@phdthesis{22684, abstract = {Contact electrification (CE) is a simple yet elusive phenomenon that occurs when two materials come into contact and separate, leaving behind net electrical charge. Despite its ubiquity, the microscopic origin of CE remains unclear. In this thesis, we investigate CE from three complementary perspectives: developing a quantitative method to measure charge at the nanoscale, exploring the dynamic behavior of charge on insulating surfaces, and uncovering the role of mechanical history in forming a triboelectric series. In the first part, we establish a rigorous framework for converting qualitative Kelvin probe force microscopy (KPFM) voltage maps into quantitative charge density distributions. Using finite element method (FEM) simulations, we determine the point-spread function of the KPFM tip–sample geometry and demonstrate that the true surface charge can be reconstructed by numerical deconvolution. This procedure enables the recovery of both the magnitude and sign of charge density with high fidelity, resolving nanoscale features that are otherwise obscured. Applying the method to contact-charged SiO$_2$ surfaces, we show that existing analytical approximations, such as parallel plate or spherical models, can miscalculate charge magnitude by orders of magnitude. Our hybrid FEM/KPFM approach therefore provides a fast and general method to convert qualitative KPFM signals into quantitative charge data, enabling nanoscale charge mapping under realistic experimental conditions. In the second part, we study the temporal stability of CE-induced charges and identify the key material factors that determine whether KPFM can capture meaningful charge patterns. Through time-resolved experiments combining a custom-built transfer system with both microscopic and macroscopic measurements, we demonstrate that only the best insulators, such as SiO$_2$, preserve CE charge long enough for stationary imaging. For less conductive polymers, such as PDMS, charge decays within the duration of a single KPFM scan due to bulk conduction. Using a simple capacitor-based model, we reproduce the observed decay dynamics and confirm that the transferred charge decays characteristic to the sample's bulk conductivity. Further, we always observe homogeneous charge transfer. In the third part, we address the question: can we form a triboelectric series with identical materials? Using controlled repetitive contact experiments, we show that nominally identical materials can progressively order themselves into a triboelectric series, where surfaces with more contact history charge negatively relative to fresher ones. By constructing a minimal model based on this ``contact bias'', we replicate the evolution from random to ordered charging observed in experiments. Supporting surface analyses, including atomic force microscopy, reveal that repeated contact induces nanoscale morphological changes, suggesting a mechanism tightly coupled to mechanical strain. These results highlight the crucial role of surface history and nanoscale mechanics in dictating charge transfer, motivating further exploration of mechanisms such as mechanochemical bond cleavage and flexoelectric polarization.}, author = {Pertl, Felix}, isbn = {978-3-99078-083-1}, issn = {2663-337X}, pages = {107}, publisher = {Institute of Science and Technology Austria}, title = {{Experimental probing of nanoscale charge features and surface morphology changes during tribocharging}}, doi = {10.15479/AT-ISTA-22684}, year = {2026}, } @article{17437, abstract = {We prove that the zero-fiber of the moment map of a totally negative quiver has rational singularities. Our proof consists in generalizing dimension bounds on jet spaces of this fiber, which were introduced by Budur. We also transfer the rational singularities property to other moduli spaces of objects in 2-Calabi-Yau categories, based on recent work of Davison. This has interesting arithmetic applications on quiver moment maps and moduli spaces of objects in 2-Calabi-Yau categories. First, we generalize results of Wyss on the asymptotic behaviour of counts of jets of quiver moment maps over finite fields. Moreover, we interpret the limit of counts of jets on a given moduli space as its p-adic volume under a canonical measure analogous to the measure built by Carocci, Orecchia and Wyss on certain moduli spaces of coherent sheaves.}, author = {Vernet, Tanguy}, issn = {1531-586X}, journal = {Transformation Groups}, pages = {1047--1083}, publisher = {Springer Nature}, title = {{Rational singularities for moment maps of totally negative quivers}}, doi = {10.1007/s00031-024-09873-0}, volume = {31}, year = {2026}, } @article{22247, abstract = {A linearly ordered (LO) k-colouring of a hypergraph is a colouring of its vertices with colours 1, …, k such that each edge contains a unique maximal colour. Deciding whether an input hypergraph admits LO k-colouring with a fixed number of colours is NP-complete (and in the special case of graphs, LO colouring coincides with the usual graph colouring). Here, we investigate the complexity of approximating the “linearly ordered chromatic number” of a hypergraph. We prove that the following promise problem is NP-complete: Given a 3-uniform hypergraph, distinguish between the case that it is LO 3-colourable, and the case that it is not even LO 4-colourable. We prove this result by a combination of algebraic, topological, and combinatorial methods, building on and extending a topological approach for studying approximate graph colouring introduced by Krokhin, Opršal, Wrochna, and Živný (2023).}, author = {Filakovský, Marek and Nakajima, Tamio Vesa and Opršal, Jakub and Tasinato, Gianluca and Wagner, Uli}, issn = {1942-3462}, journal = {ACM Transactions on Computation Theory}, keywords = {Constraint satisfaction problem, hypergraph colouring, promise problem, topological methods}, number = {2}, publisher = {Association for Computing Machinery}, title = {{Hardness of linearly ordered 4-colouring of 3-colourable 3-uniform hypergraphs}}, doi = {10.1145/3779121}, volume = {18}, year = {2026}, } @article{19860, abstract = {An eight-partition of a finite set of points (respectively, of a continuous mass distribution) in R^3 consists of three planes that divide the space into 8 octants, such that each open octant contains at most 1/8 of the points (respectively, of the mass). In 1966, Hadwiger showed that any mass distribution in R^3 admits an eight-partition; moreover, one can prescribe the normal direction of one of the three planes. The analogous result for finite point sets follows by a standard limit argument. We prove the following variant of this result: any mass distribution (or point set) in R^3 admits an eight-partition for which the intersection of two of the planes is a line with a prescribed direction. Moreover, we present an efficient algorithm for calculating an eight-partition of a set of n points in R^3 (with prescribed normal direction of one of the planes) in time O(n^7/3). A preliminary version of this work appeared in SoCG’24 (Aronov et al., 40th International Symposium on Computational Geometry, 2024).}, author = {Aronov, Boris and Basit, Abdul and Ramesh, Indu and Tasinato, Gianluca and Wagner, Uli}, issn = {1432-0444}, journal = {Discrete & Computational Geometry}, pages = {1331--1355}, publisher = {Springer Nature}, title = {{Eight-partitioning points in 3D, and efficiently too}}, doi = {10.1007/s00454-025-00739-0}, volume = {75}, year = {2026}, } @article{21763, abstract = {Reactive oxygen species (ROS) have been implicated in multiple signaling processes in plants, but the underlying mechanisms and roles remain enigmatic. In this study, we developed a method of live imaging of apoplastic ROS at the root surface. Distinct signals, including auxin, extracellular adenosine triphosphate, and rapid alkalinization factor 1 peptide, induce cytosolic calcium transients and apoplastic ROS bursts. Genetic and optogenetic manipulations of Arabidopsis identified calcium transients as necessary and sufficient for ROS bursts through activation of reduced nicotinamide adenine dinucleotide phosphate (NADPH) oxidases RBOHC and RBOHF. Apoplastic ROS bursts are not required, but they do limit gravity-induced root bending. Root bending is sensed by the stretch-activated calcium channel MCA1, leading to NADPH oxidase activation. The resulting ROS production stiffens cell walls to facilitate soil penetration. Apoplastic ROS thus provides a means to balance tissue flexibility and stiffness to navigate soil.}, author = {Kulich, Ivan and Vladimirtsev, Dmitrii and Randuch, Marek and Gao, Shiqiang and Citterico, Matteo and Konrad, Kai R. and Nagel, Georg and Wrzaczek, Michael and Cascaro, Léa and Vinet, Pauline and Durand, Pauline and Asnacios, Atef and Verma, Lokesh and Bennett, Malcolm J. and Pandey, Bipin K. and Friml, Jiří}, issn = {1095-9203}, journal = {Science}, number = {6795}, pages = {296--300}, publisher = {AAAS}, title = {{Calcium-triggered apoplastic ROS bursts balance gravity and mechanical signals for soil navigation}}, doi = {10.1126/science.adu8197}, volume = {392}, year = {2026}, } @phdthesis{23145, author = {Randuch, Marek}, issn = {2663-337X}, pages = {289}, publisher = {Institute of Science and Technology Austria}, title = {{Fast growth responses in plants: Growth regulation and phospho-proteomic }}, doi = {10.15479/AT-ISTA-23145}, year = {2026}, } @unpublished{23175, abstract = {Plants must continually balance growth with arrest, especially under stress. Auxin signaling acts as a central regulatory hub in this process, yet the mechanisms that dynamically tune early auxin signalling in real time remain unknown. Here, we used the light-gated, Ca2+-permeable Channelrhodopsin 2 variant XXM2.0 to optogenetically impose defined Ca2+ signatures on Arabidopsis root cells. Repetitive light activation triggered cytosolic Ca2+ signals that in turn suppressed auxin-induced membrane depolarization and Ca2+ transients. Moreover, prolonged optogenetic Ca2+ stimulation affects auxin-responsive transcriptional reprogramming. As phenotypic output, reversible inhibition of root growth by suppressing cell division and elongation was observed. We further identify a candidate CaM7–CNGC14 module that likely mediates Ca2+-dependent gating of early auxin signalling. Our study thus introduces a synthetic biology approach to decompose calcium–auxin crosstalk in plant cells, and demonstrates that optogenetically imposed cytosolic Ca2+ signals act as dynamic regulators of auxin susceptibility in roots.}, author = {Song, Huifang and Baudon, Angel and Freund, Matthias and Randuch, Marek and Pěnčík, Aleš and Ondřej, Novák and He, Zhaohui and Kaufmann, Kerstin and Li, Nan and Gilliham, Matthew and Friml, Jiří and Hedrich, Rainer and Huang, Shouguang}, booktitle = {bioRxiv}, title = {{Ca2+ signature gates early auxin signaling in Arabidopsis roots}}, doi = {10.1101/2025.10.04.680446}, year = {2026}, } @inproceedings{23197, abstract = {We develop a quantum theory of light-matter interactions in 229Th nanophotonic resonators pumped via the optonuclear quadrupolar effect, predicting detectable photon fluxes with realistic platforms and revealing how collective dynamics shape the future nuclear clock performance.}, author = {Mamian, Karen and De Haan, Jan and Bi, Toby and Dubey, Swadheen and Kazakov, Georgy A. and Beeks, Kjeld and Marquardt, Christoph and Kraemer, Sandro and Pereira, Lino M.C. and Del’Haye, Pascal and Van Gasse, Kasper and Schumm, Thorsten and Roques-Carmes, Charles}, booktitle = {CLEO Fundamental Science Proceedings}, isbn = {9781957171586}, location = {Long Beach, CA, United States}, publisher = {Optica Publishing Group}, title = {{Collective optonuclear cavity quantum electrodynamics in 229Th nanophotonic resonators}}, doi = {10.1364/CLEO_FS.2026.FTU1B.4}, year = {2026}, } @article{21983, abstract = {Promoters and enhancers are cis-regulatory elements (CREs), DNA sequences that bind transcription factor (TF) proteins to up- or down-regulate target genes. Decades-long efforts yielded TF-DNA interaction models that predict how strongly an individual TF binds arbitrary DNA sequences and how individual binding events on the CRE combine to affect gene expression. These insights can be synthesized into a global, biophysically realistic, and quantitative genotype–phenotype map for gene regulation, a ‘holy grail’ for the application of evolutionary theory. A global map provides a rare opportunity to simulate the long-term evolution of regulatory sequences and pose several fundamental questions: How long does it take to evolve CREs de novo? How many non-trivial regulatory functions exist in sequence space? How connected are they? For which regulatory architecture is CRE evolution most rapid and evolvable? In this article, the first of a two-part series, we briefly review the pertinent modeling and simulation efforts for a unique system that enables close, quantitative, and mechanistic links between biophysics, as well as systems, synthetic, and evolutionary biology.}, author = {Mascolo, Elia and Körei, Reka E and Herrera-Álvarez, Santiago and Guet, Calin C and Crocker, Justin and Tkačik, Gašper}, issn = {1879-0380}, journal = {Current Opinion in Genetics & Development}, publisher = {Elsevier}, title = {{Long-term evolution of regulatory DNA sequences. Part 1: Simulations on global, biophysically-realistic genotype–phenotype maps}}, doi = {10.1016/j.gde.2026.102483}, volume = {99}, year = {2026}, } @article{23198, abstract = {Small RNAs (sRNAs) are widespread across diverse flowering plant species and play important roles regulating reproduction and environmental responses. However, how sRNAs exert their function is largely unknown, likely due to their typical origin in non-genic regions, the lack of distinct gene targets, and the sparse characterization of their associated Argonaute (AGO) effector proteins. Here we show that Arabidopsis male reproductive sRNAs associate with AGO4, 5, 6 and 9, all of which are enriched in meiocytes along with RNA Polymerase V (Pol V). This enables these sRNAs to methylate loci with imperfect sequence homology. AGO4, AGO6 and AGO9 predominantly load 24-nucleotide (nt) Pol IV-derived sRNAs and mediate DNA methylation in meiocytes in a dosage-dependent manner. Despite closer homology to microRNA-associated AGO1 and AGO10, AGO5 primarily binds CLSY3- and Pol IV-derived 21-24 nt sRNAs. Transcriptomic and methylomic analyses of meiocytes from single and compound ago mutants demonstrate distinct yet complementary roles of AGO4/6/9 and AGO5 in regulating protein-coding genes and silencing transposons in the germline. These molecular disruptions are accompanied by significant meiotic defects. Together, our findings reveal how AGO4/6/9-mediated DNA methylation and AGO5, likely acting through post-transcriptional gene silencing, work together to promote male germline development.}, author = {Long, Jincheng and Yang, Chao and Xu, Shujuan and De Jaeger-Braet, Joke G and She, Wenjing and Ono, Seijiro and Walker, James and de Souza Vieira, Ygor and Schnittger, Arp and Feng, Xiaoqi}, issn = {2041-1723}, journal = {Nature Communications}, publisher = {Springer Nature}, title = {{Multiple Argonaute complexes orchestrate epigenetic silencing in the Arabidopsis germline}}, doi = {10.1038/s41467-026-77326-1}, volume = {17}, year = {2026}, } @article{23200, abstract = {We investigate the low-ionization electron density in the interstellar medium (ISM) of galaxies across 0 < z < 8, derived with the [O II] λλ3727, 3730 and [S II] λλ6718, 6733 doublets, using both deep JWST/NIRCam/grism and NIRSpec/MSA spectroscopy. Along with ancillary density samples from the literature at 0 < z < 6, we assemble three samples containing a total of 703 galaxies spanning 3.7 < z < 7.8 at 〈z〉 ∼ 5.6; 691 galaxies in the luminosity-complete NIRCam/grism programs CONGRESS and FRESCO at 〈z〉 ∼ 4.3 and ∼5.3, respectively; and 12 galaxies with high-resolution NIRSpec/MSA spectra from the GO 1871 and GLASS programs. We find median electron densities of ne[S II] = + 463 203 cm 281 3 for CONGRESS, ne[S II] = + 301 206 cm 388 3 for FRESCO, and ne[O II] = + 202 102 cm 145 3 for the NIRSpec/MSA sample. The median low-ionization ne increases from z = 0 to 4, in agreement with previous studies and those using JWST observations. However, beyond z ∼ 4 median ne begins to deviate from a monotonically increasing evolution with z. We find a positive, but shallow, correlation between O32 (a proxy for the ionization parameter) and ne, while also confirming a positive correlation between O32 and z. We suggest that these trends are possibly due to an evolving ISM gas density and ionization structure, and propose a toy model where the gas clumping evolves with z to explain the observed density and ionization variations.}, author = {Stephenson, Mabel G. and Chisholm, John and Saldana-Lopez, A. and Matthee, Jorryt J and Henry, Alaina and Naidu, Rohan P. and Flury, Sophia R. and Hutchison, Taylor A. and Finkelstein, Steven L. and Guseva, Natalia G. and Izotov, Yuri I. and Marques-Chaves, Rui and Oesch, Pascal A. and Reddy, Naveen A. and Schaerer, Daniel}, issn = {1538-4357}, journal = {The Astrophysical Journal}, number = {2}, publisher = {IOP Publishing}, title = {{The evolution of low-ionization electron densities in galaxies across cosmic epochs}}, doi = {10.3847/1538-4357/ae9eb7}, volume = {1010}, year = {2026}, } @article{23199, abstract = {The physics governing the morphology of radio-loud active galactic nucleus (AGN) jets is not fully understood. We investigate how magnetization, flickering jet power and the interplay between them affects the morphology of radio galaxies. We present a grid of relativistic magnetohydrodynamic simulations using the pluto code covering constant and variable jets with two levels of magnetization. We find that the constant high-magnetization jets can lead to highly asymmetrical cocoon morphologies, while the variable high-magnetization jet can exhibit a broken morphology, caused by a discontinuous jet beam. Our work highlights the importance of magnetization and variability on the stability and resulting morphology of radio-loud AGN jets, suggesting both are significant factors in addition to jet power or environment. Furthermore, we show that the interaction between magnetization and variability can lead to the development of localized kink instabilities along the jet beam. Finally, we discuss the effects of hydrodynamic mixing in low-magnetization jets and the role of viewing-angle dependence in comparisons between our simulations and observed sources. To facilitate this comparison we present a library of simulated radio images at different times in the simulations and from various viewing angles, which highlight a diverse set of complex morphologies.}, author = {Elley, Emma L and Matthews, James H and Whitehead, Henry William and Cooper, Alex J}, issn = {1365-2966}, journal = {Monthly Notices of the Royal Astronomical Society}, number = {4}, publisher = {Oxford University Press}, title = {{The impact of flickering variability and magnetization on the dynamics, stability, and morphology of radio-loud AGN jets}}, doi = {10.1093/mnras/stag1798}, volume = {552}, year = {2026}, } @inproceedings{23196, abstract = {We introduce an experimental realization of the measurement, processing, and generation of partially coherent light on a photonic chip. This device relies on self-configuring networks optimized sequentially to learn the coherency matrix of input light.}, author = {Mor, Paul Alexis and Kroo, Annie R. and Valdez, Carson G. and Šimić, Marko and Karnieli, Aviv and Cavicchioli, Gabriele and Sun, Zhanghao and Grimaldi, Vittorio and Fan, Shanhui and Solgaard, Olav and Miller, David A.B. and Roques-Carmes, Charles}, booktitle = {CLEO Science and Innovations Proceedings}, isbn = {9781957171586}, location = {Long Beach, CA, United States}, publisher = {Optica Publishing Group}, title = {{Variational processing of partially coherent light in a photonic integrated circuit}}, doi = {10.1364/CLEO_SI.2026.STU2F.1}, year = {2026}, } @article{23239, abstract = {Highly magnified stars at cosmological distances (z ≳ 0.7) become detectable thanks to microlensing by intracluster stars near the critical curves of galaxy clusters. Multi-epoch photometric campaigns targeting caustic crossing galaxies magnified by massive galaxy clusters enable the detection of these objects as transient events. Such stars provide unique opportunities to study stellar populations at early cosmic times, probe the nature of dark matter, reveal small-scale structure in the cluster, and improve lens models. To date, only a few dozen high-redshift stars have been reported, with a single lensed galaxy, the Dragon, holding the current record of 44 detections. These numbers, however, remain insufficient to exploit their full potential. In this paper, owing to the inclusion of new observations, we report the identification of more than 100 magnified stellar events in the Dragon, behind the massive galaxy cluster Abell 370. The relatively low redshift of the Dragon (z ≈ 0.725) facilitates the detection of its most massive stars. Using imaging data from three different cycles (2022–2024) with the James Webb Space Telescope, we applied a time-domain technique to identify flux variations associated with caustic-crossing events. From the spatial distribution of stellar events, we constrained the high-end slope of the stellar luminosity function, finding β = 2.18−0.30+0.20. Alternatively, assuming a fixed slope, we constrained the microlens surface mass density. In addition, we examined the parity asymmetry of the detected caustic-crossing events, a proposed probe of wave dark matter, and found that it remains present in our fiducial lens model. We also used the events to trace the regions of highest magnification, offering an alternative way to map the system critical curves.}, author = {Palencia, José María and Sun, Fengwu and Diego, José María and Fudamoto, Yoshinobu and Koekemoer, Anton M. and Willmer, Christopher N.A. and Iani, Edoardo and Lin, Xiaojing and Pierel, Justin D.R. and Amruth, Alfred and Bauer, Franz E. and Broadhurst, Tom and Chen, Wenlei and Dai, Liang and Espada, Daniel and Filippenko, Alexei V. and Fujimoto, Seiji and Kelly, Patrick L. and Li, Mingyu and Li, Sung Kei and Meena, Ashish Kumar and Miralda-Escudé, Jordi and Morilla, Paloma and Struble, Mitchell F. and Williams, Hayley and Windhorst, Rogier A. and Zackrison, Erick and Zhou, Ruwen and Zitrin, Adi}, issn = {1432-0746}, journal = {Astronomy & Astrophysics}, publisher = {EDP Sciences}, title = {{The first statistical study of over 100 magnified stellar events at a redshift z ≈ 0.725 with JWST}}, doi = {10.1051/0004-6361/202660640}, volume = {714}, year = {2026}, } @article{23240, abstract = {Little red dots (LRDs) are a class of sources discovered by the James Webb Space Telescope observationally defined by a V-shaped rest-frame UV-optical spectral energy distribution, a compact or unresolved morphology, and, frequently, broad hydrogen emission lines. How these characteristics translate into physical and structural properties remains unclear. Among various models, those involving a quasi-star interpret LRDs as an intermediate stage in the evolution of a super-massive black hole (SMBH) seed into a classic active galactic nucleus. In this paper, we employ the radiative-transfer code Cloudy to study whether this model is able to reproduce the spectral features commonly observed in LRDs. The model consists of an accreting SMBH (MBH ∼ 105-6 M⊙) surrounded by a convective layer where a black-body (BB) spectrum with T ∼ 5000 K and L ∼ 1044.4 erg s−1 is produced. This BB spectrum is then reprocessed by a concentric thick (∆R ∼ 1000 AU) shell of dense (nH ∼ 1011 cm−3) gas partially ionised by thermal collisions. The emerging radiation is further reprocessed by a diffuse clumpy medium surrounding the quasi-star. We fit this model to JWST/NIRSpec spectra of LRDs from the literature, deriving the main physical parameters and the SMBH masses. Once coupled with the UV emission from a host galaxy, this model is able to reproduce the shape of the UV-to-NIR continuum, including the presence of a Balmer break, as well as the luminosity of the hydrogen emission lines. However, this quasi-star model does not natively account for the presence of broad helium lines and for the possible presence of hot dust, needing additional components to match these observables. Our main result is to show how some LRDs can be modelled as quasi-stars, highlighting that a significant degeneracy exists among different LRD models. This has important consequences for our understanding of the mechanisms driving black hole growth in the early Universe.}, author = {Gentile, F. and Giavalisco, M. and Daddi, E. and Elbaz, D. and Billand, J. B. and Franco, M. and Magnelli, B. and Barro, G. and Cheng, Y. and Cleri, N. J. and Davis, K. and Delvecchio, I. and Dickinson, M. and Finkelstein, S. L. and Gandolfi, G. and Hirschmann, M. and Hu, W. and Kartaltepe, J. S. and Kocevski, D. and Koekemoer, A. M. and Lucas, R. A. and Mascia, Sara and Napolitano, L. and Papovich, C. and Pérez-Díaz, B. and Perez-Gonzalez, P. and Trump, J. R. and Wang, X. and Yung, L. Y.Aaron}, issn = {1432-0746}, journal = {Astronomy & Astrophysics}, publisher = {EDP Sciences}, title = {{The quasi-star model for little red dots: Potential and challenges}}, doi = {10.1051/0004-6361/202661289}, volume = {714}, year = {2026}, } @article{23241, abstract = {While partial coherence often degrades interference and information transfer, its correlations can be engineered to enhance imaging and optical information processing. However, approaches based on tomography and numerical reconstruction do not physically separate unknown fields into their coherence modes—that is, their orthogonal and mutually incoherent components. Here we demonstrate the separation of partially coherent light into coherence modes. We use variational processing in layered self-configuring interferometers on a silicon photonic circuit. This process finds the eigenvectors and eigenvalues of the coherency matrix, characterizing the state while leaving it intact and separated after optimization. We show that spatially orthogonal, mutually incoherent beams can be routed to separate outputs even when their intensity profiles overlap. Our experiment separates the two strongest coherence modes from a nine-input sampling of overlapping fields from two independent lasers; operation beyond two modes is verified in a rank-3 experiment. The number of physical components scales linearly with the rank r of the coherency matrix, through r in situ gradient-based optimizations enabled by electronic drive-frequency multiplexing of the phase shifters. We benchmark performance against an on-chip mixture-based tomographic method. These results establish a scalable framework for programmable coherence analysis and control.}, author = {Mor, Paul-Alexis and Kroo, Anne R. and Valdez, Carson G. and Šimić, Marko and Karnieli, Aviv and Cavicchioli, Gabriele and Sun, Zhanghao and Grimaldi, Vittorio and Fan, Shanhui and Solgaard, Olav and Miller, David A.B. and Roques-Carmes, Charles}, issn = {1749-4893}, journal = {Nature Photonics}, publisher = {Springer Nature}, title = {{Automatic on-chip separation of partially coherent light into its mutually incoherent components}}, doi = {10.1038/s41566-026-02035-6}, year = {2026}, } @article{23242, abstract = {Nanofluidic memristors promise brain-inspired information processing with ions, yet their microscopic origin remains debated. So far, ionic memory has been attributed to ion-specific interactions, dynamic wetting, chemical reactions or mechanical deformations, yet typically without direct experimental evidence. Here, by combining operando interferometric imaging with electrokinetic measurements, we directly visualize voltage-induced blistering of the confining walls of two-dimensional (2D) nanochannels as the key origin of memristive hysteresis. We identify two distinct classes of blisters: unidirectional, driven by electrostatic forces on surface charges, and bidirectional, arising from osmotic pressure due to concentration polarization. This mechanistic framework explains device evolution and device-to-device variability, and reframes stochastic blistering as a functional design element. Our results constitute a direct proof of electromechanical coupling as a robust pathway to ionic memory in 2D nanochannels and open routes towards high-performance ionic memristors and electrically actuated nanofluidic valves.}, author = {Saurav, Kalluvadi Veetil and Ronceray, Nathan and Coquinot, Baptiste and Pizarro, Agustin D. and Keerthi, Ashok and Emmerich, Theo and Radenovic, Aleksandra and Radha, Boya}, issn = {1476-4660}, journal = {Nature Materials}, publisher = {Springer Nature}, title = {{Direct imaging elucidates ionic memory in two-dimensional nanochannels}}, doi = {10.1038/s41563-026-02775-4}, year = {2026}, } @article{23235, abstract = {Modular DNA assembly based Golden Gate cloning (MoClo) is a widely used framework to assemble genetic constructs. A number of MoClo “destination vectors” have been developed, however, available options are still limited with regards to copy number and antibiotic resistance in bacteria, vector compactness, and industry researchers’ access to materials. Here, we assembled combinations of five resistance cassettes, four origins of replication and two colour markers to develop a collection of compact MoClo-compatible pCORE destination vectors. pCORE vectors support MoClo Level 1 and Level 2 assembly, and can serve as starting points for developing vectors for other hosts. We tested the performance of our vector collection in Escherichia coli, Agrobacterium tumefaciens and Saccharomyces cerevisiae. pCORE vectors are available to academia and industry under the terms of OpenMTA licence.}, author = {Gonzalez Somermeyer, Louisa and Perfilov, Maxim M. and Gao, Feng and Gorbachev, Dmitry A. and Sytov, Nikita V. and Kovalenko, Victoria and Sureda-Vives, Macià and Fleiss, Aubin and Baldominos Flores, Pilar and Yampolsky, Ilia V. and Kondrashov, Fyodor and Mishin, Alexander S. and Sarkisyan, Karen}, issn = {2045-2322}, journal = {Scientific Reports}, publisher = {Springer Nature}, title = {{pCORE, a set of open modular plasmids compatible with golden gate assembly}}, doi = {10.1038/s41598-026-66483-4}, volume = {16}, year = {2026}, } @article{23236, abstract = {A growing number of core-collapse supernovae (CCSNe) exhibit diverse light-curve morphologies that indicate strong interactions with dense, pre-existing circumstellar material (CSM). Understanding the physical origin of such CSM is essential for exploring the late-stage evolution of SN progenitors and the diversity of observed transients. Non-conservative mass transfer during binary interactions provides a promising channel for producing dense CSM before core collapse. Using the stellar evolution code MESA, we simulate post-common-envelope binaries that give rise to ultra-stripped progenitors before core collapse, and self-consistently construct the CSM from the mass loss during binary evolution. We further analytically predict the resulting bolometric and radio light curves by following the shock dynamics of SN ejecta interacting with the CSM. We find that surface-radius variations in the ultra-stripped progenitors, which reflect changes in core energy generation after a delay comparable to the thermal timescale, trigger multiple episodes of mass transfer and give rise to a variety of CSM density profiles, including detached shells and multi-peaked structures. When interacting with SN ejecta, such CSMs give rise to non-monotonic, multi-peaked optical and radio light curves that qualitatively resemble features observed in some stripped-envelope SNe. Future long-term multi-wavelength monitoring of ultra-stripped SN candidates, particularly at late times, will be crucial for probing structured CSM and constraining the long-term mass-loss history of stripped progenitors prior to core collapse. Our results suggest that SN-CSM interaction in binaries hosting ultra-stripped progenitors can provide a possible channel for producing diverse light-curve morphologies, highlighting a potential connection between the pre-SN evolution of massive binary stars and the diversity of their explosive transients.}, author = {Wei, Dandan and Schneider, Fabian R.N. and Podsiadlowski, Philipp and Moriya, Takashi J. and Laplace, Eva}, issn = {1432-0746}, journal = {Astronomy and Astrophysics}, publisher = {EDP Sciences}, title = {{Diversity of stripped-envelope supernova light curves from interactions with binary-driven circumstellar material}}, doi = {10.1051/0004-6361/202659812}, volume = {715}, year = {2026}, } @article{23237, abstract = {Context. Understanding the large-scale dynamics of molecular clouds (MCs) is crucial to constraining the processes that govern star formation and the structure and evolution of the Galaxy. While gas tracers have traditionally been used to map MC kinematics, stellar tracers such as young stellar objects (YSOs) and open clusters (OCs) provide a complementary approach that enables direct comparisons between the stellar and gaseous components. Aims. We aim to compare the kinematics of young (≤30 Myr) OCs with YSOs in the same star-forming region, the latter being assumed to trace the motions of the parent cloud gas. Subsequently, we intend to reconstruct the three-dimensional (3D) motions of the main MC complexes within 2.5 kpc of the Sun using both YSOs and young OCs as tracers. Methods. Using Gaia Data Release 3 (DR3) astrometry and complementary spectroscopic surveys providing radial velocities (RVs), we compiled a unified sample of24 146 young stars, comprising YSOs and OC members. We applied robust clustering in proper-motion space to identify co-moving YSOs and derived cloud-averaged motions via Monte Carlo sampling. These motions were compared with the kinematics inferred from OCs younger than 30 Myr. Finally, we performed orbital integrations in a realistic Galactic potential to trace the past evolution of the clouds and to quantify their expansion and rotation. Results. We derive homogeneous 3D kinematics for 15 star-forming regions within 2.5 kpc. YSOs and OCs exhibit strongly consistent kinematics within each cloud, with a median spatial velocity offset of ≲2 km s−1, allowing us to combine them into a unified tracer sample. The resulting bulk cloud motions show a median peculiar velocity of ≃9 km s−1 with respect to the Galactic rotation. We used our catalogue to trace back the Solar System’s voyage through the Orion cloud and the common origin of Lupus, Ophiuchus, and Corona Australis in the Sco-Cen region. Internally, we detected significant expansion in Orion and Ophiuchus (at a 5σ level) and coherent rotation in at least six complexes, likely reflecting local processes such as stellar feedback and angular-momentum redistribution. Conclusions. Young OCs and YSOs exhibit broadly consistent kinematics, and therefore OCs can also be used to trace the bulk motion of the star-forming regions.}, author = {Pérez-Couto, X. and Torres Rodriguez, Santiago and Miret-Roig, N. and Anders, F. and Villaver, E. and Mustill, A. J. and Manteiga, M.}, issn = {1432-0746}, journal = {Astronomy & Astrophysics}, publisher = {EDP Sciences}, title = {{A homogeneous three-dimensional view of molecular cloud kinematics out to 2.5 kpc: Using young stellar objects and open clusters as complementary tracers}}, doi = {10.1051/0004-6361/202558818}, volume = {714}, year = {2026}, }