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<titleInfo><title>Self-regulating the early growth of black holes through global warming</title></titleInfo>


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<name type="personal">
  <namePart type="given">Zoltán</namePart>
  <namePart type="family">Haiman</namePart>
  <role><roleTerm type="text">author</roleTerm> </role><identifier type="local">7c006e8c-cc0d-11ee-8322-cb904ef76f36</identifier></name>
<name type="personal">
  <namePart type="given">Takamitsu</namePart>
  <namePart type="family">Tanaka</namePart>
  <role><roleTerm type="text">author</roleTerm> </role></name>
<name type="personal">
  <namePart type="given">Rosalba</namePart>
  <namePart type="family">Perna</namePart>
  <role><roleTerm type="text">author</roleTerm> </role></name>









<name type="conference">
  <namePart>FIRST STARS IV - From Hayashi to the Future</namePart>
</name>






<abstract lang="eng">A decade after their first discovery, the origin of giant supermassive black holes (SMBHs), with masses in excess of 109 Msolar, at redshifts as early as z &gt; 6, remains a puzzle. One possibility is that stellar-mass ``seed&apos;&apos; BHs, left behind by the first stars, accrete gas at close to the Eddington limit during a large fraction (&gt;~ 50%) of the time. While maintaining such a high accretion rate may itself be difficult, here we focus on another, less commonly discussed problem in this scenario: unless BH seed formation and growth are preferentially suppressed in less massive protogalaxies, the mass density in M~106Msolar SMBHs at z ~ 6 already exceeds the locally observed SMBH mass density by several orders of magnitude. We show that the X-rays from the earliest accreting BHs themselves can cause a self-regulation, by partially ionizing and heating the intergalactic medium (IGM). This ``global warming&apos;&apos; suppresses the formation and growth of subsequent generations of BHs in low-mass halos, and can produce excellent agreement with recent estimates of the z = 6 SMBH mass function, without impeding the growth of the largest (M&gt;~109Msolar) holes, which reside in the most massive galaxies that formed first. The proposed gravitational-wave observatory eLISA could detect several tens of major mergers between SMBHs at z &gt; 6.</abstract>

<originInfo><publisher>American Institute of Physics</publisher><dateIssued encoding="w3cdtf">2012</dateIssued><place><placeTerm type="text">Kyoto, Japan</placeTerm></place>
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<language><languageTerm authority="iso639-2b" type="code">eng</languageTerm>
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<relatedItem type="host"><titleInfo><title>AIP Conference Proceedings</title></titleInfo>
  <identifier type="issn">0094-243X</identifier><identifier type="doi">10.1063/1.4754372</identifier>
<part><detail type="volume"><number>1480</number></detail><extent unit="pages">303-308</extent>
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<bibliographicCitation>
<ama>Haiman Z, Tanaka T, Perna R. Self-regulating the early growth of black holes through global warming. In: &lt;i&gt;AIP Conference Proceedings&lt;/i&gt;. Vol 1480. American Institute of Physics; 2012:303-308. doi:&lt;a href=&quot;https://doi.org/10.1063/1.4754372&quot;&gt;10.1063/1.4754372&lt;/a&gt;</ama>
<ieee>Z. Haiman, T. Tanaka, and R. Perna, “Self-regulating the early growth of black holes through global warming,” in &lt;i&gt;AIP Conference Proceedings&lt;/i&gt;, Kyoto, Japan, 2012, vol. 1480, pp. 303–308.</ieee>
<apa>Haiman, Z., Tanaka, T., &amp;#38; Perna, R. (2012). Self-regulating the early growth of black holes through global warming. In &lt;i&gt;AIP Conference Proceedings&lt;/i&gt; (Vol. 1480, pp. 303–308). Kyoto, Japan: American Institute of Physics. &lt;a href=&quot;https://doi.org/10.1063/1.4754372&quot;&gt;https://doi.org/10.1063/1.4754372&lt;/a&gt;</apa>
<chicago>Haiman, Zoltán, Takamitsu Tanaka, and Rosalba Perna. “Self-Regulating the Early Growth of Black Holes through Global Warming.” In &lt;i&gt;AIP Conference Proceedings&lt;/i&gt;, 1480:303–8. American Institute of Physics, 2012. &lt;a href=&quot;https://doi.org/10.1063/1.4754372&quot;&gt;https://doi.org/10.1063/1.4754372&lt;/a&gt;.</chicago>
<ista>Haiman Z, Tanaka T, Perna R. 2012. Self-regulating the early growth of black holes through global warming. AIP Conference Proceedings. FIRST STARS IV - From Hayashi to the Future vol. 1480, 303–308.</ista>
<mla>Haiman, Zoltán, et al. “Self-Regulating the Early Growth of Black Holes through Global Warming.” &lt;i&gt;AIP Conference Proceedings&lt;/i&gt;, vol. 1480, American Institute of Physics, 2012, pp. 303–08, doi:&lt;a href=&quot;https://doi.org/10.1063/1.4754372&quot;&gt;10.1063/1.4754372&lt;/a&gt;.</mla>
<short>Z. Haiman, T. Tanaka, R. Perna, in:, AIP Conference Proceedings, American Institute of Physics, 2012, pp. 303–308.</short>
</bibliographicCitation>
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