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        <identifier>oai:www.ideals.illinois.edu:2142/18227</identifier>
        <datestamp>2023-07-10</datestamp>
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        <thesis xmlns="http://www.ndltd.org/standards/metadata/etdms/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/" xsi:schemaLocation="http://www.ndltd.org/standards/metadata/etdms/1.1/ http://www.ndltd.org/standards/metadata/etdms/1.1/etdms11.xsd http://purl.org/dc/elements/1.1/ http://www.ndltd.org/standards/metadata/etdms/1.1/etdmsdc.xsd">
          <dc:contributor>Baym, Gordon A.</dc:contributor>
          <dc:contributor>Thaler, Jonathan J.</dc:contributor>
          <dc:contributor>Baym, Gordon A.</dc:contributor>
          <dc:contributor>Stone, Michael</dc:contributor>
          <dc:contributor>Hubler, Alfred W.</dc:contributor>
          <dc:creator>Kircher, Keiko I.</dc:creator>
          <dc:date>2011-01-14T22:40:34Z</dc:date>
          <dc:date>2011-01-14T22:40:34Z</dc:date>
          <dc:date>2011-01-14T22:40:34Z</dc:date>
          <dc:date>2010-12</dc:date>
          <dc:description>This thesis discusses a gas around a thermal source that emits particles with a temperature
that is high enough for the emitted particles to self-interact.
Particles emitted from a hot thermal source by means of Hawking radiation could self-
interact. With such strong interactions, the Stefan-Boltzmann law would not accurately
describe the properties of the radiation. This thesis discusses two different regions of a
strongly interacting gas around a thermal source: the region where the gas can be accurately
described by a perfect fluid in a strong gravitational field, and where the gas freezes out due
to an increasing mean free path.
Here we show that properties of radiation would change due to self-interaction of such gas,
and as the interaction weakens due to increasing mean free path of the particles, parameters
of the gas change rapidly, which indicates that the gas freezes out. The temperature of self-
interacting radiation becomes lower in both perfect fluid region and freezeout region. The
temperature measured at infinity is lower than the temperature of non-interacting radiation
approximately by a factor of two.
The result shows that a thermal source surrounded by a strongly interacting gas would
seem colder than when self-interaction of the particles is not taken into account, and that
such strongly-interacting radiation would go through a rapid change in its parameters such
as temperature and fluid velocity.</dc:description>
          <dc:description>Item withdrawn by Mark Zulauf (zulauf@illinois.edu) on 2010-08-23T13:48:02Z
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University of Illinois Theses &amp; Dissertations (ID: 1)
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          <dc:identifier>http://hdl.handle.net/2142/18227</dc:identifier>
          <dc:language>en</dc:language>
          <dc:rights>Copyright 2010 Keiko I. Kircher</dc:rights>
          <dc:subject>Freezeout</dc:subject>
          <dc:subject>Hawking Temperature</dc:subject>
          <dc:title>Radiation of strongly interacting particles by thermal sources: Violation of the Stefan-Boltzmann law</dc:title>
          <degree>
            <department>Physics</department>
            <departmentCode>1244</departmentCode>
            <discipline>Physics</discipline>
            <disciplineCode>0240</disciplineCode>
            <grantor>University of Illinois at Urbana-Champaign</grantor>
            <level>Dissertation</level>
            <name>Ph.D.</name>
            <program>PHD:Physics -UIUC</program>
            <programCode>10KS0240PHD</programCode>
          </degree>
        </thesis>
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