<?xml version="1.0" encoding="UTF-8"?>
<rdf:RDF xmlns:taxo="http://purl.org/rss/1.0/modules/taxonomy/" xmlns:syn="http://purl.org/rss/1.0/modules/syndication/" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:admin="http://webns.net/mvcb/" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns="http://purl.org/rss/1.0/">
  <channel rdf:about="http://prd.aps.org/">
    <title>Recent Articles in Phys. Rev. D</title>
    <link>http://prd.aps.org/</link>
    <description>Recent articles in  Physical Review D</description>
    <dc:language>en-us</dc:language>
    <dc:rights>Copyright (c) 2008 The American Physical Society</dc:rights>
    <dc:date>2008-05-14T14:15:27-04:00</dc:date>
    <dc:publisher>assocpub@aps.org</dc:publisher>
    <dc:creator>rss@aps.org</dc:creator>
    <syn:updatePeriod>hourly</syn:updatePeriod>
    <syn:updateFrequency>4</syn:updateFrequency>
    <syn:updateBase>2008-05-14T14:15:27-04:00</syn:updateBase>
    <prism:rightsAgent>rss@aps.org</prism:rightsAgent>
    <items>
      <rdf:Seq>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.107702"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.107302"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.105013"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.105012"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.104017"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.104016"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.104015"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.103512"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.103511"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.103510"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.103003"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.096006"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.095011"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.095010"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.095009"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.094504"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.106005"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.103509"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.094008"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.091103"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.107701"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.107502"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.106004"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.106003"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.105011"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.105010"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.105009"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.104014"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.104013"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevD.77.104012"/>
      </rdf:Seq>
    </items>
  </channel>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.107702">
    <title>Compact Q-balls in the complex signum-Gordon model</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.107702</link>
    <description>Author(s): H. Arod&#378; and J. Lis&lt;br/&gt;We discuss Q-balls in the complex signum-Gordon model in d-dimensional space for d=1, 2, 3. The Q-balls have strictly finite size. Their total energy is a powerlike function of the conserved U(1) charge with the exponent equal to (d+2)(d+3)^{-1} . In the cases d=1 and d=3 explicit analytic solutions...&lt;br/&gt;[Phys. Rev. D 77, 107702] Published Wed May 14, 2008</description>
    <dc:creator>H. Arod&#378; and J. Lis</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.107702</dc:identifier>
    <dc:source>Phys. Rev. D 77, 107702</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>107702</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.107302">
    <title>Slow decay of magnetic fields in open Friedmann universes</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.107302</link>
    <description>Author(s): John D. Barrow and Christos G. Tsagas&lt;br/&gt;Magnetic fields in Friedmann universes can experience superadiabatic growth without departing from conventional electromagnetism. The reason is the relativistic coupling between vector fields and spacetime geometry, which slows down the decay of large-scale magnetic fields in open universes, compare...&lt;br/&gt;[Phys. Rev. D 77, 107302] Published Wed May 14, 2008</description>
    <dc:creator>John D. Barrow and Christos G. Tsagas</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.107302</dc:identifier>
    <dc:source>Phys. Rev. D 77, 107302</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>107302</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.105013">
    <title>Polarization tensor of charged gluons in color magnetic background field at finite temperature</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.105013</link>
    <description>Author(s): M. Bordag and V. Skalozub&lt;br/&gt;We calculate the polarization tensor of charged gluons in a Abelian homogeneous magnetic background field at a finite temperature in one-loop order in Lorentz background field gauge in full generality. Thereby, we first determine the ten independent tensor structures. For the calculation of the corr...&lt;br/&gt;[Phys. Rev. D 77, 105013] Published Wed May 14, 2008</description>
    <dc:creator>M. Bordag and V. Skalozub</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.105013</dc:identifier>
    <dc:source>Phys. Rev. D 77, 105013</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>105013</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.105012">
    <title>One-loop self-energy and counterterms in a massive Yang-Mills theory based on the nonlinearly realized gauge group</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.105012</link>
    <description>Author(s): D. Bettinelli, R. Ferrari, and A. Quadri&lt;br/&gt;In this paper, we evaluate the self-energy of the vector mesons at one loop in our recently proposed subtraction scheme for the massive nonlinearly realized SU(2) Yang-Mills theory. We check the fulfillment of physical unitarity. The resulting self-mass can be compared with the value obtained in the...&lt;br/&gt;[Phys. Rev. D 77, 105012] Published Wed May 14, 2008</description>
    <dc:creator>D. Bettinelli, R. Ferrari, and A. Quadri</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.105012</dc:identifier>
    <dc:source>Phys. Rev. D 77, 105012</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>105012</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.104017">
    <title>Template bank for gravitational waveforms from coalescing binary black holes: Nonspinning binaries</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.104017</link>
    <description>Author(s): P. Ajith, S. Babak, Y. Chen, M. Hewitson, B. Krishnan, A. M. Sintes, J. T. Whelan, B. Br&#252;gmann, P. Diener, N. Dorband, J. Gonzalez, M. Hannam, S. Husa, D. Pollney, L. Rezzolla, L. Santamar&#237;a, U. Sperhake, and J. Thornburg&lt;br/&gt;Gravitational waveforms from the inspiral and ring-down stages of the binary black-hole coalescences can be modeled accurately by approximation/perturbation techniques in general relativity. Recent progress in numerical relativity has enabled us to model also the nonperturbative merger phase of the ...&lt;br/&gt;[Phys. Rev. D 77, 104017] Published Wed May 14, 2008</description>
    <dc:creator>P. Ajith, S. Babak, Y. Chen, M. Hewitson, B. Krishnan, A. M. Sintes, J. T. Whelan, B. Br&#252;gmann, P. Diener, N. Dorband, J. Gonzalez, M. Hannam, S. Husa, D. Pollney, L. Rezzolla, L. Santamar&#237;a, U. Sperhake, and J. Thornburg</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.104017</dc:identifier>
    <dc:source>Phys. Rev. D 77, 104017</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>104017</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.104016">
    <title>Modifications by the QCD transition and e^{+} e^{-}  annihilation of the analytic spectrum of relic gravitational waves in the accelerating universe</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.104016</link>
    <description>Author(s): S. Wang, Y. Zhang, T. Y. Xia, and H. X. Miao&lt;br/&gt;As predicted by quantum chromodynamics (QCD), at around T&#8764;190&#8201;&#8201;MeV in the early Universe, the QCD transition occurs during which the quarks are combined into the massive hadrons. This process reduces the effective relativistic degree of freedom and causes a change in the expansion behavior of ...&lt;br/&gt;[Phys. Rev. D 77, 104016] Published Wed May 14, 2008</description>
    <dc:creator>S. Wang, Y. Zhang, T. Y. Xia, and H. X. Miao</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.104016</dc:identifier>
    <dc:source>Phys. Rev. D 77, 104016</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>104016</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.104015">
    <title>Stable cosmological models driven by a free quantum scalar field</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.104015</link>
    <description>Author(s): Claudio Dappiaggi, Klaus Fredenhagen, and Nicola Pinamonti&lt;br/&gt;In the mathematically rigorous analysis of semiclassical Einstein equations, the renormalization of the stress-energy tensor plays a crucial role. We address such a topic in the case of a scalar field with both arbitrary mass and coupling with gravity in the hypothesis that the underlying algebraic ...&lt;br/&gt;[Phys. Rev. D 77, 104015] Published Wed May 14, 2008</description>
    <dc:creator>Claudio Dappiaggi, Klaus Fredenhagen, and Nicola Pinamonti</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.104015</dc:identifier>
    <dc:source>Phys. Rev. D 77, 104015</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>104015</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.103512">
    <title>Do Newton&#8217;s G and Milgrom&#8217;s a_{0}  vary with cosmological epoch?</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.103512</link>
    <description>Author(s): Jacob D. Bekenstein and Eva Sagi&lt;br/&gt;In the scalar-tensor gravitational theories Newton&#8217;s constant G_{N} evolves in the expanding universe. Likewise, it has been speculated that the acceleration scale a_{0} in Milgrom&#8217;s modified Newtonian dynamics is tied to the scale of the cosmos, and must thus evolve. With the advent of relativi...&lt;br/&gt;[Phys. Rev. D 77, 103512] Published Wed May 14, 2008</description>
    <dc:creator>Jacob D. Bekenstein and Eva Sagi</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.103512</dc:identifier>
    <dc:source>Phys. Rev. D 77, 103512</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>103512</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.103511">
    <title>Cosmological constraints on invisible decay of dark matter</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.103511</link>
    <description>Author(s): Yan Gong and Xuelei Chen&lt;br/&gt;Cold dark matter may be in a metastable state and decays to other particles with a very long lifetime. If the decaying products of the dark matter are weakly interacting, e.g., neutrinos, then it would have little impact on astrophysical processes and is therefore difficult to observe. However, such...&lt;br/&gt;[Phys. Rev. D 77, 103511] Published Wed May 14, 2008</description>
    <dc:creator>Yan Gong and Xuelei Chen</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.103511</dc:identifier>
    <dc:source>Phys. Rev. D 77, 103511</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>103511</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.103510">
    <title>Nonthermal x rays from the Ophiuchus galaxy cluster and dark matter annihilation</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.103510</link>
    <description>Author(s): Stefano Profumo&lt;br/&gt;We investigate a scenario where the recently discovered nonthermal hard x-ray emission from the Ophiuchus cluster originates from inverse Compton scattering of energetic electrons and positrons produced in weakly interacting dark matter pair annihilations. We show that this scenario can account for ...&lt;br/&gt;[Phys. Rev. D 77, 103510] Published Wed May 14, 2008</description>
    <dc:creator>Stefano Profumo</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.103510</dc:identifier>
    <dc:source>Phys. Rev. D 77, 103510</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>103510</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.103003">
    <title>Coupled and extended quintessence: Theoretical differences and structure formation</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.103003</link>
    <description>Author(s): Valeria Pettorino and Carlo Baccigalupi&lt;br/&gt;The case of a coupling between dark energy and matter [coupled quintessence (CQ)] or gravity [extended quintessence (EQ)] has recently attracted a deep interest and has been widely investigated both in the Einstein and in the Jordan frames (EF, JF), within scalar-tensor theories. Focusing on the sim...&lt;br/&gt;[Phys. Rev. D 77, 103003] Published Wed May 14, 2008</description>
    <dc:creator>Valeria Pettorino and Carlo Baccigalupi</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.103003</dc:identifier>
    <dc:source>Phys. Rev. D 77, 103003</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>103003</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.096006">
    <title>BCS-BEC crossover in dense relativistic matter: Collective excitations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.096006</link>
    <description>Author(s): Tom&#225;&#353; Brauner&lt;br/&gt;We study the relativistic BCS-BEC crossover within a class of Nambu-Jona-Lasinio type models, including arbitrary Lorentz-scalar pairing channels. Using the mean-field approximation we investigate spectral properties of the collective bosonic excitations in the superfluid phase, with particular atte...&lt;br/&gt;[Phys. Rev. D 77, 096006] Published Wed May 14, 2008</description>
    <dc:creator>Tom&#225;&#353; Brauner</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.096006</dc:identifier>
    <dc:source>Phys. Rev. D 77, 096006</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>096006</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.095011">
    <title>Models and phenomenology of maximal flavor violation</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.095011</link>
    <description>Author(s): Shaouly Bar-Shalom and Arvind Rajaraman&lt;br/&gt;We consider models of maximal flavor violation, in which a new scalar mediates large q_{3} &#8596;q_{1} or q_{3} &#8596;q_{2} flavor-changing transitions (q_{i} is an i&#8217;th generation quark), while q_{3} &#8596;q_{3} transitions are suppressed, e.g., &#958;_{31} , &#958;_{13} &#8764;V_{tb} and &#958;_{33} &#8764;V_{td} , where &#958;...&lt;br/&gt;[Phys. Rev. D 77, 095011] Published Wed May 14, 2008</description>
    <dc:creator>Shaouly Bar-Shalom and Arvind Rajaraman</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.095011</dc:identifier>
    <dc:source>Phys. Rev. D 77, 095011</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>095011</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.095010">
    <title>Patterns of flavor signals in supersymmetric models</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.095010</link>
    <description>Author(s): Toru Goto, Yasuhiro Okada, Tetsuo Shindou, and Minoru Tanaka&lt;br/&gt;Quark and lepton flavor signals are studied in four supersymmetric models, namely, the minimal supergravity model, the minimal supersymmetric standard model with right-handed neutrinos, SU(5) supersymmetric grand unified theory with right-handed neutrinos, and the minimal supersymmetric standard mod...&lt;br/&gt;[Phys. Rev. D 77, 095010] Published Wed May 14, 2008</description>
    <dc:creator>Toru Goto, Yasuhiro Okada, Tetsuo Shindou, and Minoru Tanaka</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.095010</dc:identifier>
    <dc:source>Phys. Rev. D 77, 095010</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>095010</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.095009">
    <title>Unitarity bounds in the Higgs model including triplet fields with custodial symmetry</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.095009</link>
    <description>Author(s): Mayumi Aoki and Shinya Kanemura&lt;br/&gt;We study bounds on Higgs-boson masses from perturbative unitarity in the Georgi-Machacek model, whose Higgs sector is composed of a scalar isospin doublet and a real and a complex isospin triplet field. This model can be compatible with the electroweak precision data without fine-tuning because of t...&lt;br/&gt;[Phys. Rev. D 77, 095009] Published Wed May 14, 2008</description>
    <dc:creator>Mayumi Aoki and Shinya Kanemura</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.095009</dc:identifier>
    <dc:source>Phys. Rev. D 77, 095009</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>095009</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.094504">
    <title>Lattice actions for Yang-Mills quantum mechanics with exact supersymmetry</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.094504</link>
    <description>Author(s): Simon Catterall and Anosh Joseph&lt;br/&gt;We derive lattice actions for Yang-Mills quantum mechanics for models with Q=4, 8 and 16&#160;supercharges which possess an exact supersymmetry at nonzero lattice spacing. These are obtained by dimensional reduction of twisted versions of the corresponding super Yang-Mills theories in D=2, 3 and 4&#160;dime...&lt;br/&gt;[Phys. Rev. D 77, 094504] Published Wed May 14, 2008</description>
    <dc:creator>Simon Catterall and Anosh Joseph</dc:creator>
    <dc:date>2008-05-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.094504</dc:identifier>
    <dc:source>Phys. Rev. D 77, 094504</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2008-05-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>094504</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.106005">
    <title>Reconstructing the universe history, from inflation to acceleration, with phantom and canonical scalar fields</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.106005</link>
    <description>Author(s): Emilio Elizalde, Shin&#8217;ichi Nojiri, Sergei D. Odintsov, Diego S&#225;ez-G&#243;mez, and Valerio Faraoni&lt;br/&gt;We consider the reconstruction technique in theories with a single or multiple (phantom and/or canonical) scalar fields. With the help of several examples, it is demonstrated explicitly that the universe expansion history, unifying early-time inflation and late-time acceleration, can be realized in ...&lt;br/&gt;[Phys. Rev. D 77, 106005] Published Tue May 13, 2008</description>
    <dc:creator>Emilio Elizalde, Shin&#8217;ichi Nojiri, Sergei D. Odintsov, Diego S&#225;ez-G&#243;mez, and Valerio Faraoni</dc:creator>
    <dc:date>2008-05-13T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.106005</dc:identifier>
    <dc:source>Phys. Rev. D 77, 106005</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-13T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>106005</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.103509">
    <title>Galactic substructure and direct detection of dark matter</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.103509</link>
    <description>Author(s): Marc Kamionkowski and Savvas M. Koushiappas&lt;br/&gt;We study the effects of substructure in the Galactic halo on direct detection of dark matter, on searches for energetic neutrinos from weakly interacting massive particles (WIMP) annihilation in the Sun and Earth, and on the enhancement in the WIMP annihilation rate in the halo. Our central result i...&lt;br/&gt;[Phys. Rev. D 77, 103509] Published Tue May 13, 2008</description>
    <dc:creator>Marc Kamionkowski and Savvas M. Koushiappas</dc:creator>
    <dc:date>2008-05-13T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.103509</dc:identifier>
    <dc:source>Phys. Rev. D 77, 103509</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-13T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>103509</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.094008">
    <title>Two-loop jet function and jet mass for top quarks</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.094008</link>
    <description>Author(s): Ambar Jain, Ignazio Scimemi, and Iain W. Stewart&lt;br/&gt;We compute the two-loop heavy-quark jet function in the heavy-quark limit. This is one of the key ingredients in next-to-next-to-leading order and next-to-next-to-leading-log order computations of the invariant mass distribution of top-jets at a future e^{+} e^{-} collider. The shape of the top-inva...&lt;br/&gt;[Phys. Rev. D 77, 094008] Published Tue May 13, 2008</description>
    <dc:creator>Ambar Jain, Ignazio Scimemi, and Iain W. Stewart</dc:creator>
    <dc:date>2008-05-13T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.094008</dc:identifier>
    <dc:source>Phys. Rev. D 77, 094008</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2008-05-13T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>094008</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.091103">
    <title>Measurements of time-dependent CP violation in B^{0} &#8594;&#968;(2S)K_{S}^{0}  decays</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.091103</link>
    <description>Author(s): H. Sahoo et al. Belle Collaboration&lt;br/&gt;We report improved measurements of time-dependent CP violation parameters for B^{0} (B [over &#175;] ^{0} )&#8594;&#968;(2S)K_{S}^{0} . This analysis is based on a data sample of 657&#215;10^{6} BB [over &#175;] pairs collected at the &#933;(4S) resonance with the Belle detector at the KEKB energy-asymmetric e^{+} e^{-} co...&lt;br/&gt;&lt;img src="http://prola.aps.org/graphics/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/&gt;&lt;br/&gt;[Phys. Rev. D 77, 091103] Published Tue May 13, 2008</description>
    <dc:creator>H. Sahoo et al. Belle Collaboration</dc:creator>
    <dc:date>2008-05-13T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.091103</dc:identifier>
    <dc:source>Phys. Rev. D 77, 091103</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2008-05-13T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>091103</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.107701">
    <title>Asymptotic analysis of the Skyrme-like monopole</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.107701</link>
    <description>Author(s): Yves Brihaye, J&#252;rgen Burzlaff, and D. H. Tchrakian&lt;br/&gt;We consider a variant of the Georgi-Glashow model in the Bogomol&#8217;nyi-Prasad-Sommerfield limit, augmented by a higher derivative Skyrme-like term, which is the simplest Yang-Mills-Higgs model that can support monopole bound states. The spherically symmetric solutions are studied with a combination ...&lt;br/&gt;[Phys. Rev. D 77, 107701] Published Mon May 12, 2008</description>
    <dc:creator>Yves Brihaye, J&#252;rgen Burzlaff, and D. H. Tchrakian</dc:creator>
    <dc:date>2008-05-12T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.107701</dc:identifier>
    <dc:source>Phys. Rev. D 77, 107701</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-12T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>107701</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.107502">
    <title>Remark on orbital precession due to central-force perturbations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.107502</link>
    <description>Author(s): O. I. Chashchina and Z. K. Silagadze&lt;br/&gt;We show that the main result of the recent paper by G.&#8201;S. Adkins and J. McDonnell, Phys. Rev. D 75, 082001 (2007), the formula for the precession of Keplerian orbits induced by central-force perturbations, can be obtained very simply by the use of Hamilton&#8217;s vector.&lt;br/&gt;[Phys. Rev. D 77, 107502] Published Mon May 12, 2008</description>
    <dc:creator>O. I. Chashchina and Z. K. Silagadze</dc:creator>
    <dc:date>2008-05-12T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.107502</dc:identifier>
    <dc:source>Phys. Rev. D 77, 107502</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-12T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>107502</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.106004">
    <title>D^{6} R^{4}  term in type&#160;IIB string theory on T^{2}  and U-duality</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.106004</link>
    <description>Author(s): Anirban Basu&lt;br/&gt;We propose a manifestly U-duality invariant modular form for the D^{6} R^{4} interaction in the effective action of type&#160;IIB string theory compactified on T^{2} . It receives perturbative contributions up to genus three, as well as nonperturbative contributions from D-instantons and (p,q) string in...&lt;br/&gt;[Phys. Rev. D 77, 106004] Published Mon May 12, 2008</description>
    <dc:creator>Anirban Basu</dc:creator>
    <dc:date>2008-05-12T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.106004</dc:identifier>
    <dc:source>Phys. Rev. D 77, 106004</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-12T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>106004</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.106003">
    <title>D^{4} R^{4}  term in type&#160;IIB string theory on T^{2}  and U-duality</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.106003</link>
    <description>Author(s): Anirban Basu&lt;br/&gt;We propose a manifestly U-duality invariant modular form for the D^{4} R^{4} interaction in type&#160;IIB string theory compactified on T^{2} . It receives perturbative contributions up to two loops, and nonperturbative contributions from D-instantons and (p,q) string instantons wrapping T^{2} . We prov...&lt;br/&gt;[Phys. Rev. D 77, 106003] Published Mon May 12, 2008</description>
    <dc:creator>Anirban Basu</dc:creator>
    <dc:date>2008-05-12T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.106003</dc:identifier>
    <dc:source>Phys. Rev. D 77, 106003</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-12T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>106003</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.105011">
    <title>Energy-momentum tensor of a Casimir apparatus in a weak gravitational field: Scalar case</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.105011</link>
    <description>Author(s): Giampiero Esposito, George M. Napolitano, and Luigi Rosa&lt;br/&gt;Recent work in the literature had evaluated the energy-momentum tensor of a Casimir apparatus in a weak gravitational field, for an electromagnetic field subject to perfect conductor boundary conditions on parallel plates. The Casimir apparatus was then predicted to experience a tiny push in the upw...&lt;br/&gt;[Phys. Rev. D 77, 105011] Published Mon May 12, 2008</description>
    <dc:creator>Giampiero Esposito, George M. Napolitano, and Luigi Rosa</dc:creator>
    <dc:date>2008-05-12T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.105011</dc:identifier>
    <dc:source>Phys. Rev. D 77, 105011</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-12T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>105011</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.105010">
    <title>Twisted statistics in &#954;-Minkowski spacetime</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.105010</link>
    <description>Author(s): T. R. Govindarajan, Kumar S. Gupta, E. Harikumar, S. Meljanac, and D. Meljanac&lt;br/&gt;We consider the issue of statistics for identical particles or fields in &#954;-deformed spaces, where the system admits a symmetry group G. We obtain the twisted flip operator compatible with the action of the symmetry group, which is relevant for describing particle statistics in the presence of the n...&lt;br/&gt;[Phys. Rev. D 77, 105010] Published Mon May 12, 2008</description>
    <dc:creator>T. R. Govindarajan, Kumar S. Gupta, E. Harikumar, S. Meljanac, and D. Meljanac</dc:creator>
    <dc:date>2008-05-12T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.105010</dc:identifier>
    <dc:source>Phys. Rev. D 77, 105010</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-12T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>105010</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.105009">
    <title>Nonsupersymmetric Seiberg duality, orientifold QCD, and noncritical strings</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.105009</link>
    <description>Author(s): Adi Armoni, Dan Isra&#235;l, Gregory Moraitis, and Vasilis Niarchos&lt;br/&gt;We propose an electric-magnetic duality and conjecture an exact conformal window for a class of nonsupersymmetric U(N_{c} ) gauge theories with fermions in the (anti)symmetric representation of the gauge group and N_{f} additional scalar and fermion flavors. The duality exchanges N_{c} &#8594;N_{f} -N_{...&lt;br/&gt;[Phys. Rev. D 77, 105009] Published Mon May 12, 2008</description>
    <dc:creator>Adi Armoni, Dan Isra&#235;l, Gregory Moraitis, and Vasilis Niarchos</dc:creator>
    <dc:date>2008-05-12T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.105009</dc:identifier>
    <dc:source>Phys. Rev. D 77, 105009</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-12T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>105009</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.104014">
    <title>Generating gravity waves with matter and electromagnetic waves</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.104014</link>
    <description>Author(s): C. Barrab&#232;s and P A. Hogan&lt;br/&gt;If a homogeneous plane lightlike shell collides head on with a homogeneous plane electromagnetic shock wave having a step-function profile then no backscattered gravitational waves are produced. We demonstrate, by explicit calculation, that if the matter is accompanied by a homogeneous plane electro...&lt;br/&gt;[Phys. Rev. D 77, 104014] Published Mon May 12, 2008</description>
    <dc:creator>C. Barrab&#232;s and P A. Hogan</dc:creator>
    <dc:date>2008-05-12T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.104014</dc:identifier>
    <dc:source>Phys. Rev. D 77, 104014</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-12T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>104014</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.104013">
    <title>de Sitter thermodynamics: A glimpse into nonequilibrium</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.104013</link>
    <description>Author(s): Rodrigo Aros&lt;br/&gt;In this article it is shown that the thermodynamical evolution of a Schwarzschild de Sitter space is the evaporation of its black hole. The result is extended in higher dimensions to Lovelock theories of gravity with a single positive cosmological constant.&lt;br/&gt;[Phys. Rev. D 77, 104013] Published Mon May 12, 2008</description>
    <dc:creator>Rodrigo Aros</dc:creator>
    <dc:date>2008-05-12T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.104013</dc:identifier>
    <dc:source>Phys. Rev. D 77, 104013</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-12T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>104013</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.104012">
    <title>Quantum reference frames and deformed symmetries</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.104012</link>
    <description>Author(s): Florian Girelli and David Poulin&lt;br/&gt;In the context of constrained quantum mechanics, reference systems are used to construct relational observables that are invariant under the action of the symmetry group. Upon measurement of a relational observable, the reference system undergoes an unavoidable measurement &#8220;back-action&#8221; that mod...&lt;br/&gt;[Phys. Rev. D 77, 104012] Published Mon May 12, 2008</description>
    <dc:creator>Florian Girelli and David Poulin</dc:creator>
    <dc:date>2008-05-12T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.104012</dc:identifier>
    <dc:source>Phys. Rev. D 77, 104012</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-05-12T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>104012</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
</rdf:RDF>
