treatment with Changes in Flavonol Accumulation, Root Hair Elongation and Lateral Root Density.” <i>Plant &#38; Cell Physiology</i>, vol. 63, no. 1, Oxford University Press, 2022, pp. 104–19, doi:<a href=\"https://doi.org/10.1093/pcp/pcab149\">10.1093/pcp/pcab149</a>."},"title":"Transcriptional analysis in the Arabidopsis roots reveals new regulators that link rac-GR24 treatment with changes in flavonol accumulation, root hair elongation and lateral root density","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","date_published":"2022-01-21T00:00:00Z","author":[{"first_name":"Sylwia","full_name":"Struk, Sylwia","last_name":"Struk"},{"first_name":"Lukas","last_name":"Braem","full_name":"Braem, Lukas"},{"full_name":"Matthys, Cedrick","last_name":"Matthys","first_name":"Cedrick"},{"first_name":"Alan","full_name":"Walton, Alan","last_name":"Walton"},{"first_name":"Nick","full_name":"Vangheluwe, Nick","last_name":"Vangheluwe"},{"last_name":"Van Praet","full_name":"Van Praet, Stan","first_name":"Stan"},{"last_name":"Jiang","full_name":"Jiang, Lingxiang","first_name":"Lingxiang"},{"first_name":"Pawel","id":"3028BD74-F248-11E8-B48F-1D18A9856A87","full_name":"Baster, Pawel","last_name":"Baster"},{"last_name":"De Cuyper","full_name":"De Cuyper, Carolien","first_name":"Carolien"},{"full_name":"Boyer, Francois-Didier","last_name":"Boyer","first_name":"Francois-Didier"},{"first_name":"Elisabeth","last_name":"Stes","full_name":"Stes, Elisabeth"},{"first_name":"Tom","last_name":"Beeckman","full_name":"Beeckman, Tom"},{"orcid":"0000-0002-8302-7596","first_name":"Jiří","full_name":"Friml, Jiří","id":"4159519E-F248-11E8-B48F-1D18A9856A87","last_name":"Friml"},{"first_name":"Kris","last_name":"Gevaert","full_name":"Gevaert, Kris"},{"last_name":"Goormachtig","full_name":"Goormachtig, Sofie","first_name":"Sofie"}],"date_updated":"2023-08-02T13:40:43Z","language":[{"iso":"eng"}],"external_id":{"isi":["000877899400009"],"pmid":["34791413"]},"month":"01","oa_version":"Published Version","scopus_import":"1","doi":"10.1093/pcp/pcab149","publication_identifier":{"issn":["0032-0781"],"eissn":["1471-9053"]},"acknowledgement":"The authors thank Ralf Stracke (Bielefeld University, Bielefeld, Germany) for providing the myb mutants and their colleagues Bert De Rybel for the tmo5t;mo5l1 double mutant, Boris Parizot for tips on the RNA-seq analysis, Veronique Storme for statistical help on both the RNA-seq and lateral root density, and Martine De Cock for help in preparing the manuscript.","department":[{"_id":"JiFr"}],"isi":1},{"title":"Electrically tunable lens (ETL) - based variable focus imaging system for parametric surface texture analysis of materials","file_date_updated":"2022-01-03T13:43:01Z","user_id":"3E5EF7F0-F248-11E8-B48F-1D18A9856A87","year":"2022","date_created":"2022-01-02T23:01:33Z","article_type":"original","quality_controlled":"1","oa":1,"citation":{"ama":"Nirwan JS, Lou S, Hussain S, et al. Electrically tunable lens (ETL) - based variable focus imaging system for parametric surface texture analysis of materials. <i>Micromachines</i>. 2022;13(1). doi:<a href=\"https://doi.org/10.3390/mi13010017\">10.3390/mi13010017</a>","ista":"Nirwan JS, Lou S, Hussain S, Nauman M, Hussain T, Conway BR, Ghori MU. 2022. Electrically tunable lens (ETL) - based variable focus imaging system for parametric surface texture analysis of materials. Micromachines. 13(1), 17.","apa":"Nirwan, J. S., Lou, S., Hussain, S., Nauman, M., Hussain, T., Conway, B. R., &#38; Ghori, M. U. (2022). Electrically tunable lens (ETL) - based variable focus imaging system for parametric surface texture analysis of materials. <i>Micromachines</i>. MDPI. <a href=\"https://doi.org/10.3390/mi13010017\">https://doi.org/10.3390/mi13010017</a>","chicago":"Nirwan, Jorabar Singh, Shan Lou, Saqib Hussain, Muhammad Nauman, Tariq Hussain, Barbara R. Conway, and Muhammad Usman Ghori. “Electrically Tunable Lens (ETL) - Based Variable Focus Imaging System for Parametric Surface Texture Analysis of Materials.” <i>Micromachines</i>. MDPI, 2022. <a href=\"https://doi.org/10.3390/mi13010017\">https://doi.org/10.3390/mi13010017</a>.","short":"J.S. Nirwan, S. Lou, S. Hussain, M. Nauman, T. Hussain, B.R. Conway, M.U. Ghori, Micromachines 13 (2022).","ieee":"J. S. Nirwan <i>et al.</i>, “Electrically tunable lens (ETL) - based variable focus imaging system for parametric surface texture analysis of materials,” <i>Micromachines</i>, vol. 13, no. 1. MDPI, 2022.","mla":"Nirwan, Jorabar Singh, et al. “Electrically Tunable Lens (ETL) - Based Variable Focus Imaging System for Parametric Surface Texture Analysis of Materials.” <i>Micromachines</i>, vol. 13, no. 1, 17, MDPI, 2022, doi:<a href=\"https://doi.org/10.3390/mi13010017\">10.3390/mi13010017</a>."},"publisher":"MDPI","publication":"Micromachines","issue":"1","article_processing_charge":"Yes","type":"journal_article","day":"01","keyword":["surface texture","electrically tunable lens","materials","hypromellose","surface topography","surface roughness","pharmaceutical tablet","variable focus imaging"],"volume":13,"file":[{"relation":"main_file","content_type":"application/pdf","file_name":"2021_Micromachines_Singh.pdf","date_created":"2022-01-03T13:43:01Z","creator":"alisjak","success":1,"date_updated":"2022-01-03T13:43:01Z","file_size":5370675,"checksum":"5d062cae3f1acb251cacb21021724c4e","file_id":"10601","access_level":"open_access"}],"publication_status":"published","status":"public","intvolume":"        13","_id":"10584","abstract":[{"lang":"eng","text":"Electrically tunable lenses (ETLs) are those with the ability to alter their optical power in response to an electric signal. This feature allows such systems to not only image the areas of interest but also obtain spatial depth perception (depth of field, DOF). The aim of the present study was to develop an ETL-based imaging system for quantitative surface analysis. Firstly, the system was calibrated to achieve high depth resolution, warranting the accurate measurement of the depth and to account for and correct any influences from external factors on the ETL. This was completed using the Tenengrad operator which effectively identified the plane of best focus as demonstrated by the linear relationship between the control current applied to the ETL and the height at which the optical system focuses. The system was then employed to measure amplitude, spatial, hybrid, and volume surface texture parameters of a model material (pharmaceutical dosage form) which were validated against the parameters obtained using a previously validated surface texture analysis technique, optical profilometry. There were no statistically significant differences between the surface texture parameters measured by the techniques, highlighting the potential application of ETL-based imaging systems as an easily adaptable and low-cost alternative surface texture analysis technique to conventional microscopy techniques"}],"article_number":"17","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"department":[{"_id":"KiMo"}],"isi":1,"doi":"10.3390/mi13010017","publication_identifier":{"eissn":["2072-666X"]},"acknowledgement":"The authors acknowledge the financial assistance provided by the University of Huddersfield.","language":[{"iso":"eng"}],"external_id":{"isi":["000758547200001"]},"month":"01","has_accepted_license":"1","oa_version":"Published Version","scopus_import":"1","ddc":["620"],"date_published":"2022-01-01T00:00:00Z","author":[{"first_name":"Jorabar Singh","full_name":"Nirwan, Jorabar Singh","last_name":"Nirwan"},{"first_name":"Shan","full_name":"Lou, Shan","last_name":"Lou"},{"first_name":"Saqib","full_name":"Hussain, Saqib","last_name":"Hussain"},{"last_name":"Nauman","id":"32c21954-2022-11eb-9d5f-af9f93c24e71","full_name":"Nauman, Muhammad","first_name":"Muhammad","orcid":"0000-0002-2111-4846"},{"full_name":"Hussain, Tariq","last_name":"Hussain","first_name":"Tariq"},{"full_name":"Conway, Barbara R.","last_name":"Conway","first_name":"Barbara R."},{"last_name":"Ghori","full_name":"Ghori, Muhammad Usman","first_name":"Muhammad Usman"}],"date_updated":"2023-08-09T10:16:10Z"},{"author":[{"last_name":"Balazs","id":"302BADF6-85FC-11EA-9E3B-B9493DDC885E","full_name":"Balazs, Daniel","first_name":"Daniel","orcid":"0000-0001-7597-043X"},{"last_name":"Erkan","full_name":"Erkan, N. Deniz","first_name":"N. Deniz"},{"first_name":"Michelle","last_name":"Quien","full_name":"Quien, Michelle"},{"first_name":"Tobias","full_name":"Hanrath, Tobias","last_name":"Hanrath"}],"date_published":"2022-05-01T00:00:00Z","date_updated":"2023-08-02T13:47:21Z","external_id":{"isi":["000735340300001"]},"language":[{"iso":"eng"}],"oa_version":"Submitted Version","scopus_import":"1","month":"05","doi":"10.1007/s12274-021-4022-7","acknowledgement":"This project was supported by the US Department of Energy through award (No. DE-SC0018026). The work was performed in part at the Cornell NanoScale Facility, a member of the National Nanotechnology Coordinated Infrastructure (NNCI), which is supported by the National Science Foundation (No. NNCI-1542081) and in part at the Cornell Center for Materials Research with funding from the NSF MRSEC program (No. DMR-1719875). The authors thank Beth Rhodes for the technical assistance with inkjet printing, and E. Peretz and Q. Wen for the early exploratory experiments.","publication_identifier":{"issn":["1998-0124"],"eissn":["1998-0000"]},"department":[{"_id":"MaIb"}],"isi":1,"publication_status":"published","main_file_link":[{"open_access":"1","url":"https://www.osti.gov/biblio/1837946"}],"intvolume":"        15","_id":"10587","abstract":[{"text":"Access to a blossoming library of colloidal nanomaterials provides building blocks for complex assembled materials. The journey to bring these prospects to fruition stands to benefit from the application of advanced processing methods. Epitaxially connected nanocrystal (or quantum dot) superlattices present a captivating model system for mesocrystals with intriguing emergent properties. The conventional processing approach to creating these materials involves assembling and attaching the constituent nanocrystals at the interface between two immiscible fluids. Processing small liquid volumes of the colloidal nanocrystal solution involves several complexities arising from the concurrent spreading, evaporation, assembly, and attachment. The ability of inkjet printers to deliver small (typically picoliter) liquid volumes with precise positioning is attractive to advance fundamental insights into the processing science, and thereby potentially enable new routes to incorporate the epitaxially connected superlattices into technology platforms. In this study, we identified the processing window of opportunity, including nanocrystal ink formulation and printing approach to enable delivery of colloidal nanocrystals from an inkjet nozzle onto the surface of a sessile droplet of the immiscible subphase. We demonstrate how inkjet printing can be scaled-down to enable the fabrication of epitaxially connected superlattices on patterned sub-millimeter droplets. We anticipate that insights from this work will spur on future advances to enable more mechanistic insights into the assembly processes and new avenues to create high-fidelity superlattices.","lang":"eng"}],"status":"public","article_processing_charge":"No","issue":"5","publication":"Nano Research","publisher":"Springer Nature","volume":15,"day":"01","page":"4536–4543","keyword":["interfacial assembly","colloidal nanocrystal","superlattice","inkjet printing"],"type":"journal_article","quality_controlled":"1","article_type":"original","date_created":"2022-01-02T23:01:34Z","year":"2022","citation":{"ama":"Balazs D, Erkan ND, Quien M, Hanrath T. Inkjet printing of epitaxially connected nanocrystal superlattices. <i>Nano Research</i>. 2022;15(5):4536–4543. doi:<a href=\"https://doi.org/10.1007/s12274-021-4022-7\">10.1007/s12274-021-4022-7</a>","ista":"Balazs D, Erkan ND, Quien M, Hanrath T. 2022. Inkjet printing of epitaxially connected nanocrystal superlattices. Nano Research. 15(5), 4536–4543.","apa":"Balazs, D., Erkan, N. D., Quien, M., &#38; Hanrath, T. (2022). Inkjet printing of epitaxially connected nanocrystal superlattices. <i>Nano Research</i>. Springer Nature. <a href=\"https://doi.org/10.1007/s12274-021-4022-7\">https://doi.org/10.1007/s12274-021-4022-7</a>","chicago":"Balazs, Daniel, N. Deniz Erkan, Michelle Quien, and Tobias Hanrath. “Inkjet Printing of Epitaxially Connected Nanocrystal Superlattices.” <i>Nano Research</i>. Springer Nature, 2022. <a href=\"https://doi.org/10.1007/s12274-021-4022-7\">https://doi.org/10.1007/s12274-021-4022-7</a>.","ieee":"D. Balazs, N. D. Erkan, M. Quien, and T. Hanrath, “Inkjet printing of epitaxially connected nanocrystal superlattices,” <i>Nano Research</i>, vol. 15, no. 5. Springer Nature, pp. 4536–4543, 2022.","short":"D. Balazs, N.D. Erkan, M. Quien, T. Hanrath, Nano Research 15 (2022) 4536–4543.","mla":"Balazs, Daniel, et al. “Inkjet Printing of Epitaxially Connected Nanocrystal Superlattices.” <i>Nano Research</i>, vol. 15, no. 5, Springer Nature, 2022, pp. 4536–4543, doi:<a href=\"https://doi.org/10.1007/s12274-021-4022-7\">10.1007/s12274-021-4022-7</a>."},"oa":1,"user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","title":"Inkjet printing of epitaxially connected nanocrystal superlattices"},{"type":"journal_article","day":"01","page":"1815-1832","keyword":["quasi curvature-dimension condition","sub-riemannian geometry","Sobolev-to-Lipschitz property","Varadhan short-time asymptotics"],"volume":384,"publisher":"Springer Nature","publication":"Mathematische Annalen","article_processing_charge":"Yes (via OA deal)","status":"public","_id":"10588","abstract":[{"lang":"eng","text":"We prove the Sobolev-to-Lipschitz property for metric measure spaces satisfying the quasi curvature-dimension condition recently introduced in Milman (Commun Pure Appl Math, to appear). We provide several applications to properties of the corresponding heat semigroup. In particular, under the additional assumption of infinitesimal Hilbertianity, we show the Varadhan short-time asymptotics for the heat semigroup with respect to the distance, and prove the irreducibility of the heat semigroup. These results apply in particular to large classes of (ideal) sub-Riemannian manifolds."}],"intvolume":"       384","arxiv":1,"file":[{"checksum":"2593abbf195e38efa93b6006b1e90eb1","file_size":410090,"file_id":"10596","access_level":"open_access","relation":"main_file","content_type":"application/pdf","file_name":"2021_MathAnn_DelloSchiavo.pdf","date_created":"2022-01-03T11:08:31Z","creator":"alisjak","success":1,"date_updated":"2022-01-03T11:08:31Z"}],"publication_status":"published","ec_funded":1,"title":"Sobolev-to-Lipschitz property on QCD- spaces and applications","file_date_updated":"2022-01-03T11:08:31Z","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","oa":1,"citation":{"ieee":"L. Dello Schiavo and K. Suzuki, “Sobolev-to-Lipschitz property on QCD- spaces and applications,” <i>Mathematische Annalen</i>, vol. 384. Springer Nature, pp. 1815–1832, 2022.","short":"L. Dello Schiavo, K. Suzuki, Mathematische Annalen 384 (2022) 1815–1832.","mla":"Dello Schiavo, Lorenzo, and Kohei Suzuki. “Sobolev-to-Lipschitz Property on QCD- Spaces and Applications.” <i>Mathematische Annalen</i>, vol. 384, Springer Nature, 2022, pp. 1815–32, doi:<a href=\"https://doi.org/10.1007/s00208-021-02331-2\">10.1007/s00208-021-02331-2</a>.","chicago":"Dello Schiavo, Lorenzo, and Kohei Suzuki. “Sobolev-to-Lipschitz Property on QCD- Spaces and Applications.” <i>Mathematische Annalen</i>. Springer Nature, 2022. <a href=\"https://doi.org/10.1007/s00208-021-02331-2\">https://doi.org/10.1007/s00208-021-02331-2</a>.","apa":"Dello Schiavo, L., &#38; Suzuki, K. (2022). Sobolev-to-Lipschitz property on QCD- spaces and applications. <i>Mathematische Annalen</i>. Springer Nature. <a href=\"https://doi.org/10.1007/s00208-021-02331-2\">https://doi.org/10.1007/s00208-021-02331-2</a>","ista":"Dello Schiavo L, Suzuki K. 2022. Sobolev-to-Lipschitz property on QCD- spaces and applications. Mathematische Annalen. 384, 1815–1832.","ama":"Dello Schiavo L, Suzuki K. Sobolev-to-Lipschitz property on QCD- spaces and applications. <i>Mathematische Annalen</i>. 2022;384:1815-1832. doi:<a href=\"https://doi.org/10.1007/s00208-021-02331-2\">10.1007/s00208-021-02331-2</a>"},"year":"2022","date_created":"2022-01-02T23:01:35Z","article_type":"original","quality_controlled":"1","corr_author":"1","month":"12","has_accepted_license":"1","scopus_import":"1","oa_version":"Published Version","language":[{"iso":"eng"}],"external_id":{"isi":["000734150200001"],"arxiv":["2110.05137"]},"project":[{"call_identifier":"H2020","_id":"256E75B8-B435-11E9-9278-68D0E5697425","name":"Optimal Transport and Stochastic Dynamics","grant_number":"716117"},{"grant_number":"F6504","_id":"fc31cba2-9c52-11eb-aca3-ff467d239cd2","name":"Taming Complexity in Partial Differential Systems"},{"name":"IST Austria Open Access Fund","_id":"B67AFEDC-15C9-11EA-A837-991A96BB2854"}],"date_updated":"2025-04-14T07:27:46Z","ddc":["510"],"date_published":"2022-12-01T00:00:00Z","author":[{"full_name":"Dello Schiavo, Lorenzo","last_name":"Dello Schiavo","id":"ECEBF480-9E4F-11EA-B557-B0823DDC885E","orcid":"0000-0002-9881-6870","first_name":"Lorenzo"},{"full_name":"Suzuki, Kohei","last_name":"Suzuki","first_name":"Kohei"}],"tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"department":[{"_id":"JaMa"}],"isi":1,"publication_identifier":{"issn":["0025-5831"],"eissn":["1432-1807"]},"acknowledgement":"The authors are grateful to Dr. Bang-Xian Han for helpful discussions on the Sobolev-to-Lipschitz property on metric measure spaces, and to Professor Kazuhiro Kuwae, Professor Emanuel Milman, Dr. Giorgio Stefani, and Dr. Gioacchino Antonelli for reading a preliminary version of this work and for their valuable comments and suggestions. Finally, they wish to express their gratitude to two anonymous Reviewers whose suggestions improved the presentation of this work.\r\n\r\nL.D.S. gratefully acknowledges funding of his position by the Austrian Science Fund (FWF) grant F65, and by the European Research Council (ERC, grant No. 716117, awarded to Prof. Dr. Jan Maas).\r\n\r\nK.S. gratefully acknowledges funding by: the JSPS Overseas Research Fellowships, Grant Nr. 290142; World Premier International Research Center Initiative (WPI), MEXT, Japan; JSPS Grant-in-Aid for Scientific Research on Innovative Areas “Discrete Geometric Analysis for Materials Design”, Grant Number 17H06465; and the Alexander von Humboldt Stiftung, Humboldt-Forschungsstipendium.","doi":"10.1007/s00208-021-02331-2"},{"citation":{"ama":"Higginbotham AP. A secret source. <i>Nature Physics</i>. 2022;18:126. doi:<a href=\"https://doi.org/10.1038/s41567-021-01459-x\">10.1038/s41567-021-01459-x</a>","ista":"Higginbotham AP. 2022. A secret source. Nature Physics. 18, 126.","apa":"Higginbotham, A. P. (2022). A secret source. <i>Nature Physics</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s41567-021-01459-x\">https://doi.org/10.1038/s41567-021-01459-x</a>","chicago":"Higginbotham, Andrew P. “A Secret Source.” <i>Nature Physics</i>. Springer Nature, 2022. <a href=\"https://doi.org/10.1038/s41567-021-01459-x\">https://doi.org/10.1038/s41567-021-01459-x</a>.","ieee":"A. P. Higginbotham, “A secret source,” <i>Nature Physics</i>, vol. 18. Springer Nature, p. 126, 2022.","mla":"Higginbotham, Andrew P. “A Secret Source.” <i>Nature Physics</i>, vol. 18, Springer Nature, 2022, p. 126, doi:<a href=\"https://doi.org/10.1038/s41567-021-01459-x\">10.1038/s41567-021-01459-x</a>.","short":"A.P. Higginbotham, Nature Physics 18 (2022) 126."},"article_type":"letter_note","quality_controlled":"1","corr_author":"1","year":"2022","date_created":"2022-01-02T23:01:35Z","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","title":"A secret source","status":"public","intvolume":"        18","_id":"10589","abstract":[{"text":"Superconducting devices ubiquitously have an excess of broken Cooper pairs, which can hamper their performance. It is widely believed that external radiation is responsible but a study now suggests there must be an additional, unknown source.","lang":"eng"}],"publication_status":"published","day":"01","page":"126","keyword":["superconducting devices","superconducting properties and materials"],"volume":18,"type":"journal_article","article_processing_charge":"No","publisher":"Springer Nature","publication":"Nature Physics","publication_identifier":{"issn":["1745-2473"],"eissn":["1745-2481"]},"doi":"10.1038/s41567-021-01459-x","isi":1,"department":[{"_id":"AnHi"}],"date_updated":"2024-10-09T21:01:21Z","author":[{"first_name":"Andrew P","orcid":"0000-0003-2607-2363","last_name":"Higginbotham","full_name":"Higginbotham, Andrew P","id":"4AD6785A-F248-11E8-B48F-1D18A9856A87"}],"date_published":"2022-02-01T00:00:00Z","scopus_import":"1","oa_version":"None","month":"02","external_id":{"isi":["000733431000007"]},"language":[{"iso":"eng"}]},{"type":"journal_article","volume":63,"keyword":["mathematical physics","statistical and nonlinear physics"],"day":"03","issue":"1","publication":"Journal of Mathematical Physics","publisher":"AIP Publishing","article_processing_charge":"No","_id":"10600","abstract":[{"lang":"eng","text":"We show that recent results on adiabatic theory for interacting gapped many-body systems on finite lattices remain valid in the thermodynamic limit. More precisely, we prove a generalized super-adiabatic theorem for the automorphism group describing the infinite volume dynamics on the quasi-local algebra of observables. The key assumption is the existence of a sequence of gapped finite volume Hamiltonians, which generates the same infinite volume dynamics in the thermodynamic limit. Our adiabatic theorem also holds for certain perturbations of gapped ground states that close the spectral gap (so it is also an adiabatic theorem for resonances and, in this sense, “generalized”), and it provides an adiabatic approximation to all orders in the adiabatic parameter (a property often called “super-adiabatic”). In addition to the existing results for finite lattices, we also perform a resummation of the adiabatic expansion and allow for observables that are not strictly local. Finally, as an application, we prove the validity of linear and higher order response theory for our class of perturbations for infinite systems. While we consider the result and its proof as new and interesting in itself, we also lay the foundation for the proof of an adiabatic theorem for systems with a gap only in the bulk, which will be presented in a follow-up article."}],"intvolume":"        63","status":"public","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2012.15238"}],"arxiv":1,"publication_status":"published","title":"Adiabatic theorem in the thermodynamic limit: Systems with a uniform gap","ec_funded":1,"user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","oa":1,"citation":{"apa":"Henheik, S. J., &#38; Teufel, S. (2022). Adiabatic theorem in the thermodynamic limit: Systems with a uniform gap. <i>Journal of Mathematical Physics</i>. AIP Publishing. <a href=\"https://doi.org/10.1063/5.0051632\">https://doi.org/10.1063/5.0051632</a>","chicago":"Henheik, Sven Joscha, and Stefan Teufel. “Adiabatic Theorem in the Thermodynamic Limit: Systems with a Uniform Gap.” <i>Journal of Mathematical Physics</i>. AIP Publishing, 2022. <a href=\"https://doi.org/10.1063/5.0051632\">https://doi.org/10.1063/5.0051632</a>.","ama":"Henheik SJ, Teufel S. Adiabatic theorem in the thermodynamic limit: Systems with a uniform gap. <i>Journal of Mathematical Physics</i>. 2022;63(1). doi:<a href=\"https://doi.org/10.1063/5.0051632\">10.1063/5.0051632</a>","ista":"Henheik SJ, Teufel S. 2022. Adiabatic theorem in the thermodynamic limit: Systems with a uniform gap. Journal of Mathematical Physics. 63(1), 011901.","mla":"Henheik, Sven Joscha, and Stefan Teufel. “Adiabatic Theorem in the Thermodynamic Limit: Systems with a Uniform Gap.” <i>Journal of Mathematical Physics</i>, vol. 63, no. 1, 011901, AIP Publishing, 2022, doi:<a href=\"https://doi.org/10.1063/5.0051632\">10.1063/5.0051632</a>.","short":"S.J. Henheik, S. Teufel, Journal of Mathematical Physics 63 (2022).","ieee":"S. J. Henheik and S. Teufel, “Adiabatic theorem in the thermodynamic limit: Systems with a uniform gap,” <i>Journal of Mathematical Physics</i>, vol. 63, no. 1. AIP Publishing, 2022."},"date_created":"2022-01-03T12:19:48Z","year":"2022","quality_controlled":"1","article_type":"original","month":"01","oa_version":"Preprint","scopus_import":"1","language":[{"iso":"eng"}],"external_id":{"isi":["000739446000009"],"arxiv":["2012.15238"]},"project":[{"grant_number":"101020331","name":"Random matrices beyond Wigner-Dyson-Mehta","call_identifier":"H2020","_id":"62796744-2b32-11ec-9570-940b20777f1d"}],"date_updated":"2025-04-14T07:57:17Z","date_published":"2022-01-03T00:00:00Z","author":[{"first_name":"Sven Joscha","orcid":"0000-0003-1106-327X","last_name":"Henheik","full_name":"Henheik, Sven Joscha","id":"31d731d7-d235-11ea-ad11-b50331c8d7fb"},{"last_name":"Teufel","full_name":"Teufel, Stefan","first_name":"Stefan"}],"department":[{"_id":"GradSch"},{"_id":"LaEr"}],"isi":1,"article_number":"011901","publication_identifier":{"eissn":["1089-7658"],"issn":["0022-2488"]},"acknowledgement":"J.H. acknowledges partial financial support from ERC Advanced Grant “RMTBeyond” No. 101020331.","doi":"10.1063/5.0051632"},{"file_date_updated":"2022-01-07T07:50:31Z","title":"Index appearance record with preorders","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","oa":1,"citation":{"chicago":"Kretinsky, Jan, Tobias Meggendorfer, Clara Waldmann, and Maximilian Weininger. “Index Appearance Record with Preorders.” <i>Acta Informatica</i>. Springer Nature, 2022. <a href=\"https://doi.org/10.1007/s00236-021-00412-y\">https://doi.org/10.1007/s00236-021-00412-y</a>.","apa":"Kretinsky, J., Meggendorfer, T., Waldmann, C., &#38; Weininger, M. (2022). Index appearance record with preorders. <i>Acta Informatica</i>. Springer Nature. <a href=\"https://doi.org/10.1007/s00236-021-00412-y\">https://doi.org/10.1007/s00236-021-00412-y</a>","ista":"Kretinsky J, Meggendorfer T, Waldmann C, Weininger M. 2022. Index appearance record with preorders. Acta Informatica. 59, 585–618.","ama":"Kretinsky J, Meggendorfer T, Waldmann C, Weininger M. Index appearance record with preorders. <i>Acta Informatica</i>. 2022;59:585-618. doi:<a href=\"https://doi.org/10.1007/s00236-021-00412-y\">10.1007/s00236-021-00412-y</a>","mla":"Kretinsky, Jan, et al. “Index Appearance Record with Preorders.” <i>Acta Informatica</i>, vol. 59, Springer Nature, 2022, pp. 585–618, doi:<a href=\"https://doi.org/10.1007/s00236-021-00412-y\">10.1007/s00236-021-00412-y</a>.","short":"J. Kretinsky, T. Meggendorfer, C. Waldmann, M. Weininger, Acta Informatica 59 (2022) 585–618.","ieee":"J. Kretinsky, T. Meggendorfer, C. Waldmann, and M. Weininger, “Index appearance record with preorders,” <i>Acta Informatica</i>, vol. 59. Springer Nature, pp. 585–618, 2022."},"date_created":"2022-01-06T12:37:27Z","year":"2022","quality_controlled":"1","corr_author":"1","article_type":"original","type":"journal_article","volume":59,"page":"585-618","keyword":["computer networks and communications","information systems","software"],"day":"01","publication":"Acta Informatica","publisher":"Springer Nature","article_processing_charge":"Yes (via OA deal)","_id":"10602","intvolume":"        59","abstract":[{"text":"Transforming ω-automata into parity automata is traditionally done using appearance records. We present an efficient variant of this idea, tailored to Rabin automata, and several optimizations applicable to all appearance records. We compare the methods experimentally and show that our method produces significantly smaller automata than previous approaches.","lang":"eng"}],"status":"public","publication_status":"published","file":[{"file_size":1066082,"checksum":"bf1c195b6aaf59e8530cf9e3a9d731f7","access_level":"open_access","file_id":"10603","file_name":"2021_ActaInfor_Křetínský.pdf","date_created":"2022-01-07T07:50:31Z","relation":"main_file","content_type":"application/pdf","date_updated":"2022-01-07T07:50:31Z","creator":"cchlebak","success":1}],"tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"isi":1,"department":[{"_id":"KrCh"}],"publication_identifier":{"issn":["0001-5903"],"eissn":["1432-0525"]},"acknowledgement":"This work is partially funded by the German Research Foundation (DFG) projects Verified Model Checkers (No. 317422601) and Statistical Unbounded Verification (No. 383882557), and the Alexander von Humboldt Foundation with funds from the German Federal Ministry of Education and Research. It is an extended version of [21], including all proofs together with further explanations and examples. Moreover, we provide a new, more efficient construction based on (total) preorders, unifying previous optimizations. Experiments are performed with a new, performant implementation, comparing our approach to the current state of the art.","doi":"10.1007/s00236-021-00412-y","month":"10","oa_version":"Published Version","scopus_import":"1","has_accepted_license":"1","language":[{"iso":"eng"}],"external_id":{"isi":["000735765500001"]},"date_updated":"2025-04-15T06:53:08Z","project":[{"_id":"B67AFEDC-15C9-11EA-A837-991A96BB2854","name":"IST Austria Open Access Fund"}],"date_published":"2022-10-01T00:00:00Z","ddc":["000"],"author":[{"full_name":"Kretinsky, Jan","id":"44CEF464-F248-11E8-B48F-1D18A9856A87","last_name":"Kretinsky","first_name":"Jan","orcid":"0000-0002-8122-2881"},{"id":"b21b0c15-30a2-11eb-80dc-f13ca25802e1","full_name":"Meggendorfer, Tobias","last_name":"Meggendorfer","first_name":"Tobias","orcid":"0000-0002-1712-2165"},{"first_name":"Clara","last_name":"Waldmann","full_name":"Waldmann, Clara"},{"last_name":"Weininger","full_name":"Weininger, Maximilian","first_name":"Maximilian"}]},{"department":[{"_id":"NiBa"}],"isi":1,"doi":"10.1002/evl3.270","publication_identifier":{"eissn":["2056-3744"]},"acknowledgement":"We thank S. O'Neill, C. Simmons, and the World Mosquito Project for providing access to unpublished data. S. Ritchie provided valuable insights into Aedes aegypti biology and the literature describing A. aegypti populations near Cairns. We thank B. Cooper for help with the figures and D. Shropshire, S. O'Neill, S. Ritchie, A. Hoffmann, B. Cooper, and members of the Cooper lab for comments on an earlier draft. Comments from three reviewers greatly improved our presentation.","language":[{"iso":"eng"}],"external_id":{"pmid":["35127140"],"isi":["000754412600008"]},"month":"02","oa_version":"Published Version","scopus_import":"1","has_accepted_license":"1","date_published":"2022-02-01T00:00:00Z","ddc":["570"],"author":[{"full_name":"Turelli, Michael","last_name":"Turelli","first_name":"Michael"},{"orcid":"0000-0002-8548-5240","first_name":"Nicholas H","last_name":"Barton","id":"4880FE40-F248-11E8-B48F-1D18A9856A87","full_name":"Barton, Nicholas H"}],"date_updated":"2025-06-11T13:45:56Z","file_date_updated":"2022-07-29T06:59:10Z","title":"Why did the Wolbachia transinfection cross the road? Drift, deterministic dynamics, and disease control","related_material":{"record":[{"status":"public","id":"11686","relation":"research_data"}]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_created":"2022-01-09T09:45:17Z","year":"2022","quality_controlled":"1","article_type":"original","oa":1,"citation":{"ama":"Turelli M, Barton NH. Why did the Wolbachia transinfection cross the road? Drift, deterministic dynamics, and disease control. <i>Evolution Letters</i>. 2022;6(1):92-105. doi:<a href=\"https://doi.org/10.1002/evl3.270\">10.1002/evl3.270</a>","ista":"Turelli M, Barton NH. 2022. Why did the Wolbachia transinfection cross the road? Drift, deterministic dynamics, and disease control. Evolution Letters. 6(1), 92–105.","apa":"Turelli, M., &#38; Barton, N. H. (2022). Why did the Wolbachia transinfection cross the road? Drift, deterministic dynamics, and disease control. <i>Evolution Letters</i>. Wiley. <a href=\"https://doi.org/10.1002/evl3.270\">https://doi.org/10.1002/evl3.270</a>","chicago":"Turelli, Michael, and Nicholas H Barton. “Why Did the Wolbachia Transinfection Cross the Road? Drift, Deterministic Dynamics, and Disease Control.” <i>Evolution Letters</i>. Wiley, 2022. <a href=\"https://doi.org/10.1002/evl3.270\">https://doi.org/10.1002/evl3.270</a>.","short":"M. Turelli, N.H. Barton, Evolution Letters 6 (2022) 92–105.","mla":"Turelli, Michael, and Nicholas H. Barton. “Why Did the Wolbachia Transinfection Cross the Road? Drift, Deterministic Dynamics, and Disease Control.” <i>Evolution Letters</i>, vol. 6, no. 1, Wiley, 2022, pp. 92–105, doi:<a href=\"https://doi.org/10.1002/evl3.270\">10.1002/evl3.270</a>.","ieee":"M. Turelli and N. H. Barton, “Why did the Wolbachia transinfection cross the road? Drift, deterministic dynamics, and disease control,” <i>Evolution Letters</i>, vol. 6, no. 1. Wiley, pp. 92–105, 2022."},"issue":"1","publication":"Evolution Letters","publisher":"Wiley","article_processing_charge":"No","type":"journal_article","volume":6,"day":"01","page":"92-105","keyword":["genetics","ecology","evolution","behavior and systematics"],"publication_status":"published","file":[{"checksum":"7e9a37e3b65b480cd7014a6a4a7e460a","file_size":2435185,"access_level":"open_access","file_id":"11689","file_name":"2022_EvolutionLetters_Turelli.pdf","date_created":"2022-07-29T06:59:10Z","relation":"main_file","content_type":"application/pdf","date_updated":"2022-07-29T06:59:10Z","creator":"dernst","success":1}],"pmid":1,"_id":"10604","intvolume":"         6","abstract":[{"text":"Maternally inherited Wolbachia transinfections are being introduced into natural mosquito populations to reduce the transmission of dengue, Zika, and other arboviruses. Wolbachia-induced cytoplasmic incompatibility provides a frequency-dependent reproductive advantage to infected females that can spread transinfections within and among populations. However, because transinfections generally reduce host fitness, they tend to spread within populations only after their frequency exceeds a critical threshold. This produces bistability with stable equilibrium frequencies at both 0 and 1, analogous to the bistability produced by underdominance between alleles or karyotypes and by population dynamics under Allee effects. Here, we analyze how stochastic frequency variation produced by finite population size can facilitate the local spread of variants with bistable dynamics into areas where invasion is unexpected from deterministic models. Our exemplar is the establishment of wMel Wolbachia in the Aedes aegypti population of Pyramid Estates (PE), a small community in far north Queensland, Australia. In 2011, wMel was stably introduced into Gordonvale, separated from PE by barriers to A. aegypti dispersal. After nearly 6 years during which wMel was observed only at low frequencies in PE, corresponding to an apparent equilibrium between immigration and selection, wMel rose to fixation by 2018. Using analytic approximations and statistical analyses, we demonstrate that the observed fixation of wMel at PE is consistent with both stochastic transition past an unstable threshold frequency and deterministic transformation produced by steady immigration at a rate just above the threshold required for deterministic invasion. The indeterminacy results from a delicate balance of parameters needed to produce the delayed transition observed. Our analyses suggest that once Wolbachia transinfections are established locally through systematic introductions, stochastic “threshold crossing” is likely to only minimally enhance spatial spread, providing a local ratchet that slightly—but systematically—aids area-wide transformation of disease-vector populations in heterogeneous landscapes.","lang":"eng"}],"status":"public"},{"author":[{"first_name":"Thomas","last_name":"Weighill","full_name":"Weighill, Thomas"},{"first_name":"Takamitsu","last_name":"Yamauchi","full_name":"Yamauchi, Takamitsu"},{"first_name":"Nicolò","orcid":"0000-0001-8686-1888","last_name":"Zava","id":"c8b3499c-7a77-11eb-b046-aa368cbbf2ad","full_name":"Zava, Nicolò"}],"date_published":"2022-03-01T00:00:00Z","ddc":["500"],"date_updated":"2024-05-22T11:10:22Z","language":[{"iso":"eng"}],"scopus_import":"1","oa_version":"Published Version","has_accepted_license":"1","month":"03","doi":"10.1007/s40879-021-00515-3","acknowledgement":"We would like to thank the referees for their careful reading and the comments that improved our work. The third named author would like to thank the Division of Mathematics, Physics and Earth Sciences of the Graduate School of Science and Engineering of Ehime University and the second named author for hosting his visit in June 2018. Open access funding provided by Institute of Science and Technology (IST Austria).","publication_identifier":{"eissn":["2199-6768"],"issn":["2199-675X"]},"tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"department":[{"_id":"HeEd"}],"publication_status":"published","file":[{"date_updated":"2024-05-22T11:10:10Z","creator":"kschuh","success":1,"date_created":"2024-05-22T11:10:10Z","file_name":"2022_EuJournalMath_Weighill.pdf","relation":"main_file","content_type":"application/pdf","access_level":"open_access","file_id":"17036","file_size":371515,"checksum":"ce35cbb2d8c889dc7750719972634ed4"}],"_id":"10608","abstract":[{"text":"We consider infinite-dimensional properties in coarse geometry for hyperspaces consisting of finite subsets of metric spaces with the Hausdorff metric. We see that several infinite-dimensional properties are preserved by taking the hyperspace of subsets with at most n points. On the other hand, we prove that, if a metric space contains a sequence of long intervals coarsely, then its hyperspace of finite subsets is not coarsely embeddable into any uniformly convex Banach space. As a corollary, the hyperspace of finite subsets of the real line is not coarsely embeddable into any uniformly convex Banach space. It is also shown that every (not necessarily bounded geometry) metric space with straight finite decomposition complexity has metric sparsification property.","lang":"eng"}],"intvolume":"         8","status":"public","article_processing_charge":"Yes (via OA deal)","issue":"1","publication":"European Journal of Mathematics","publisher":"Springer Nature","volume":8,"day":"01","page":"335-355","type":"journal_article","quality_controlled":"1","article_type":"original","date_created":"2022-01-09T23:01:27Z","year":"2022","citation":{"ieee":"T. Weighill, T. Yamauchi, and N. Zava, “Coarse infinite-dimensionality of hyperspaces of finite subsets,” <i>European Journal of Mathematics</i>, vol. 8, no. 1. Springer Nature, pp. 335–355, 2022.","short":"T. Weighill, T. Yamauchi, N. Zava, European Journal of Mathematics 8 (2022) 335–355.","mla":"Weighill, Thomas, et al. “Coarse Infinite-Dimensionality of Hyperspaces of Finite Subsets.” <i>European Journal of Mathematics</i>, vol. 8, no. 1, Springer Nature, 2022, pp. 335–55, doi:<a href=\"https://doi.org/10.1007/s40879-021-00515-3\">10.1007/s40879-021-00515-3</a>.","apa":"Weighill, T., Yamauchi, T., &#38; Zava, N. (2022). Coarse infinite-dimensionality of hyperspaces of finite subsets. <i>European Journal of Mathematics</i>. Springer Nature. <a href=\"https://doi.org/10.1007/s40879-021-00515-3\">https://doi.org/10.1007/s40879-021-00515-3</a>","chicago":"Weighill, Thomas, Takamitsu Yamauchi, and Nicolò Zava. “Coarse Infinite-Dimensionality of Hyperspaces of Finite Subsets.” <i>European Journal of Mathematics</i>. Springer Nature, 2022. <a href=\"https://doi.org/10.1007/s40879-021-00515-3\">https://doi.org/10.1007/s40879-021-00515-3</a>.","ama":"Weighill T, Yamauchi T, Zava N. Coarse infinite-dimensionality of hyperspaces of finite subsets. <i>European Journal of Mathematics</i>. 2022;8(1):335-355. doi:<a href=\"https://doi.org/10.1007/s40879-021-00515-3\">10.1007/s40879-021-00515-3</a>","ista":"Weighill T, Yamauchi T, Zava N. 2022. Coarse infinite-dimensionality of hyperspaces of finite subsets. European Journal of Mathematics. 8(1), 335–355."},"oa":1,"user_id":"3E5EF7F0-F248-11E8-B48F-1D18A9856A87","file_date_updated":"2024-05-22T11:10:10Z","title":"Coarse infinite-dimensionality of hyperspaces of finite subsets"},{"date_published":"2022-03-01T00:00:00Z","author":[{"full_name":"Windhaber, Stefan","last_name":"Windhaber","first_name":"Stefan"},{"last_name":"Xin","full_name":"Xin, Qilin","first_name":"Qilin"},{"last_name":"Uckeley","full_name":"Uckeley, Zina M.","first_name":"Zina M."},{"last_name":"Koch","full_name":"Koch, Jana","first_name":"Jana"},{"full_name":"Obr, Martin","last_name":"Obr","id":"4741CA5A-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0003-1756-6564","first_name":"Martin"},{"full_name":"Garnier, Céline","last_name":"Garnier","first_name":"Céline"},{"last_name":"Luengo-Guyonnot","full_name":"Luengo-Guyonnot, Catherine","first_name":"Catherine"},{"full_name":"Duboeuf, Maëva","last_name":"Duboeuf","first_name":"Maëva"},{"full_name":"Schur, Florian KM","last_name":"Schur","id":"48AD8942-F248-11E8-B48F-1D18A9856A87","first_name":"Florian KM","orcid":"0000-0003-4790-8078"},{"last_name":"Lozach","full_name":"Lozach, Pierre-Yves","first_name":"Pierre-Yves"}],"date_updated":"2025-04-15T08:24:49Z","project":[{"grant_number":"P31445","name":"Structural conservation and diversity in retroviral capsid","call_identifier":"FWF","_id":"26736D6A-B435-11E9-9278-68D0E5697425"}],"acknowledged_ssus":[{"_id":"EM-Fac"}],"language":[{"iso":"eng"}],"external_id":{"isi":["000779305000033"],"pmid":["35019710"]},"month":"03","scopus_import":"1","oa_version":"Published Version","doi":"10.1128/jvi.02146-21","publication_identifier":{"issn":["0022-538X"],"eissn":["1098-5514"]},"acknowledgement":"This work  was  supported  by  INRAE  starter  funds, Project IDEXLYON  (University  of  Lyon) within  the  Programme  Investissements  d’Avenir  (ANR-16-IDEX-0005),  and  FINOVIAO14 (Fondation  pour  l’Université  de  Lyon),  all  to  P.Y.L.  This  work  was  also  supported  by CellNetworks  Research  Group  funds  and  Deutsche  Forschungsgemeinschaft  (DFG)  funding (grant  numbers  LO-2338/1-1  and  LO-2338/3-1)  awarded  to  P.Y.L., Austrian  Science  Fund (FWF)  grant  P31445  to  F.K.M.S., a  Chinese  Scholarship  Council (CSC;no.  201904910701) fellowship  to   Q.X.,  and  a  ministére  de  l’enseignement  supérieur,  de  la  recherche  et  de l’innovation (MESRI) doctoral thesis grant to M.D.","article_number":"e02146-21","department":[{"_id":"FlSc"}],"isi":1,"publication_status":"published","status":"public","_id":"10639","abstract":[{"text":"With more than 80 members worldwide, the Orthobunyavirus genus in the Peribunyaviridae family is a large genus of enveloped RNA viruses, many of which are emerging pathogens in humans and livestock. How orthobunyaviruses (OBVs) penetrate and infect mammalian host cells remains poorly characterized. Here, we investigated the entry mechanisms of the OBV Germiston (GERV). Viral particles were visualized by cryo-electron microscopy and appeared roughly spherical with an average diameter of 98 nm. Labeling of the virus with fluorescent dyes did not adversely affect its infectivity and allowed the monitoring of single particles in fixed and live cells. Using this approach, we found that endocytic internalization of bound viruses was asynchronous and occurred within 30-40 min. The virus entered Rab5a+ early endosomes and, subsequently, late endosomal vacuoles containing Rab7a but not LAMP-1. Infectious entry did not require proteolytic cleavage, and endosomal acidification was sufficient and necessary for viral fusion. Acid-activated penetration began 15-25 min after initiation of virus internalization and relied on maturation of early endosomes to late endosomes. The optimal pH for viral membrane fusion was slightly below 6.0, and penetration was hampered when the potassium influx was abolished. Overall, our study provides real-time visualization of GERV entry into host cells and demonstrates the importance of late endosomal maturation in facilitating OBV penetration.","lang":"eng"}],"intvolume":"        96","pmid":1,"main_file_link":[{"open_access":"1","url":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8906410"}],"publisher":"American Society for Microbiology","issue":"5","publication":"Journal of Virology","article_processing_charge":"No","type":"journal_article","day":"01","keyword":["virology","insect science","immunology","microbiology"],"volume":96,"year":"2022","date_created":"2022-01-18T10:04:18Z","article_type":"original","quality_controlled":"1","oa":1,"citation":{"mla":"Windhaber, Stefan, et al. “The Orthobunyavirus Germiston Enters Host Cells from Late Endosomes.” <i>Journal of Virology</i>, vol. 96, no. 5, e02146-21, American Society for Microbiology, 2022, doi:<a href=\"https://doi.org/10.1128/jvi.02146-21\">10.1128/jvi.02146-21</a>.","ieee":"S. Windhaber <i>et al.</i>, “The Orthobunyavirus Germiston enters host cells from late endosomes,” <i>Journal of Virology</i>, vol. 96, no. 5. American Society for Microbiology, 2022.","short":"S. Windhaber, Q. Xin, Z.M. Uckeley, J. Koch, M. Obr, C. Garnier, C. Luengo-Guyonnot, M. Duboeuf, F.K. Schur, P.-Y. Lozach, Journal of Virology 96 (2022).","apa":"Windhaber, S., Xin, Q., Uckeley, Z. M., Koch, J., Obr, M., Garnier, C., … Lozach, P.-Y. (2022). The Orthobunyavirus Germiston enters host cells from late endosomes. <i>Journal of Virology</i>. American Society for Microbiology. <a href=\"https://doi.org/10.1128/jvi.02146-21\">https://doi.org/10.1128/jvi.02146-21</a>","chicago":"Windhaber, Stefan, Qilin Xin, Zina M. Uckeley, Jana Koch, Martin Obr, Céline Garnier, Catherine Luengo-Guyonnot, Maëva Duboeuf, Florian KM Schur, and Pierre-Yves Lozach. “The Orthobunyavirus Germiston Enters Host Cells from Late Endosomes.” <i>Journal of Virology</i>. American Society for Microbiology, 2022. <a href=\"https://doi.org/10.1128/jvi.02146-21\">https://doi.org/10.1128/jvi.02146-21</a>.","ama":"Windhaber S, Xin Q, Uckeley ZM, et al. The Orthobunyavirus Germiston enters host cells from late endosomes. <i>Journal of Virology</i>. 2022;96(5). doi:<a href=\"https://doi.org/10.1128/jvi.02146-21\">10.1128/jvi.02146-21</a>","ista":"Windhaber S, Xin Q, Uckeley ZM, Koch J, Obr M, Garnier C, Luengo-Guyonnot C, Duboeuf M, Schur FK, Lozach P-Y. 2022. The Orthobunyavirus Germiston enters host cells from late endosomes. Journal of Virology. 96(5), e02146-21."},"title":"The Orthobunyavirus Germiston enters host cells from late endosomes","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8"},{"title":"Adiabatic theorem in the thermodynamic limit: Systems with a gap in the bulk","ec_funded":1,"file_date_updated":"2022-01-19T09:27:43Z","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","oa":1,"citation":{"ieee":"S. J. Henheik and S. Teufel, “Adiabatic theorem in the thermodynamic limit: Systems with a gap in the bulk,” <i>Forum of Mathematics, Sigma</i>, vol. 10. Cambridge University Press, 2022.","mla":"Henheik, Sven Joscha, and Stefan Teufel. “Adiabatic Theorem in the Thermodynamic Limit: Systems with a Gap in the Bulk.” <i>Forum of Mathematics, Sigma</i>, vol. 10, e4, Cambridge University Press, 2022, doi:<a href=\"https://doi.org/10.1017/fms.2021.80\">10.1017/fms.2021.80</a>.","short":"S.J. Henheik, S. Teufel, Forum of Mathematics, Sigma 10 (2022).","chicago":"Henheik, Sven Joscha, and Stefan Teufel. “Adiabatic Theorem in the Thermodynamic Limit: Systems with a Gap in the Bulk.” <i>Forum of Mathematics, Sigma</i>. Cambridge University Press, 2022. <a href=\"https://doi.org/10.1017/fms.2021.80\">https://doi.org/10.1017/fms.2021.80</a>.","apa":"Henheik, S. J., &#38; Teufel, S. (2022). Adiabatic theorem in the thermodynamic limit: Systems with a gap in the bulk. <i>Forum of Mathematics, Sigma</i>. Cambridge University Press. <a href=\"https://doi.org/10.1017/fms.2021.80\">https://doi.org/10.1017/fms.2021.80</a>","ista":"Henheik SJ, Teufel S. 2022. Adiabatic theorem in the thermodynamic limit: Systems with a gap in the bulk. Forum of Mathematics, Sigma. 10, e4.","ama":"Henheik SJ, Teufel S. Adiabatic theorem in the thermodynamic limit: Systems with a gap in the bulk. <i>Forum of Mathematics, Sigma</i>. 2022;10. doi:<a href=\"https://doi.org/10.1017/fms.2021.80\">10.1017/fms.2021.80</a>"},"year":"2022","date_created":"2022-01-18T16:18:51Z","article_type":"original","corr_author":"1","quality_controlled":"1","type":"journal_article","keyword":["computational mathematics","discrete mathematics and combinatorics","geometry and topology","mathematical physics","statistics and probability","algebra and number theory","theoretical computer science","analysis"],"day":"18","volume":10,"publisher":"Cambridge University Press","publication":"Forum of Mathematics, Sigma","article_processing_charge":"Yes","status":"public","_id":"10643","intvolume":"        10","abstract":[{"text":"We prove a generalised super-adiabatic theorem for extended fermionic systems assuming a spectral gap only in the bulk. More precisely, we assume that the infinite system has a unique ground state and that the corresponding Gelfand–Naimark–Segal Hamiltonian has a spectral gap above its eigenvalue zero. Moreover, we show that a similar adiabatic theorem also holds in the bulk of finite systems up to errors that vanish faster than any inverse power of the system size, although the corresponding finite-volume Hamiltonians need not have a spectral gap.\r\n\r\n","lang":"eng"}],"arxiv":1,"file":[{"file_id":"10646","access_level":"open_access","checksum":"87592a755adcef22ea590a99dc728dd3","file_size":705323,"creator":"cchlebak","success":1,"date_updated":"2022-01-19T09:27:43Z","content_type":"application/pdf","relation":"main_file","file_name":"2022_ForumMathSigma_Henheik.pdf","date_created":"2022-01-19T09:27:43Z"}],"publication_status":"published","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"department":[{"_id":"GradSch"},{"_id":"LaEr"}],"isi":1,"article_number":"e4","publication_identifier":{"eissn":["2050-5094"]},"acknowledgement":"J.H. acknowledges partial financial support by the ERC Advanced Grant ‘RMTBeyond’ No. 101020331. Support for publication costs from the Deutsche Forschungsgemeinschaft and the Open Access Publishing Fund of the University of Tübingen is gratefully acknowledged.","doi":"10.1017/fms.2021.80","month":"01","has_accepted_license":"1","scopus_import":"1","oa_version":"Published Version","language":[{"iso":"eng"}],"external_id":{"arxiv":["2012.15239"],"isi":["000743615000001"]},"date_updated":"2025-04-14T07:57:17Z","project":[{"name":"Random matrices beyond Wigner-Dyson-Mehta","call_identifier":"H2020","_id":"62796744-2b32-11ec-9570-940b20777f1d","grant_number":"101020331"}],"ddc":["510"],"date_published":"2022-01-18T00:00:00Z","author":[{"id":"31d731d7-d235-11ea-ad11-b50331c8d7fb","last_name":"Henheik","full_name":"Henheik, Sven Joscha","orcid":"0000-0003-1106-327X","first_name":"Sven Joscha"},{"full_name":"Teufel, Stefan","last_name":"Teufel","first_name":"Stefan"}]},{"publication_status":"published","file":[{"date_updated":"2022-01-24T11:12:44Z","success":1,"creator":"cchlebak","date_created":"2022-01-24T11:12:44Z","file_name":"2022_PhysRevResearch_Hosten.pdf","relation":"main_file","content_type":"application/pdf","access_level":"open_access","file_id":"10660","checksum":"7254d267a0633ca5d63131d345e58686","file_size":236329}],"_id":"10652","intvolume":"         4","abstract":[{"text":"Finding a feasible scheme for testing the quantum mechanical nature of the gravitational interaction has been attracting an increasing level of attention. Gravity mediated entanglement generation so far appears to be the key ingredient for a potential experiment. In a recent proposal [D. Carney et al., PRX Quantum 2, 030330 (2021)] combining an atom interferometer with a low-frequency mechanical oscillator, a coherence revival test is proposed for verifying this entanglement generation. With measurements performed only on the atoms, this protocol bypasses the need for correlation measurements. Here, we explore formulations of such a protocol, and specifically find that in the envisioned regime of operation with high thermal excitation, semiclassical models, where there is no concept of entanglement, also give the same experimental signatures. We elucidate in a fully quantum mechanical calculation that entanglement is not the source of the revivals in the relevant parameter regime. We argue that, in its current form, the suggested test is only relevant if the oscillator is nearly in a pure quantum state, and in this regime the effects are too small to be measurable. We further discuss potential open ends. The results highlight the importance and subtleties of explicitly considering how the quantum case differs from the classical expectations when testing for the quantum mechanical nature of a physical system.","lang":"eng"}],"status":"public","publication":"Physical Review Research","issue":"1","publisher":"American Physical Society","article_processing_charge":"Yes (via OA deal)","type":"journal_article","volume":4,"day":"10","date_created":"2022-01-23T23:01:27Z","year":"2022","corr_author":"1","quality_controlled":"1","article_type":"original","oa":1,"citation":{"ista":"Hosten O. 2022. Constraints on probing quantum coherence to infer gravitational entanglement. Physical Review Research. 4(1), 013023.","ama":"Hosten O. Constraints on probing quantum coherence to infer gravitational entanglement. <i>Physical Review Research</i>. 2022;4(1). doi:<a href=\"https://doi.org/10.1103/PhysRevResearch.4.013023\">10.1103/PhysRevResearch.4.013023</a>","chicago":"Hosten, Onur. “Constraints on Probing Quantum Coherence to Infer Gravitational Entanglement.” <i>Physical Review Research</i>. American Physical Society, 2022. <a href=\"https://doi.org/10.1103/PhysRevResearch.4.013023\">https://doi.org/10.1103/PhysRevResearch.4.013023</a>.","apa":"Hosten, O. (2022). Constraints on probing quantum coherence to infer gravitational entanglement. <i>Physical Review Research</i>. American Physical Society. <a href=\"https://doi.org/10.1103/PhysRevResearch.4.013023\">https://doi.org/10.1103/PhysRevResearch.4.013023</a>","mla":"Hosten, Onur. “Constraints on Probing Quantum Coherence to Infer Gravitational Entanglement.” <i>Physical Review Research</i>, vol. 4, no. 1, 013023, American Physical Society, 2022, doi:<a href=\"https://doi.org/10.1103/PhysRevResearch.4.013023\">10.1103/PhysRevResearch.4.013023</a>.","ieee":"O. Hosten, “Constraints on probing quantum coherence to infer gravitational entanglement,” <i>Physical Review Research</i>, vol. 4, no. 1. American Physical Society, 2022.","short":"O. Hosten, Physical Review Research 4 (2022)."},"file_date_updated":"2022-01-24T11:12:44Z","title":"Constraints on probing quantum coherence to infer gravitational entanglement","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_published":"2022-01-10T00:00:00Z","ddc":["530"],"author":[{"last_name":"Hosten","full_name":"Hosten, Onur","id":"4C02D85E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-2031-204X","first_name":"Onur"}],"date_updated":"2024-10-09T21:01:26Z","language":[{"iso":"eng"}],"month":"01","oa_version":"Published Version","scopus_import":"1","has_accepted_license":"1","doi":"10.1103/PhysRevResearch.4.013023","publication_identifier":{"issn":["2643-1564"]},"acknowledgement":"O.H. is supported by Institute of Science and Technology Austria. The author thanks Jess Riedel for discussions.","article_number":"013023","department":[{"_id":"OnHo"}],"tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"}},{"has_accepted_license":"1","oa_version":"Published Version","scopus_import":"1","month":"01","external_id":{"isi":["000743989800040"],"pmid":["35865077"]},"language":[{"iso":"eng"}],"project":[{"grant_number":"805041","name":"Organization of CLoUdS, and implications of Tropical  cyclones and for the Energetics of the tropics, in current and waRming climate","_id":"629205d8-2b32-11ec-9570-e1356ff73576","call_identifier":"H2020"}],"date_updated":"2025-04-14T07:58:00Z","author":[{"last_name":"Abramian","full_name":"Abramian, Sophie","first_name":"Sophie"},{"first_name":"Caroline J","orcid":"0000-0001-5836-5350","full_name":"Muller, Caroline J","id":"f978ccb0-3f7f-11eb-b193-b0e2bd13182b","last_name":"Muller"},{"last_name":"Risi","full_name":"Risi, Camille","first_name":"Camille"}],"ddc":["550"],"date_published":"2022-01-16T00:00:00Z","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"department":[{"_id":"CaMu"}],"isi":1,"article_number":"e2021GL095184","acknowledgement":"The authors gratefully acknowledge funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (Project CLUSTER, Grant Agreement No. 805041), and from the PhD fellowship of Ecole Normale Supérieure de Paris-Saclay. Two supplementary movies are also provided showing the angle detection method and the squall line of the Usfc = 10 m s−1 simulation.","publication_identifier":{"eissn":["1944-8007"],"issn":["0094-8276"]},"doi":"10.1029/2021GL095184","day":"16","volume":49,"type":"journal_article","article_processing_charge":"No","publisher":"Wiley","publication":"Geophysical Research Letters","issue":"1","status":"public","_id":"10653","intvolume":"        49","abstract":[{"lang":"eng","text":"Squall lines are known to be the consequence of the interaction of low-level shear with cold pools associated with convective downdrafts. Also, as the magnitude of the shear increases beyond a critical shear, squall lines tend to orient themselves. The existing literature suggests that this orientation reduces incoming wind shear to the squall line, and maintains equilibrium between wind shear and cold pool spreading. Although this theory is widely accepted, very few quantitative studies have been conducted on supercritical regime especially. Here, we test this hypothesis with tropical squall lines obtained by imposing a vertical wind shear in cloud resolving simulations in radiative convective equilibrium. In the sub-critical regime, squall lines are perpendicular to the shear. In the super-critical regime, their orientation maintain the equilibrium, supporting existing theories. We also find that as shear increases, cold pools become more intense. However, this intensification has little impact on squall line orientation."}],"pmid":1,"file":[{"file_id":"10662","access_level":"open_access","file_size":1117408,"checksum":"08f88b57b8e409b42e382452cd5f297b","success":1,"creator":"cchlebak","date_updated":"2022-01-24T12:14:41Z","relation":"main_file","content_type":"application/pdf","file_name":"2022_GeophysResearchLet_Abramian.pdf","date_created":"2022-01-24T12:14:41Z"}],"publication_status":"published","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","related_material":{"link":[{"url":"https://doi.org/10.1002/essoar.10507697.1","relation":"earlier_version"}]},"ec_funded":1,"title":"Shear-convection interactions and orientation of tropical squall lines","file_date_updated":"2022-01-24T12:14:41Z","citation":{"ista":"Abramian S, Muller CJ, Risi C. 2022. Shear-convection interactions and orientation of tropical squall lines. Geophysical Research Letters. 49(1), e2021GL095184.","ama":"Abramian S, Muller CJ, Risi C. Shear-convection interactions and orientation of tropical squall lines. <i>Geophysical Research Letters</i>. 2022;49(1). doi:<a href=\"https://doi.org/10.1029/2021GL095184\">10.1029/2021GL095184</a>","chicago":"Abramian, Sophie, Caroline J Muller, and Camille Risi. “Shear-Convection Interactions and Orientation of Tropical Squall Lines.” <i>Geophysical Research Letters</i>. Wiley, 2022. <a href=\"https://doi.org/10.1029/2021GL095184\">https://doi.org/10.1029/2021GL095184</a>.","apa":"Abramian, S., Muller, C. J., &#38; Risi, C. (2022). Shear-convection interactions and orientation of tropical squall lines. <i>Geophysical Research Letters</i>. Wiley. <a href=\"https://doi.org/10.1029/2021GL095184\">https://doi.org/10.1029/2021GL095184</a>","mla":"Abramian, Sophie, et al. “Shear-Convection Interactions and Orientation of Tropical Squall Lines.” <i>Geophysical Research Letters</i>, vol. 49, no. 1, e2021GL095184, Wiley, 2022, doi:<a href=\"https://doi.org/10.1029/2021GL095184\">10.1029/2021GL095184</a>.","short":"S. Abramian, C.J. Muller, C. Risi, Geophysical Research Letters 49 (2022).","ieee":"S. Abramian, C. J. Muller, and C. Risi, “Shear-convection interactions and orientation of tropical squall lines,” <i>Geophysical Research Letters</i>, vol. 49, no. 1. Wiley, 2022."},"oa":1,"article_type":"original","quality_controlled":"1","year":"2022","date_created":"2022-01-23T23:01:27Z"}]