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    <title>Recent Articles in Phys. Rev. D</title>
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    <description>Recent articles in Physical Review D</description>
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    <dc:date>2013-05-17T21:06:12-04:00</dc:date>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.094018">
    <title>Searching for the signal of dark matter and photon associated production at the LHC beyond leading order</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.094018</link>
    <description>Author(s): Fa Peng Huang, Chong Sheng Li, Jian Wang, and Ding Yu Shao&lt;br/&gt;&lt;p&gt;We study the signal of dark matter and photon associated production induced by the vector and axial-vector operators at the LHC, including the QCD next-to-leading order (NLO) effects. We find that the QCD NLO corrections reduce the dependence of the total cross sections on the factorization and reno...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 094018] Published Fri May 17, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Fa Peng Huang, Chong Sheng Li, Jian Wang, and Ding Yu Shao</p><p> We study the signal of dark matter and photon associated production induced by the vector and axial-vector operators at the LHC, including the QCD next-to-leading order (NLO) effects. We find that the QCD NLO corrections reduce the dependence of the total cross sections on the factorization and reno...</p><p>[Phys. Rev. D 87, 094018] Published Fri May 17, 2013</p>]]></content:encoded>
    <dc:title>Searching for the signal of dark matter and photon associated production at the LHC beyond leading order</dc:title>
    <dc:creator>Fa Peng Huang, Chong Sheng Li, Jian Wang, and Ding Yu Shao</dc:creator>
    <dc:date>2013-05-17T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.094018</dc:identifier>
    <dc:source>Phys. Rev. D 87, 094018 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>9</prism:number>
    <prism:publicationDate>2013-05-17T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.094018</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.094018</prism:url>
    <prism:startingPage>094018</prism:startingPage>
    <dc:subject>Strong interactions &amp; Lattice methods</dc:subject>
    <prism:section>Strong interactions &amp; Lattice methods</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.094019">
    <title>Simultaneous extraction of transversity and Collins functions from new semi-inclusive deep inelastic scattering and e^{+}e^{-} data</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.094019</link>
    <description>Author(s): M. Anselmino, M. Boglione, U. D’Alesio, S. Melis, F. Murgia, and A. Prokudin&lt;br/&gt;&lt;p&gt;We present a global reanalysis of the most recent experimental data on azimuthal asymmetries in semi-inclusive deep inelastic scattering, from the HERMES and COMPASS Collaborations, and in &lt;span style="font-style: italic;"&gt;e&lt;/span&gt;&lt;sup&gt;+&lt;/sup&gt;&lt;span style="font-style: italic;"&gt;e&lt;/span&gt;&lt;sup&gt;-&lt;/sup&gt;→&lt;span style="font-style: italic;"&gt;h&lt;/span&gt;&lt;sub&gt;1&lt;/sub&gt;&lt;span style="font-style: italic;"&gt;h&lt;/span&gt;&lt;sub&gt;2&lt;/sub&gt;&lt;span style="font-style: italic;"&gt;X&lt;/span&gt; processes, from the Belle Collaboration. The transversity and the Collins functions are extracted si...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 094019] Published Fri May 17, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): M. Anselmino, M. Boglione, U. D’Alesio, S. Melis, F. Murgia, and A. Prokudin</p><p> We present a global reanalysis of the most recent experimental data on azimuthal asymmetries in semi-inclusive deep inelastic scattering, from the HERMES and COMPASS Collaborations, and in <span style="font-style: italic;">e</span><sup>+</sup><span style="font-style: italic;">e</span><sup>-</sup>→<span style="font-style: italic;">h</span><sub>1</sub><span style="font-style: italic;">h</span><sub>2</sub><span style="font-style: italic;">X</span> processes, from the Belle Collaboration. The transversity and the Collins functions are extracted si...</p><p>[Phys. Rev. D 87, 094019] Published Fri May 17, 2013</p>]]></content:encoded>
    <dc:title>Simultaneous extraction of transversity and Collins functions from new semi-inclusive deep inelastic scattering and e^{+}e^{-} data</dc:title>
    <dc:creator>M. Anselmino, M. Boglione, U. D’Alesio, S. Melis, F. Murgia, and A. Prokudin</dc:creator>
    <dc:date>2013-05-17T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.094019</dc:identifier>
    <dc:source>Phys. Rev. D 87, 094019 (2013)</dc:source>
    <dc:type>article</dc:type>
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    <prism:number>9</prism:number>
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    <prism:doi>10.1103/PhysRevD.87.094019</prism:doi>
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    <prism:startingPage>094019</prism:startingPage>
    <dc:subject>Strong interactions &amp; Lattice methods</dc:subject>
    <prism:section>Strong interactions &amp; Lattice methods</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.096012">
    <title>Isoscalar-vector interaction and hybrid quark core in massive neutron stars</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.096012</link>
    <description>Author(s): G. Y. Shao, M. Colonna, M. Di Toro, Y. X. Liu, and B. Liu&lt;br/&gt;&lt;p&gt;The hadron-quark phase transition in the core of massive neutron stars is studied with a newly constructed two-phase model. For nuclear matter, a nonlinear Walecka type model with general nucleon-meson and meson-meson couplings, recently calibrated by Steiner, Hemper and Fischer, is taken. For quark...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 096012] Published Fri May 17, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): G. Y. Shao, M. Colonna, M. Di Toro, Y. X. Liu, and B. Liu</p><p> The hadron-quark phase transition in the core of massive neutron stars is studied with a newly constructed two-phase model. For nuclear matter, a nonlinear Walecka type model with general nucleon-meson and meson-meson couplings, recently calibrated by Steiner, Hemper and Fischer, is taken. For quark...</p><p>[Phys. Rev. D 87, 096012] Published Fri May 17, 2013</p>]]></content:encoded>
    <dc:title>Isoscalar-vector interaction and hybrid quark core in massive neutron stars</dc:title>
    <dc:creator>G. Y. Shao, M. Colonna, M. Di Toro, Y. X. Liu, and B. Liu</dc:creator>
    <dc:date>2013-05-17T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.096012</dc:identifier>
    <dc:source>Phys. Rev. D 87, 096012 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>9</prism:number>
    <prism:publicationDate>2013-05-17T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.096012</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.096012</prism:url>
    <prism:startingPage>096012</prism:startingPage>
    <dc:subject>Field theory, general methods</dc:subject>
    <prism:section>Field theory, general methods</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.102001">
    <title>Gravitational wave tests of strong field general relativity with binary inspirals: Realistic injections and optimal model selection</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.102001</link>
    <description>Author(s): Laura Sampson, Neil Cornish, and Nicolás Yunes&lt;br/&gt;&lt;p&gt;We study generic tests of strong-field general relativity using gravitational waves emitted during the inspiral of compact binaries. Previous studies have considered simple extensions to the standard post-Newtonian waveforms that differ by a single term in the phase. Here we improve on these studies...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 102001] Published Fri May 17, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Laura Sampson, Neil Cornish, and Nicolás Yunes</p><p> We study generic tests of strong-field general relativity using gravitational waves emitted during the inspiral of compact binaries. Previous studies have considered simple extensions to the standard post-Newtonian waveforms that differ by a single term in the phase. Here we improve on these studies...</p><p>[Phys. Rev. D 87, 102001] Published Fri May 17, 2013</p>]]></content:encoded>
    <dc:title>Gravitational wave tests of strong field general relativity with binary inspirals: Realistic injections and optimal model selection</dc:title>
    <dc:creator>Laura Sampson, Neil Cornish, and Nicolás Yunes</dc:creator>
    <dc:date>2013-05-17T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.102001</dc:identifier>
    <dc:source>Phys. Rev. D 87, 102001 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-17T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.102001</prism:doi>
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    <prism:startingPage>102001</prism:startingPage>
    <dc:subject>Experiment</dc:subject>
    <prism:section>Experiment</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.104019">
    <title>Relativistic effects in galaxy clustering in a parametrized post-Friedmann universe</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.104019</link>
    <description>Author(s): Lucas Lombriser, Jaiyul Yoo, and Kazuya Koyama&lt;br/&gt;&lt;p&gt;We explore the signatures of quintessence and modified gravity theories in the relativistic description of galaxy clustering within a parametrized post-Friedmann framework. For this purpose, we develop a calibration method to consistently account for horizon-scale effects in the linear parametrized ...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 104019] Published Fri May 17, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Lucas Lombriser, Jaiyul Yoo, and Kazuya Koyama</p><p> We explore the signatures of quintessence and modified gravity theories in the relativistic description of galaxy clustering within a parametrized post-Friedmann framework. For this purpose, we develop a calibration method to consistently account for horizon-scale effects in the linear parametrized ...</p><p>[Phys. Rev. D 87, 104019] Published Fri May 17, 2013</p>]]></content:encoded>
    <dc:title>Relativistic effects in galaxy clustering in a parametrized post-Friedmann universe</dc:title>
    <dc:creator>Lucas Lombriser, Jaiyul Yoo, and Kazuya Koyama</dc:creator>
    <dc:date>2013-05-17T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.104019</dc:identifier>
    <dc:source>Phys. Rev. D 87, 104019 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-17T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.104019</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.104019</prism:url>
    <prism:startingPage>104019</prism:startingPage>
    <dc:subject>General relativity, gravitation</dc:subject>
    <prism:section>General relativity, gravitation</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.105014">
    <title>Finite temperature phase diagrams of gauge theories</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.105014</link>
    <description>Author(s): Kimmo Tuominen&lt;br/&gt;&lt;p&gt;We discuss finite temperature phase diagrams of SU(N) gauge theory with massless fermions as a function of the number of fermion flavors. Inside the conformal window we find a phase boundary separating two different finite temperature phases. Below the conformal window we find different phase struct...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 105014] Published Fri May 17, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Kimmo Tuominen</p><p> We discuss finite temperature phase diagrams of SU(N) gauge theory with massless fermions as a function of the number of fermion flavors. Inside the conformal window we find a phase boundary separating two different finite temperature phases. Below the conformal window we find different phase struct...</p><p>[Phys. Rev. D 87, 105014] Published Fri May 17, 2013</p>]]></content:encoded>
    <dc:title>Finite temperature phase diagrams of gauge theories</dc:title>
    <dc:creator>Kimmo Tuominen</dc:creator>
    <dc:date>2013-05-17T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.105014</dc:identifier>
    <dc:source>Phys. Rev. D 87, 105014 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-17T10:00:00-04:00</prism:publicationDate>
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    <prism:startingPage>105014</prism:startingPage>
    <dc:subject>Field theory, formal particle theory</dc:subject>
    <prism:section>Field theory, formal particle theory</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.109902">
    <title>Publisher’s Note: Fixed points and FLRW cosmologies: Flat case [Phys. Rev. D 87, 103001 (2013)]</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.109902</link>
    <description>Author(s): Adel Awad&lt;br/&gt;[Phys. Rev. D 87, 109902] Published Fri May 17, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Adel Awad</p><p>[Phys. Rev. D 87, 109902] Published Fri May 17, 2013</p>]]></content:encoded>
    <dc:title>Publisher’s Note: Fixed points and FLRW cosmologies: Flat case [Phys. Rev. D 87, 103001 (2013)]</dc:title>
    <dc:creator>Adel Awad</dc:creator>
    <dc:date>2013-05-17T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.109902</dc:identifier>
    <dc:source>Phys. Rev. D 87, 109902 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
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    <prism:startingPage>109902</prism:startingPage>
    <dc:subject>Errata</dc:subject>
    <prism:section>Errata</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.094017">
    <title>Diffractive W^{±} production at hadron colliders as a test of color singlet exchange mechanisms</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.094017</link>
    <description>Author(s): Gunnar Ingelman, Roman Pasechnik, Johan Rathsman, and Dominik Werder&lt;br/&gt;&lt;p&gt;We revisit diffractive and exclusive &lt;span style="font-style: italic;"&gt;W&lt;/span&gt;&lt;sup&gt;±&lt;/sup&gt;&lt;span style="font-style: italic;"&gt;X&lt;/span&gt; production at hadron colliders in different models for soft color exchanges. The process &lt;span style="font-style: italic;"&gt;p&lt;/span&gt;&lt;span style="font-style: italic;"&gt;p&lt;/span&gt;→&lt;span style="font-style: italic;"&gt;p&lt;/span&gt;[&lt;span style="font-style: italic;"&gt;W&lt;/span&gt;&lt;sup&gt;±&lt;/sup&gt;&lt;span style="font-style: italic;"&gt;X&lt;/span&gt;]&lt;span style="font-style: italic;"&gt;p&lt;/span&gt;, and in particular a &lt;span style="font-style: italic;"&gt;W&lt;/span&gt;&lt;sup&gt;±&lt;/sup&gt; charge asymmetry, has been suggested as a way to discriminate diffractive processes as being due to pomeron exchange in Regge phenomeno...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 094017] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Gunnar Ingelman, Roman Pasechnik, Johan Rathsman, and Dominik Werder</p><p> We revisit diffractive and exclusive <span style="font-style: italic;">W</span><sup>±</sup><span style="font-style: italic;">X</span> production at hadron colliders in different models for soft color exchanges. The process <span style="font-style: italic;">p</span><span style="font-style: italic;">p</span>→<span style="font-style: italic;">p</span>[<span style="font-style: italic;">W</span><sup>±</sup><span style="font-style: italic;">X</span>]<span style="font-style: italic;">p</span>, and in particular a <span style="font-style: italic;">W</span><sup>±</sup> charge asymmetry, has been suggested as a way to discriminate diffractive processes as being due to pomeron exchange in Regge phenomeno...</p><p>[Phys. Rev. D 87, 094017] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Diffractive W^{±} production at hadron colliders as a test of color singlet exchange mechanisms</dc:title>
    <dc:creator>Gunnar Ingelman, Roman Pasechnik, Johan Rathsman, and Dominik Werder</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.094017</dc:identifier>
    <dc:source>Phys. Rev. D 87, 094017 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>9</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.094017</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.094017</prism:url>
    <prism:startingPage>094017</prism:startingPage>
    <dc:subject>Strong interactions &amp; Lattice methods</dc:subject>
    <prism:section>Strong interactions &amp; Lattice methods</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.095010">
    <title>Baryonic violation of R parity from anomalous U(1)_{H}</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.095010</link>
    <description>Author(s): Andres Florez, Diego Restrepo, Mauricio Velasquez, and Oscar Zapata&lt;br/&gt;&lt;p&gt;Supersymmetric scenarios with &lt;span style="font-style: italic;"&gt;R&lt;/span&gt;-parity conservation are becoming very constrained due to the lack of missing energy signals associated to heavy neutral particles, thus motivating scenarios with &lt;span style="font-style: italic;"&gt;R&lt;/span&gt;-parity violation. In view of this, we consider a supersymmetric model with &lt;span style="font-style: italic;"&gt;R&lt;/span&gt;-parity violation and extend...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 095010] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Andres Florez, Diego Restrepo, Mauricio Velasquez, and Oscar Zapata</p><p> Supersymmetric scenarios with <span style="font-style: italic;">R</span>-parity conservation are becoming very constrained due to the lack of missing energy signals associated to heavy neutral particles, thus motivating scenarios with <span style="font-style: italic;">R</span>-parity violation. In view of this, we consider a supersymmetric model with <span style="font-style: italic;">R</span>-parity violation and extend...</p><p>[Phys. Rev. D 87, 095010] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Baryonic violation of R parity from anomalous U(1)_{H}</dc:title>
    <dc:creator>Andres Florez, Diego Restrepo, Mauricio Velasquez, and Oscar Zapata</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.095010</dc:identifier>
    <dc:source>Phys. Rev. D 87, 095010 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>9</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.095010</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.095010</prism:url>
    <prism:startingPage>095010</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.096010">
    <title>Compton scattering off massive fundamental bosons of pure spin 1</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.096010</link>
    <description>Author(s): E. G. Delgado-Acosta, M. Kirchbach, M. Napsuciale, and S. Rodríguez&lt;br/&gt;&lt;p&gt;Relativistic particles with spins &lt;span style="font-style: italic;"&gt;J&lt;/span&gt;&amp;gt;0 are described by means of multicomponent wave functions which transform covariantly according to Lorentz-group representations that contain at rest the spin of interest. The symmetry group of space-time provides not one but an infinity of such representations...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 096010] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): E. G. Delgado-Acosta, M. Kirchbach, M. Napsuciale, and S. Rodríguez</p><p> Relativistic particles with spins <span style="font-style: italic;">J</span>&gt;0 are described by means of multicomponent wave functions which transform covariantly according to Lorentz-group representations that contain at rest the spin of interest. The symmetry group of space-time provides not one but an infinity of such representations...</p><p>[Phys. Rev. D 87, 096010] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Compton scattering off massive fundamental bosons of pure spin 1</dc:title>
    <dc:creator>E. G. Delgado-Acosta, M. Kirchbach, M. Napsuciale, and S. Rodríguez</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.096010</dc:identifier>
    <dc:source>Phys. Rev. D 87, 096010 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>9</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.096010</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.096010</prism:url>
    <prism:startingPage>096010</prism:startingPage>
    <dc:subject>Field theory, general methods</dc:subject>
    <prism:section>Field theory, general methods</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.096011">
    <title>Ultrasoft fermion mode and off-diagonal Boltzmann equation in a quark-gluon plasma at high temperature</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.096011</link>
    <description>Author(s): Daisuke Satow&lt;br/&gt;&lt;p&gt;We derive the generalized Boltzmann equation (GBE) near equilibrium from the Kadanoff-Baym equation for quark excitation with ultrasoft momentum (∼&lt;span style="font-style: italic;"&gt;g&lt;/span&gt;&lt;sup&gt;2&lt;/sup&gt;&lt;span style="font-style: italic;"&gt;T&lt;/span&gt;, where &lt;span style="font-style: italic;"&gt;g&lt;/span&gt; is the coupling constant and &lt;span style="font-style: italic;"&gt;T&lt;/span&gt; is the temperature) in quantum chromodynamics at extremely high &lt;span style="font-style: italic;"&gt;T&lt;/span&gt;, and show that the equation is equivalent t...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 096011] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Daisuke Satow</p><p> We derive the generalized Boltzmann equation (GBE) near equilibrium from the Kadanoff-Baym equation for quark excitation with ultrasoft momentum (∼<span style="font-style: italic;">g</span><sup>2</sup><span style="font-style: italic;">T</span>, where <span style="font-style: italic;">g</span> is the coupling constant and <span style="font-style: italic;">T</span> is the temperature) in quantum chromodynamics at extremely high <span style="font-style: italic;">T</span>, and show that the equation is equivalent t...</p><p>[Phys. Rev. D 87, 096011] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Ultrasoft fermion mode and off-diagonal Boltzmann equation in a quark-gluon plasma at high temperature</dc:title>
    <dc:creator>Daisuke Satow</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.096011</dc:identifier>
    <dc:source>Phys. Rev. D 87, 096011 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>9</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.096011</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.096011</prism:url>
    <prism:startingPage>096011</prism:startingPage>
    <dc:subject>Field theory, general methods</dc:subject>
    <prism:section>Field theory, general methods</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.101502">
    <title>Simulating extreme-mass-ratio systems in full general relativity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.101502</link>
    <description>Author(s): William E. East and Frans Pretorius&lt;br/&gt;&lt;p&gt;We introduce a new method for numerically evolving the full Einstein field equations in situations where the spacetime is dominated by a known background solution. The technique leverages the knowledge of the background solution to subtract off its contribution to the truncation error, thereby more ...&lt;/p&gt;&lt;br/&gt;&lt;img src="http://publish.aps.org/images/icons/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/&gt; &lt;br/&gt;[Phys. Rev. D 87, 101502] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): William E. East and Frans Pretorius</p><p><img src="http://publish.aps.org/images/icons/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/>  We introduce a new method for numerically evolving the full Einstein field equations in situations where the spacetime is dominated by a known background solution. The technique leverages the knowledge of the background solution to subtract off its contribution to the truncation error, thereby more ...</p><p>[Phys. Rev. D 87, 101502] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Simulating extreme-mass-ratio systems in full general relativity</dc:title>
    <dc:creator>William E. East and Frans Pretorius</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.101502</dc:identifier>
    <dc:source>Phys. Rev. D 87, 101502 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.101502</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.101502</prism:url>
    <prism:startingPage>101502</prism:startingPage>
    <dc:subject>General relativity, gravitation</dc:subject>
    <prism:section>General relativity, gravitation</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.103009">
    <title>Accretion disks around binary black holes: A simple GR-hybrid evolution model</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.103009</link>
    <description>Author(s): Stuart L. Shapiro&lt;br/&gt;&lt;p&gt;We consider a geometrically thin, Keplerian disk in the orbital plane of a binary black hole (BHBH) consisting of a spinning primary and low-mass secondary (mass ratio &lt;span style="font-style: italic;"&gt;q&lt;/span&gt;≲1). To account for the principle effects of general relativity (GR), we propose a modification of the standard Newtonian evolution...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 103009] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Stuart L. Shapiro</p><p> We consider a geometrically thin, Keplerian disk in the orbital plane of a binary black hole (BHBH) consisting of a spinning primary and low-mass secondary (mass ratio <span style="font-style: italic;">q</span>≲1). To account for the principle effects of general relativity (GR), we propose a modification of the standard Newtonian evolution...</p><p>[Phys. Rev. D 87, 103009] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Accretion disks around binary black holes: A simple GR-hybrid evolution model</dc:title>
    <dc:creator>Stuart L. Shapiro</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.103009</dc:identifier>
    <dc:source>Phys. Rev. D 87, 103009 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.103009</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.103009</prism:url>
    <prism:startingPage>103009</prism:startingPage>
    <dc:subject>Astrophysics &amp; Cosmology</dc:subject>
    <prism:section>Astrophysics &amp; Cosmology</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.103513">
    <title>Slow-roll inflation preceded by a topological defect phase à la Chaplygin gas</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.103513</link>
    <description>Author(s): Mariam Bouhmadi-López, Pisin Chen, Yu-Chien Huang, and Yu-Hsiang Lin&lt;br/&gt;&lt;p&gt;We present a simple toy model corresponding to a network of frustrated topological defects of domain walls or cosmic strings that exist previous to the standard slow-roll inflationary era of the Universe. Such a network (i) can produce a slower inflationary era than that of the standard scenario if ...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 103513] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Mariam Bouhmadi-López, Pisin Chen, Yu-Chien Huang, and Yu-Hsiang Lin</p><p> We present a simple toy model corresponding to a network of frustrated topological defects of domain walls or cosmic strings that exist previous to the standard slow-roll inflationary era of the Universe. Such a network (i) can produce a slower inflationary era than that of the standard scenario if ...</p><p>[Phys. Rev. D 87, 103513] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Slow-roll inflation preceded by a topological defect phase à la Chaplygin gas</dc:title>
    <dc:creator>Mariam Bouhmadi-López, Pisin Chen, Yu-Chien Huang, and Yu-Hsiang Lin</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.103513</dc:identifier>
    <dc:source>Phys. Rev. D 87, 103513 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.103513</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.103513</prism:url>
    <prism:startingPage>103513</prism:startingPage>
    <dc:subject>Astrophysics &amp; Cosmology</dc:subject>
    <prism:section>Astrophysics &amp; Cosmology</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.103514">
    <title>Scalar field perturbations with arbitrary potentials in quantum backgrounds</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.103514</link>
    <description>Author(s): F. T. Falciano, Nelson Pinto-Neto, and Sandro Dias Pinto Vitenti&lt;br/&gt;&lt;p&gt;In this paper it is shown how to obtain, without ever using the background classical equations of motion, a simple second order Hamiltonian involving the Mukhanov-Sasaki variable describing quantum linear scalar perturbations for the case of scalar fields with arbitrary potentials and arbitrary spac...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 103514] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): F. T. Falciano, Nelson Pinto-Neto, and Sandro Dias Pinto Vitenti</p><p> In this paper it is shown how to obtain, without ever using the background classical equations of motion, a simple second order Hamiltonian involving the Mukhanov-Sasaki variable describing quantum linear scalar perturbations for the case of scalar fields with arbitrary potentials and arbitrary spac...</p><p>[Phys. Rev. D 87, 103514] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Scalar field perturbations with arbitrary potentials in quantum backgrounds</dc:title>
    <dc:creator>F. T. Falciano, Nelson Pinto-Neto, and Sandro Dias Pinto Vitenti</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.103514</dc:identifier>
    <dc:source>Phys. Rev. D 87, 103514 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.103514</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.103514</prism:url>
    <prism:startingPage>103514</prism:startingPage>
    <dc:subject>Astrophysics &amp; Cosmology</dc:subject>
    <prism:section>Astrophysics &amp; Cosmology</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.104018">
    <title>Black holes without firewalls</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.104018</link>
    <description>Author(s): Klaus Larjo, David A. Lowe, and Larus Thorlacius&lt;br/&gt;&lt;p&gt;The postulates of black hole complementarity do not imply a firewall for infalling observers at a black hole horizon. The dynamics of the stretched horizon, that scrambles and reemits information, determines whether infalling observers experience anything out of the ordinary when entering a large bl...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 104018] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Klaus Larjo, David A. Lowe, and Larus Thorlacius</p><p> The postulates of black hole complementarity do not imply a firewall for infalling observers at a black hole horizon. The dynamics of the stretched horizon, that scrambles and reemits information, determines whether infalling observers experience anything out of the ordinary when entering a large bl...</p><p>[Phys. Rev. D 87, 104018] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Black holes without firewalls</dc:title>
    <dc:creator>Klaus Larjo, David A. Lowe, and Larus Thorlacius</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.104018</dc:identifier>
    <dc:source>Phys. Rev. D 87, 104018 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.104018</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.104018</prism:url>
    <prism:startingPage>104018</prism:startingPage>
    <dc:subject>General relativity, gravitation</dc:subject>
    <prism:section>General relativity, gravitation</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.105013">
    <title>Influence of the chameleon field potential on transition frequencies of gravitationally bound quantum states of ultracold neutrons</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.105013</link>
    <description>Author(s): A. N. Ivanov, R. Höllwieser, T. Jenke, M. Wellenzohn, and H. Abele&lt;br/&gt;&lt;p&gt;We calculate the chameleon field potential for ultracold neutrons bouncing on top of one, or between two, neutron mirrors in the gravitational field of the Earth. For the resulting nonlinear equations of motion, we give approximate analytical solutions and compare them with exact numerical ones for ...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 105013] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): A. N. Ivanov, R. Höllwieser, T. Jenke, M. Wellenzohn, and H. Abele</p><p> We calculate the chameleon field potential for ultracold neutrons bouncing on top of one, or between two, neutron mirrors in the gravitational field of the Earth. For the resulting nonlinear equations of motion, we give approximate analytical solutions and compare them with exact numerical ones for ...</p><p>[Phys. Rev. D 87, 105013] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Influence of the chameleon field potential on transition frequencies of gravitationally bound quantum states of ultracold neutrons</dc:title>
    <dc:creator>A. N. Ivanov, R. Höllwieser, T. Jenke, M. Wellenzohn, and H. Abele</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.105013</dc:identifier>
    <dc:source>Phys. Rev. D 87, 105013 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.105013</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.105013</prism:url>
    <prism:startingPage>105013</prism:startingPage>
    <dc:subject>Field theory, formal particle theory</dc:subject>
    <prism:section>Field theory, formal particle theory</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.106006">
    <title>Extremal surfaces in asymptotically AdS charged boson stars backgrounds</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.106006</link>
    <description>Author(s): Fernando Nogueira&lt;br/&gt;&lt;p&gt;In this paper, inspired by the holographic dual of the entanglement entropy, we consider the behavior of extremal, codimension two, spacelike surfaces in the background of three and four dimensional charged boson stars in asymptotically anti-de Sitter spacetime. We find conditions for which families...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 106006] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Fernando Nogueira</p><p> In this paper, inspired by the holographic dual of the entanglement entropy, we consider the behavior of extremal, codimension two, spacelike surfaces in the background of three and four dimensional charged boson stars in asymptotically anti-de Sitter spacetime. We find conditions for which families...</p><p>[Phys. Rev. D 87, 106006] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Extremal surfaces in asymptotically AdS charged boson stars backgrounds</dc:title>
    <dc:creator>Fernando Nogueira</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.106006</dc:identifier>
    <dc:source>Phys. Rev. D 87, 106006 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.106006</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.106006</prism:url>
    <prism:startingPage>106006</prism:startingPage>
    <dc:subject>String theory</dc:subject>
    <prism:section>String theory</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.107503">
    <title>Primordial tensor power spectrum in holonomy corrected Ω loop quantum cosmology</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.107503</link>
    <description>Author(s): Linda Linsefors, Thomas Cailleteau, Aurelien Barrau, and Julien Grain&lt;br/&gt;&lt;p&gt;The holonomy correction is one of the main terms arising when implementing loop quantum gravity ideas at an effective level in cosmology. The recent construction of an anomaly-free algebra has shown that the formalism used, up to now, to derive the primordial spectrum of fluctuations was not correct...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 107503] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Linda Linsefors, Thomas Cailleteau, Aurelien Barrau, and Julien Grain</p><p> The holonomy correction is one of the main terms arising when implementing loop quantum gravity ideas at an effective level in cosmology. The recent construction of an anomaly-free algebra has shown that the formalism used, up to now, to derive the primordial spectrum of fluctuations was not correct...</p><p>[Phys. Rev. D 87, 107503] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Primordial tensor power spectrum in holonomy corrected Ω loop quantum cosmology</dc:title>
    <dc:creator>Linda Linsefors, Thomas Cailleteau, Aurelien Barrau, and Julien Grain</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.107503</dc:identifier>
    <dc:source>Phys. Rev. D 87, 107503 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.107503</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.107503</prism:url>
    <prism:startingPage>107503</prism:startingPage>
    <dc:subject>General relativity, gravitation</dc:subject>
    <prism:section>General relativity, gravitation</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.094015">
    <title>Baryonic Isgur-Wise functions in large-N_{c} heavy quark effective theory</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.094015</link>
    <description>Author(s): Ming-Kai Du and Chun Liu&lt;br/&gt;&lt;p&gt;Large-&lt;span style="font-style: italic;"&gt;N&lt;/span&gt;&lt;sub&gt;&lt;span style="font-style: italic;"&gt;c&lt;/span&gt;&lt;/sub&gt; relations among baryonic Isgur-Wise functions appearing at the order of 1/&lt;span style="font-style: italic;"&gt;m&lt;/span&gt;&lt;sub&gt;&lt;span style="font-style: italic;"&gt;Q&lt;/span&gt;&lt;/sub&gt; are analyzed. An application to &lt;span style="font-style: italic;"&gt;Ω&lt;/span&gt;&lt;sub&gt;&lt;span style="font-style: italic;"&gt;b&lt;/span&gt;&lt;/sub&gt;→&lt;span style="font-style: italic;"&gt;Ω&lt;/span&gt;&lt;sub&gt;&lt;span style="font-style: italic;"&gt;c&lt;/span&gt;&lt;/sub&gt; weak decays is given.&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 094015] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Ming-Kai Du and Chun Liu</p><p> Large-<span style="font-style: italic;">N</span><sub><span style="font-style: italic;">c</span></sub> relations among baryonic Isgur-Wise functions appearing at the order of 1/<span style="font-style: italic;">m</span><sub><span style="font-style: italic;">Q</span></sub> are analyzed. An application to <span style="font-style: italic;">Ω</span><sub><span style="font-style: italic;">b</span></sub>→<span style="font-style: italic;">Ω</span><sub><span style="font-style: italic;">c</span></sub> weak decays is given.</p><p>[Phys. Rev. D 87, 094015] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Baryonic Isgur-Wise functions in large-N_{c} heavy quark effective theory</dc:title>
    <dc:creator>Ming-Kai Du and Chun Liu</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.094015</dc:identifier>
    <dc:source>Phys. Rev. D 87, 094015 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>9</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.094015</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.094015</prism:url>
    <prism:startingPage>094015</prism:startingPage>
    <dc:subject>Strong interactions &amp; Lattice methods</dc:subject>
    <prism:section>Strong interactions &amp; Lattice methods</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.094016">
    <title>Top quark physics in the vector color-octet model</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.094016</link>
    <description>Author(s): Sukanta Dutta, Ashok Goyal, and Mukesh Kumar&lt;br/&gt;&lt;p&gt;We study and constrain the parameter space of the vector color-octet model from the observed data at the Tevatron by studying the top quark pair production and associated observables &lt;span style="font-style: italic;"&gt;A&lt;/span&gt;&lt;sub&gt;FB&lt;/sub&gt;&lt;sup&gt;&lt;span style="font-style: italic;"&gt;t&lt;/span&gt;&lt;span style="font-style: italic;"&gt;t&lt;/span&gt;̅        &lt;/sup&gt; and spin correlation. In particular we study the invariant mass and rapidity dependence of &lt;span style="font-style: italic;"&gt;A&lt;/span&gt;&lt;sub&gt;FB&lt;/sub&gt;&lt;sup&gt;&lt;span style="font-style: italic;"&gt;t&lt;/span&gt;&lt;span style="font-style: italic;"&gt;t&lt;/span&gt;̅     ...&lt;/sup&gt;&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 094016] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Sukanta Dutta, Ashok Goyal, and Mukesh Kumar</p><p> We study and constrain the parameter space of the vector color-octet model from the observed data at the Tevatron by studying the top quark pair production and associated observables <span style="font-style: italic;">A</span><sub>FB</sub><sup><span style="font-style: italic;">t</span><span style="font-style: italic;">t</span>̅        </sup> and spin correlation. In particular we study the invariant mass and rapidity dependence of <span style="font-style: italic;">A</span><sub>FB</sub><sup><span style="font-style: italic;">t</span><span style="font-style: italic;">t</span>̅     ...</sup></p><p>[Phys. Rev. D 87, 094016] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Top quark physics in the vector color-octet model</dc:title>
    <dc:creator>Sukanta Dutta, Ashok Goyal, and Mukesh Kumar</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.094016</dc:identifier>
    <dc:source>Phys. Rev. D 87, 094016 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>9</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.094016</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.094016</prism:url>
    <prism:startingPage>094016</prism:startingPage>
    <dc:subject>Strong interactions &amp; Lattice methods</dc:subject>
    <prism:section>Strong interactions &amp; Lattice methods</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.094506">
    <title>Structure and flow of the nucleon eigenstates in lattice QCD</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.094506</link>
    <description>Author(s): M. Selim Mahbub, Waseem Kamleh, Derek B. Leinweber, Peter J. Moran, and Anthony G. Williams&lt;br/&gt;&lt;p&gt;A determination of the excited energy eigenstates of the nucleon, &lt;span style="font-style: italic;"&gt;s&lt;/span&gt;=1/2, &lt;span style="font-style: italic;"&gt;I&lt;/span&gt;=1/2, &lt;span style="font-style: italic;"&gt;N&lt;/span&gt;&lt;sup&gt;±&lt;/sup&gt;, is presented in full QCD using 2+1 flavor PACS-CS gauge configurations. The correlation-matrix method is used and is built using standard nucleon interpolators employing smearings at the fermion sources and sinks. We...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 094506] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): M. Selim Mahbub, Waseem Kamleh, Derek B. Leinweber, Peter J. Moran, and Anthony G. Williams</p><p> A determination of the excited energy eigenstates of the nucleon, <span style="font-style: italic;">s</span>=1/2, <span style="font-style: italic;">I</span>=1/2, <span style="font-style: italic;">N</span><sup>±</sup>, is presented in full QCD using 2+1 flavor PACS-CS gauge configurations. The correlation-matrix method is used and is built using standard nucleon interpolators employing smearings at the fermion sources and sinks. We...</p><p>[Phys. Rev. D 87, 094506] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Structure and flow of the nucleon eigenstates in lattice QCD</dc:title>
    <dc:creator>M. Selim Mahbub, Waseem Kamleh, Derek B. Leinweber, Peter J. Moran, and Anthony G. Williams</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.094506</dc:identifier>
    <dc:source>Phys. Rev. D 87, 094506 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>9</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.094506</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.094506</prism:url>
    <prism:startingPage>094506</prism:startingPage>
    <dc:subject>Strong interactions &amp; Lattice methods</dc:subject>
    <prism:section>Strong interactions &amp; Lattice methods</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.095009">
    <title>Effects of Planck scale physics on neutrino mixing parameters in left-right symmetric models</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.095009</link>
    <description>Author(s): Debasish Borah&lt;br/&gt;&lt;p&gt;Left-right symmetric models (LRSM) are extensions of the standard model by an enlarged gauge group &lt;span style="font-style: italic;"&gt;S&lt;/span&gt;&lt;span style="font-style: italic;"&gt;U&lt;/span&gt;(2)&lt;sub&gt;&lt;span style="font-style: italic;"&gt;L&lt;/span&gt;&lt;/sub&gt;×&lt;span style="font-style: italic;"&gt;S&lt;/span&gt;&lt;span style="font-style: italic;"&gt;U&lt;/span&gt;(2)&lt;sub&gt;&lt;span style="font-style: italic;"&gt;R&lt;/span&gt;&lt;/sub&gt;×&lt;span style="font-style: italic;"&gt;U&lt;/span&gt;(1)&lt;sub&gt;&lt;span style="font-style: italic;"&gt;B&lt;/span&gt;-&lt;span style="font-style: italic;"&gt;L&lt;/span&gt;,&lt;/sub&gt; where automatic inclusion of right-handed fermions as &lt;span style="font-style: italic;"&gt;S&lt;/span&gt;&lt;span style="font-style: italic;"&gt;U&lt;/span&gt;(2)&lt;sub&gt;&lt;span style="font-style: italic;"&gt;R&lt;/span&gt;&lt;/sub&gt; doublets guarantees a natural seesaw origin of neutrino masses. Apart from the extended gauge symmetry, LRSM also has...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 095009] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Debasish Borah</p><p> Left-right symmetric models (LRSM) are extensions of the standard model by an enlarged gauge group <span style="font-style: italic;">S</span><span style="font-style: italic;">U</span>(2)<sub><span style="font-style: italic;">L</span></sub>×<span style="font-style: italic;">S</span><span style="font-style: italic;">U</span>(2)<sub><span style="font-style: italic;">R</span></sub>×<span style="font-style: italic;">U</span>(1)<sub><span style="font-style: italic;">B</span>-<span style="font-style: italic;">L</span>,</sub> where automatic inclusion of right-handed fermions as <span style="font-style: italic;">S</span><span style="font-style: italic;">U</span>(2)<sub><span style="font-style: italic;">R</span></sub> doublets guarantees a natural seesaw origin of neutrino masses. Apart from the extended gauge symmetry, LRSM also has...</p><p>[Phys. Rev. D 87, 095009] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Effects of Planck scale physics on neutrino mixing parameters in left-right symmetric models</dc:title>
    <dc:creator>Debasish Borah</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.095009</dc:identifier>
    <dc:source>Phys. Rev. D 87, 095009 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>9</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.095009</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.095009</prism:url>
    <prism:startingPage>095009</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.103008">
    <title>Detecting long-duration narrow-band gravitational wave transients associated with soft gamma repeater quasiperiodic oscillations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.103008</link>
    <description>Author(s): David Murphy, Maggie Tse, Peter Raffai, Imre Bartos, Rubab Khan, Zsuzsa Márka, Luca Matone, Keith Redwine, and Szabolcs Márka&lt;br/&gt;&lt;p&gt;We have performed an in-depth concept study of a gravitational wave data analysis method which targets repeated long quasimonochromatic transients (triggers) from cosmic sources. The algorithm concept can be applied to multitrigger data sets in which the detector-source orientation and the statistic...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 103008] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): David Murphy, Maggie Tse, Peter Raffai, Imre Bartos, Rubab Khan, Zsuzsa Márka, Luca Matone, Keith Redwine, and Szabolcs Márka</p><p> We have performed an in-depth concept study of a gravitational wave data analysis method which targets repeated long quasimonochromatic transients (triggers) from cosmic sources. The algorithm concept can be applied to multitrigger data sets in which the detector-source orientation and the statistic...</p><p>[Phys. Rev. D 87, 103008] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Detecting long-duration narrow-band gravitational wave transients associated with soft gamma repeater quasiperiodic oscillations</dc:title>
    <dc:creator>David Murphy, Maggie Tse, Peter Raffai, Imre Bartos, Rubab Khan, Zsuzsa Márka, Luca Matone, Keith Redwine, and Szabolcs Márka</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.103008</dc:identifier>
    <dc:source>Phys. Rev. D 87, 103008 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.103008</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.103008</prism:url>
    <prism:startingPage>103008</prism:startingPage>
    <dc:subject>Astrophysics &amp; Cosmology</dc:subject>
    <prism:section>Astrophysics &amp; Cosmology</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.103508">
    <title>Cosmic microwave background constraints on dark matter models of the Galactic center 511 keV signal</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.103508</link>
    <description>Author(s): Andrew R. Frey and Nicholas B. Reid&lt;br/&gt;&lt;p&gt;The high positron production rate required to explain the flux of 511 keV gamma rays from the Galactic center has inspired many models in which dark matter creates positrons. These models include the annihilation of light dark matter and the scattering of dark matter with excited states (exciting da...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 103508] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Andrew R. Frey and Nicholas B. Reid</p><p> The high positron production rate required to explain the flux of 511 keV gamma rays from the Galactic center has inspired many models in which dark matter creates positrons. These models include the annihilation of light dark matter and the scattering of dark matter with excited states (exciting da...</p><p>[Phys. Rev. D 87, 103508] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Cosmic microwave background constraints on dark matter models of the Galactic center 511 keV signal</dc:title>
    <dc:creator>Andrew R. Frey and Nicholas B. Reid</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.103508</dc:identifier>
    <dc:source>Phys. Rev. D 87, 103508 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.103508</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.103508</prism:url>
    <prism:startingPage>103508</prism:startingPage>
    <dc:subject>Astrophysics &amp; Cosmology</dc:subject>
    <prism:section>Astrophysics &amp; Cosmology</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.103509">
    <title>130 GeV gamma-ray line and generic dark matter model building constraints from continuum gamma rays, radio, and antiproton data</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.103509</link>
    <description>Author(s): Masaki Asano, Torsten Bringmann, Günter Sigl, and Martin Vollmann&lt;br/&gt;&lt;p&gt;An analysis of the Fermi gamma-ray space telescope data has recently revealed a resolved gamma-ray feature close to the galactic center which is consistent with monochromatic photons at an energy of about 130 GeV. If interpreted in terms of dark matter (DM) annihilating into &lt;span style="font-style: italic;"&gt;γ&lt;/span&gt;&lt;span style="font-style: italic;"&gt;γ&lt;/span&gt; (&lt;span style="font-style: italic;"&gt;γ&lt;/span&gt;&lt;span style="font-style: italic;"&gt;Z&lt;/span&gt;, &lt;span style="font-style: italic;"&gt;γ&lt;/span&gt;&lt;span style="font-style: italic;"&gt;h&lt;/span&gt;), this would ...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 103509] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Masaki Asano, Torsten Bringmann, Günter Sigl, and Martin Vollmann</p><p> An analysis of the Fermi gamma-ray space telescope data has recently revealed a resolved gamma-ray feature close to the galactic center which is consistent with monochromatic photons at an energy of about 130 GeV. If interpreted in terms of dark matter (DM) annihilating into <span style="font-style: italic;">γ</span><span style="font-style: italic;">γ</span> (<span style="font-style: italic;">γ</span><span style="font-style: italic;">Z</span>, <span style="font-style: italic;">γ</span><span style="font-style: italic;">h</span>), this would ...</p><p>[Phys. Rev. D 87, 103509] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>130 GeV gamma-ray line and generic dark matter model building constraints from continuum gamma rays, radio, and antiproton data</dc:title>
    <dc:creator>Masaki Asano, Torsten Bringmann, Günter Sigl, and Martin Vollmann</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.103509</dc:identifier>
    <dc:source>Phys. Rev. D 87, 103509 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.103509</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.103509</prism:url>
    <prism:startingPage>103509</prism:startingPage>
    <dc:subject>Astrophysics &amp; Cosmology</dc:subject>
    <prism:section>Astrophysics &amp; Cosmology</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.103510">
    <title>Galaxy rotation curves driven by massive vector fields: Key to the theory of the dark sector</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.103510</link>
    <description>Author(s): Boris E. Meierovich&lt;br/&gt;&lt;p&gt;The nongauge vector field with as simple a Lagrangian as possible turned out to be an adequate tool for the macroscopic description of the main properties of dark matter. The dependence of the velocity of a star on the radius of the orbit &lt;span style="font-style: italic;"&gt;V&lt;/span&gt;(&lt;span style="font-style: italic;"&gt;r&lt;/span&gt;)—galaxy rotation curve—is derived analytically from the f...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 103510] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Boris E. Meierovich</p><p> The nongauge vector field with as simple a Lagrangian as possible turned out to be an adequate tool for the macroscopic description of the main properties of dark matter. The dependence of the velocity of a star on the radius of the orbit <span style="font-style: italic;">V</span>(<span style="font-style: italic;">r</span>)—galaxy rotation curve—is derived analytically from the f...</p><p>[Phys. Rev. D 87, 103510] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Galaxy rotation curves driven by massive vector fields: Key to the theory of the dark sector</dc:title>
    <dc:creator>Boris E. Meierovich</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.103510</dc:identifier>
    <dc:source>Phys. Rev. D 87, 103510 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.103510</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.103510</prism:url>
    <prism:startingPage>103510</prism:startingPage>
    <dc:subject>Astrophysics &amp; Cosmology</dc:subject>
    <prism:section>Astrophysics &amp; Cosmology</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.103511">
    <title>Parameter space in Galileon gravity models</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.103511</link>
    <description>Author(s): Alexandre Barreira, Baojiu Li, Ariel Sanchez, Carlton M. Baugh, and Silvia Pascoli&lt;br/&gt;&lt;p&gt;We present the first constraints on the full parameter space of the Galileon modified gravity model, considering both the cosmological parameters and the coefficients which specify the additional terms in the Lagrangian due to the Galileon field, which we call the Galileon parameters. We use the lat...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 103511] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Alexandre Barreira, Baojiu Li, Ariel Sanchez, Carlton M. Baugh, and Silvia Pascoli</p><p> We present the first constraints on the full parameter space of the Galileon modified gravity model, considering both the cosmological parameters and the coefficients which specify the additional terms in the Lagrangian due to the Galileon field, which we call the Galileon parameters. We use the lat...</p><p>[Phys. Rev. D 87, 103511] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Parameter space in Galileon gravity models</dc:title>
    <dc:creator>Alexandre Barreira, Baojiu Li, Ariel Sanchez, Carlton M. Baugh, and Silvia Pascoli</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.103511</dc:identifier>
    <dc:source>Phys. Rev. D 87, 103511 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.103511</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.103511</prism:url>
    <prism:startingPage>103511</prism:startingPage>
    <dc:subject>Astrophysics &amp; Cosmology</dc:subject>
    <prism:section>Astrophysics &amp; Cosmology</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.103512">
    <title>Polarizing primordial gravitational waves by parity violation</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.103512</link>
    <description>Author(s): Anzhong Wang, Qiang Wu, Wen Zhao, and Tao Zhu&lt;br/&gt;&lt;p&gt;We study primordial gravitational waves in the Horava-Lifshitz theory of quantum gravity, in which high-order spatial derivative operators, including the ones violating parity, generically appear in order for the theory to be power-counting renormalizable and ultraviolet complete. Because of both pa...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 103512] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Anzhong Wang, Qiang Wu, Wen Zhao, and Tao Zhu</p><p> We study primordial gravitational waves in the Horava-Lifshitz theory of quantum gravity, in which high-order spatial derivative operators, including the ones violating parity, generically appear in order for the theory to be power-counting renormalizable and ultraviolet complete. Because of both pa...</p><p>[Phys. Rev. D 87, 103512] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Polarizing primordial gravitational waves by parity violation</dc:title>
    <dc:creator>Anzhong Wang, Qiang Wu, Wen Zhao, and Tao Zhu</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.103512</dc:identifier>
    <dc:source>Phys. Rev. D 87, 103512 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.103512</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.103512</prism:url>
    <prism:startingPage>103512</prism:startingPage>
    <dc:subject>Astrophysics &amp; Cosmology</dc:subject>
    <prism:section>Astrophysics &amp; Cosmology</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.87.104017">
    <title>Thermodynamic volumes and isoperimetric inequalities for de Sitter black holes</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.87.104017</link>
    <description>Author(s): Brian P. Dolan, David Kastor, David Kubizňák, Robert B. Mann, and Jennie Traschen&lt;br/&gt;&lt;p&gt;We consider the thermodynamics of rotating and charged asymptotically de Sitter (dS) black holes. Using Hamiltonian perturbation-theory techniques, we derive three different first-law relations including variations in the cosmological constant, and associated Smarr formulas that are satisfied by suc...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 87, 104017] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Brian P. Dolan, David Kastor, David Kubizňák, Robert B. Mann, and Jennie Traschen</p><p> We consider the thermodynamics of rotating and charged asymptotically de Sitter (dS) black holes. Using Hamiltonian perturbation-theory techniques, we derive three different first-law relations including variations in the cosmological constant, and associated Smarr formulas that are satisfied by suc...</p><p>[Phys. Rev. D 87, 104017] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Thermodynamic volumes and isoperimetric inequalities for de Sitter black holes</dc:title>
    <dc:creator>Brian P. Dolan, David Kastor, David Kubizňák, Robert B. Mann, and Jennie Traschen</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevD.87.104017</dc:identifier>
    <dc:source>Phys. Rev. D 87, 104017 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>10</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevD.87.104017</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevD.87.104017</prism:url>
    <prism:startingPage>104017</prism:startingPage>
    <dc:subject>General relativity, gravitation</dc:subject>
    <prism:section>General relativity, gravitation</prism:section>
  </item>
</rdf:RDF>
