<?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://prl.aps.org/">
    <title>PRL: Gravitation and Astrophysics</title>
    <link>http://prl.aps.org/</link>
    <description>Recently published articles in Phys. Rev. Lett. in the Table of Content section "Gravitation and Astrophysics"</description>
    <dc:language>en-us</dc:language>
    <dc:rights>Copyright (c) 2008 The American Physical Society</dc:rights>
    <dc:date>2008-05-07T08:09:08-04:00</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>2008-05-07T08:09:08-04:00</syn:updateBase>
    <prism:rightsAgent>rss@aps.org</prism:rightsAgent>
    <items>
      <rdf:Seq>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.171302"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.171101"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.171301"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.161302"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.161101"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.161301"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.151102"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.151101"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.141301"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.131302"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.131301"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.131101"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.121101"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.121301"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.111102"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.111101"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.101102"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.101101"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.091304"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.091303"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.091302"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.091301"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.091102"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.091101"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.081301"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.081102"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.081101"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.071301"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.061301"/>
        <rdf:li rdf:resource="http://link.aps.org/doi/10.1103/PhysRevLett.100.051101"/>
      </rdf:Seq>
    </items>
  </channel>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.171302">
    <title>Non-Gaussianities in New Ekpyrotic Cosmology</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.171302</link>
    <description>Author(s): Evgeny I. Buchbinder, Justin Khoury, and Burt A. Ovrut&lt;br/&gt;The new ekpyrotic model is an alternative scenario of the early Universe which relies on a phase of slow contraction before the big bang. We calculate the 3-point and 4-point correlation functions of primordial density perturbations and find a generically large non-Gaussian signal, just below the cu...&lt;br/&gt;[Phys. Rev. Lett. 100, 171302] Published Fri May 02, 2008</description>
    <dc:creator>Evgeny I. Buchbinder, Justin Khoury, and Burt A. Ovrut</dc:creator>
    <dc:date>2008-05-02T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.171302</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 171302</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>17</prism:issueIdentifier>
    <prism:publicationDate>2008-05-02T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>171302</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.171101">
    <title>Complete Analytic Solution of the Geodesic Equation in Schwarzschild&#8211;(Anti-)de Sitter Spacetimes</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.171101</link>
    <description>Author(s): Eva Hackmann and Claus L&#228;mmerzahl&lt;br/&gt;The complete set of analytic solutions of the geodesic equation in a Schwarzschild&#8211;(anti-)de&#160;Sitter space-time is presented. The solutions are derived from the Jacobi inversion problem restricted to the theta&#160;divisor. In its final form the solutions can be expressed in terms of derivatives of Kl...&lt;br/&gt;[Phys. Rev. Lett. 100, 171101] Published Fri May 02, 2008</description>
    <dc:creator>Eva Hackmann and Claus L&#228;mmerzahl</dc:creator>
    <dc:date>2008-05-02T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.171101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 171101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>17</prism:issueIdentifier>
    <prism:publicationDate>2008-05-02T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>171101</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.171301">
    <title>Late Time Behavior of False Vacuum Decay: Possible Implications for Cosmology and Metastable Inflating States</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.171301</link>
    <description>Author(s): Lawrence M. Krauss and James Dent&lt;br/&gt;We describe here how the late time behavior of the quantum mechanical decay of unstable states, which is predicted to deviate from an exponential form, may have important cosmological implications. It may increase the likelihood of eternal inflation and may enhance the likelihood of observing a smal...&lt;br/&gt;[Phys. Rev. Lett. 100, 171301] Published Wed Apr 30, 2008</description>
    <dc:creator>Lawrence M. Krauss and James Dent</dc:creator>
    <dc:date>2008-04-30T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.171301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 171301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>17</prism:issueIdentifier>
    <prism:publicationDate>2008-04-30T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>171301</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.161302">
    <title>Quantum Bounce and Cosmic Recall</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.161302</link>
    <description>Author(s): Alejandro Corichi and Parampreet Singh&lt;br/&gt;Loop quantum cosmology predicts that, in simple models, the big bang is replaced by a quantum bounce. A natural question is whether the universe retains, after the bounce, its memory about the previous epoch. More precisely, does the Universe retain various properties of the state after evolving uni...&lt;br/&gt;[Phys. Rev. Lett. 100, 161302] Published Wed Apr 23, 2008</description>
    <dc:creator>Alejandro Corichi and Parampreet Singh</dc:creator>
    <dc:date>2008-04-23T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.161302</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 161302</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>16</prism:issueIdentifier>
    <prism:publicationDate>2008-04-23T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>161302</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.161101">
    <title>Far-from-Constant Mean Curvature Solutions of Einstein&#8217;s Constraint Equations with Positive Yamabe Metrics</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.161101</link>
    <description>Author(s): M. Holst, G. Nagy, and G. Tsogtgerel&lt;br/&gt;We establish new existence results for the Einstein constraint equations for mean extrinsic curvature arbitrarily far from constant. The results hold for rescaled background metric in the positive Yamabe class, with freely specifiable parts of the data sufficiently small, and with matter energy dens...&lt;br/&gt;[Phys. Rev. Lett. 100, 161101] Published Wed Apr 23, 2008</description>
    <dc:creator>M. Holst, G. Nagy, and G. Tsogtgerel</dc:creator>
    <dc:date>2008-04-23T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.161101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 161101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>16</prism:issueIdentifier>
    <prism:publicationDate>2008-04-23T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>161101</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.161301">
    <title>Possibility of Precise Measurement of the Cosmological Power Spectrum with a Dedicated Survey of 21&#160;cm Emission after Reionization</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.161301</link>
    <description>Author(s): Abraham Loeb and J. Stuart Wyithe&lt;br/&gt;Measurements of the 21&#160;cm line emission by residual cosmic hydrogen after reionization can be used to trace the power spectrum of density perturbations through a significant fraction of the observable volume of the Universe. We show that a dedicated 21&#160;cm observatory could probe a number of indepe...&lt;br/&gt;[Phys. Rev. Lett. 100, 161301] Published Tue Apr 22, 2008</description>
    <dc:creator>Abraham Loeb and J. Stuart Wyithe</dc:creator>
    <dc:date>2008-04-22T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.161301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 161301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>16</prism:issueIdentifier>
    <prism:publicationDate>2008-04-22T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>161301</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.151102">
    <title>Universal Charge-Radius Relation for Subatomic and Astrophysical Compact Objects</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.151102</link>
    <description>Author(s): Jes Madsen&lt;br/&gt;Electron-positron pair creation in supercritical electric fields limits the net charge of any static, spherical object, such as superheavy nuclei, strangelets, and Q balls, or compact stars like neutron stars, quark stars, and black holes. For radii between 4&#215;10^{2} and 10^{4} &#8201;&#8201;fm the upper bo...&lt;br/&gt;[Phys. Rev. Lett. 100, 151102] Published Thu Apr 17, 2008</description>
    <dc:creator>Jes Madsen</dc:creator>
    <dc:date>2008-04-17T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.151102</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 151102</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>15</prism:issueIdentifier>
    <prism:publicationDate>2008-04-17T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>151102</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.151101">
    <title>Binary&#8211;Black-Hole Merger: Symmetry and the Spin Expansion</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.151101</link>
    <description>Author(s): Latham Boyle, Michael Kesden, and Samaya Nissanke&lt;br/&gt;We regard binary&#8211;black-hole (BBH) merger as a map from a simple initial state (two Kerr black holes, with dimensionless spins a and b) to a simple final state (a Kerr black hole with mass m, dimensionless spin s, and kick velocity k). By expanding this map around a=b=0 and applying symmetry constr...&lt;br/&gt;[Phys. Rev. Lett. 100, 151101] Published Thu Apr 17, 2008</description>
    <dc:creator>Latham Boyle, Michael Kesden, and Samaya Nissanke</dc:creator>
    <dc:date>2008-04-17T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.151101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 151101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>15</prism:issueIdentifier>
    <prism:publicationDate>2008-04-17T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>151101</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.141301">
    <title>Physical Interpretation of the Spectrum of Black Hole Quasinormal Modes</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.141301</link>
    <description>Author(s): Michele Maggiore&lt;br/&gt;When a classical black hole is perturbed, its relaxation is governed by a set of quasinormal modes with complex frequencies &#969;=&#969;_{R} +i&#969;_{I} . We show that this behavior is the same as that of damped harmonic oscillators whose real frequencies are (&#969;_{R}^{2} +&#969;_{I}^{2} )^{1/2} , rather than simp...&lt;br/&gt;&lt;img src="http://prola.aps.org/graphics/prlsugg30x30.gif" width="30" height="30" alt="PRL Editors' Suggestion"/&gt;&lt;br/&gt;[Phys. Rev. Lett. 100, 141301] Published Tue Apr 08, 2008</description>
    <dc:creator>Michele Maggiore</dc:creator>
    <dc:date>2008-04-08T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.141301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 141301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>14</prism:issueIdentifier>
    <prism:publicationDate>2008-04-08T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>141301</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.131302">
    <title>Nearly Scale Invariant Spectrum of Gravitational Radiation from Global Phase Transitions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.131302</link>
    <description>Author(s): Katherine Jones-Smith, Lawrence M. Krauss, and Harsh Mathur&lt;br/&gt;Using a large N sigma model approximation we explicitly calculate the power spectrum of gravitational waves arising from a global phase transition in the early Universe and we confirm that it is scale invariant, implying an observation of such a spectrum may not be a unique feature of inflation. Mor...&lt;br/&gt;[Phys. Rev. Lett. 100, 131302] Published Wed Apr 02, 2008</description>
    <dc:creator>Katherine Jones-Smith, Lawrence M. Krauss, and Harsh Mathur</dc:creator>
    <dc:date>2008-04-02T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.131302</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 131302</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>13</prism:issueIdentifier>
    <prism:publicationDate>2008-04-02T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>131302</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.131301">
    <title>Signatures of Gravitational Fixed Points at the Large Hadron Collider</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.131301</link>
    <description>Author(s): Daniel F. Litim and Tilman Plehn&lt;br/&gt;We study quantum-gravitational signatures at the CERN Large Hadron Collider (LHC) in the context of theories with extra spatial dimensions and a low fundamental Planck scale in the TeV range. Implications of a gravitational fixed point at high energies are worked out using Wilson&#8217;s renormalization...&lt;br/&gt;[Phys. Rev. Lett. 100, 131301] Published Tue Apr 01, 2008</description>
    <dc:creator>Daniel F. Litim and Tilman Plehn</dc:creator>
    <dc:date>2008-04-01T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.131301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 131301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>13</prism:issueIdentifier>
    <prism:publicationDate>2008-04-01T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>131301</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.131101">
    <title>Relativistic Photon Mediated Shocks</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.131101</link>
    <description>Author(s): Amir Levinson and Omer Bromberg&lt;br/&gt;A system of equations governing the structure of a steady, relativistic radiation-dominated shock is derived, starting from the general form of the transfer equation obeyed by the photon distribution function. Closure is obtained by truncating the system of moment equations at some order. The anisot...&lt;br/&gt;[Phys. Rev. Lett. 100, 131101] Published Mon Mar 31, 2008</description>
    <dc:creator>Amir Levinson and Omer Bromberg</dc:creator>
    <dc:date>2008-03-31T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.131101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 131101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>13</prism:issueIdentifier>
    <prism:publicationDate>2008-03-31T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>131101</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.121101">
    <title>Weak Cosmic Censorship: As Strong as Ever</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.121101</link>
    <description>Author(s): Shahar Hod&lt;br/&gt;Spacetime singularities that arise in gravitational collapse are always hidden inside of black holes. This is the essence of the weak cosmic censorship conjecture. The hypothesis, put forward by Penrose 40 years ago, is still one of the most important open questions in general relativity. In this Le...&lt;br/&gt;[Phys. Rev. Lett. 100, 121101] Published Wed Mar 26, 2008</description>
    <dc:creator>Shahar Hod</dc:creator>
    <dc:date>2008-03-26T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.121101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 121101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2008-03-26T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>121101</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.121301">
    <title>General Nonextremal Rotating Charged G&#246;del Black Holes in Minimal Five-Dimensional Gauged Supergravity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.121301</link>
    <description>Author(s): Shuang-Qing Wu&lt;br/&gt;I present the general exact solutions for nonextremal rotating charged black holes in the G&#246;del universe of five-dimensional minimal supergravity theory. They are uniquely characterized by four nontrivial parameters: namely, the mass m, the charge q, the Kerr equal rotation parameter a, and the G&#246;...&lt;br/&gt;[Phys. Rev. Lett. 100, 121301] Published Mon Mar 24, 2008</description>
    <dc:creator>Shuang-Qing Wu</dc:creator>
    <dc:date>2008-03-24T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.121301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 121301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2008-03-24T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>121301</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.111102">
    <title>Constraints on Torsion from Bounds on Lorentz Violation</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.111102</link>
    <description>Author(s): V. Alan Kosteleck&#253;, Neil Russell, and Jay D. Tasson&lt;br/&gt;Exceptional sensitivity to spacetime torsion can be achieved by searching for its couplings to fermions. Recent experimental searches for Lorentz&#160;violation are exploited to extract new constraints involving 19 of the 24 independent torsion components down to levels of order 10^{-31} &#8201;&#8201;GeV.&lt;br/&gt;[Phys. Rev. Lett. 100, 111102] Published Thu Mar 20, 2008</description>
    <dc:creator>V. Alan Kosteleck&#253;, Neil Russell, and Jay D. Tasson</dc:creator>
    <dc:date>2008-03-20T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.111102</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 111102</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>11</prism:issueIdentifier>
    <prism:publicationDate>2008-03-20T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>111102</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.111101">
    <title>Does the Planck Mass Run on the Cosmological-Horizon Scale?</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.111101</link>
    <description>Author(s): Georg Robbers, Niayesh Afshordi, and Michael Doran&lt;br/&gt;Einstein&#8217;s theory of general relativity contains a universal value of the Planck mass. However, one may envisage that in alternative theories of gravity the effective value of the Planck mass (or Newton&#8217;s constant), which quantifies the coupling of matter to metric perturbations, can run on the ...&lt;br/&gt;[Phys. Rev. Lett. 100, 111101] Published Tue Mar 18, 2008</description>
    <dc:creator>Georg Robbers, Niayesh Afshordi, and Michael Doran</dc:creator>
    <dc:date>2008-03-18T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.111101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 111101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>11</prism:issueIdentifier>
    <prism:publicationDate>2008-03-18T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>111101</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.101102">
    <title>Fractal Threshold Behavior in Vacuum Gravitational Collapse</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.101102</link>
    <description>Author(s): Sebastian J. Szybka and Tadeusz Chmaj&lt;br/&gt;We present the numerical evidence for fractal threshold behavior in the five dimensional vacuum Einstein equations satisfying the cohomogeneity-two triaxial Bianchi type-IX ansatz. In other words, we show that a flip of the wings of a butterfly may influence the process of the black hole formation.&lt;br/&gt;[Phys. Rev. Lett. 100, 101102] Published Wed Mar 12, 2008</description>
    <dc:creator>Sebastian J. Szybka and Tadeusz Chmaj</dc:creator>
    <dc:date>2008-03-12T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.101102</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 101102</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-03-12T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>101102</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.101101">
    <title>First Observation of the Greisen-Zatsepin-Kuzmin Suppression</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.101101</link>
    <description>Author(s): R. U. Abbasi et al. High Resolution Fly&#8217;s Eye Collaboration&lt;br/&gt;The High Resolution Fly&#8217;s Eye (HiRes) experiment has observed the Greisen-Zatsepin-Kuzmin suppression (called the GZK cutoff) with a statistical significance of five standard deviations. HiRes&#8217; measurement of the flux of ultrahigh energy cosmic rays shows a sharp suppression at an energy of 6&#215;1...&lt;br/&gt;&lt;img src="http://prola.aps.org/graphics/prlsugg30x30.gif" width="30" height="30" alt="PRL Editors' Suggestion"/&gt;&lt;br/&gt;[Phys. Rev. Lett. 100, 101101] Published Mon Mar 10, 2008</description>
    <dc:creator>R. U. Abbasi et al. High Resolution Fly&#8217;s Eye Collaboration</dc:creator>
    <dc:date>2008-03-10T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.101101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 101101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2008-03-10T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>101101</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.091304">
    <title>Planckian Birth of a Quantum de Sitter Universe</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.091304</link>
    <description>Author(s): J. Ambj&#248;rn, A. G&#246;rlich, J. Jurkiewicz, and R. Loll&lt;br/&gt;We show that the quantum universe emerging from a nonperturbative, Lorentzian sum over geometries can be described with a high accuracy by a four-dimensional de&#160;Sitter spacetime. By a scaling analysis involving Newton&#8217;s constant, we establish that the linear size of the quantum universes under st...&lt;br/&gt;[Phys. Rev. Lett. 100, 091304] Published Fri Mar 07, 2008</description>
    <dc:creator>J. Ambj&#248;rn, A. G&#246;rlich, J. Jurkiewicz, and R. Loll</dc:creator>
    <dc:date>2008-03-07T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.091304</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 091304</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2008-03-07T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>091304</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.091303">
    <title>Baryon Acoustic Oscillation Intensity Mapping of Dark Energy</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.091303</link>
    <description>Author(s): Tzu-Ching Chang, Ue-Li Pen, Jeffrey B. Peterson, and Patrick McDonald&lt;br/&gt;The expansion of the Universe appears to be accelerating, and the mysterious antigravity agent of this acceleration has been called &#8220;dark energy.&#8221; To measure the dynamics of dark energy, baryon acoustic oscillations (BAO) can be used. Previous discussions of the BAO dark energy test have focused...&lt;br/&gt;[Phys. Rev. Lett. 100, 091303] Published Wed Mar 05, 2008</description>
    <dc:creator>Tzu-Ching Chang, Ue-Li Pen, Jeffrey B. Peterson, and Patrick McDonald</dc:creator>
    <dc:date>2008-03-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.091303</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 091303</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2008-03-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>091303</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.091302">
    <title>Cosmic (Super)String Constraints from 21&#160;cm Radiation</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.091302</link>
    <description>Author(s): Rishi Khatri and Benjamin D. Wandelt&lt;br/&gt;We calculate the contribution of cosmic strings arising from a phase transition in the early Universe, or cosmic superstrings arising from brane inflation, to the cosmic 21&#160;cm power spectrum at redshifts z&#8805;30. Future experiments can exploit this effect to constrain the cosmic string tension G&#956; a...&lt;br/&gt;[Phys. Rev. Lett. 100, 091302] Published Tue Mar 04, 2008</description>
    <dc:creator>Rishi Khatri and Benjamin D. Wandelt</dc:creator>
    <dc:date>2008-03-04T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.091302</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 091302</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2008-03-04T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>091302</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.091301">
    <title>Tabletop Creation of Entangled Multi-keV Photon Pairs and the Unruh Effect</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.091301</link>
    <description>Author(s): Ralf Sch&#252;tzhold, Gernot Schaller, and Dietrich Habs&lt;br/&gt;Electrons moving in a strong periodic electromagnetic field (e.g., laser or undulator) may convert quantum vacuum fluctuations into pairs of entangled photons, which can be understood in terms of the Unruh effect. Apart from verifying this striking phenomenon, the considered effect may allow the con...&lt;br/&gt;[Phys. Rev. Lett. 100, 091301] Published Mon Mar 03, 2008</description>
    <dc:creator>Ralf Sch&#252;tzhold, Gernot Schaller, and Dietrich Habs</dc:creator>
    <dc:date>2008-03-03T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.091301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 091301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2008-03-03T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>091301</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.091102">
    <title>Anomalous Orbital-Energy Changes Observed during Spacecraft Flybys of Earth</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.091102</link>
    <description>Author(s): John D. Anderson, James K. Campbell, John E. Ekelund, Jordan Ellis, and James F. Jordan&lt;br/&gt;We report and characterize anomalous orbital-energy changes observed during six Earth flybys by the Galileo, NEAR, Cassini, Rosetta, and MESSENGER spacecraft. These anomalous energy changes are consistent with an empirical prediction formula which is proportional to the total orbital energy per unit...&lt;br/&gt;[Phys. Rev. Lett. 100, 091102] Published Mon Mar 03, 2008</description>
    <dc:creator>John D. Anderson, James K. Campbell, John E. Ekelund, Jordan Ellis, and James F. Jordan</dc:creator>
    <dc:date>2008-03-03T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.091102</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 091102</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2008-03-03T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>091102</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.091101">
    <title>Kerr Black Holes Are Not Unique to General Relativity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.091101</link>
    <description>Author(s): Dimitrios Psaltis, Delphine Perrodin, Keith R. Dienes, and Irina Mocioiu&lt;br/&gt;Considerable attention has recently focused on gravity theories obtained by extending general relativity with additional scalar, vector, or tensor degrees of freedom. In this Letter, we show that the black-hole solutions of these theories are essentially indistinguishable from those of general relat...&lt;br/&gt;[Phys. Rev. Lett. 100, 091101] Published Mon Mar 03, 2008</description>
    <dc:creator>Dimitrios Psaltis, Delphine Perrodin, Keith R. Dienes, and Irina Mocioiu</dc:creator>
    <dc:date>2008-03-03T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.091101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 091101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2008-03-03T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>091101</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.081301">
    <title>Nonlinear Growth of Firehose and Mirror Fluctuations in Astrophysical Plasmas</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.081301</link>
    <description>Author(s): A. A. Schekochihin, S. C. Cowley, R. M. Kulsrud, M. S. Rosin, and T. Heinemann&lt;br/&gt;In turbulent high-beta astrophysical plasmas (exemplified by the galaxy cluster plasmas), pressure-anisotropy-driven firehose and mirror fluctuations grow nonlinearly to large amplitudes, &#948;B/B&#8764;1, on a time scale comparable to the turnover time of the turbulent motions. The principle of their nonl...&lt;br/&gt;[Phys. Rev. Lett. 100, 081301] Published Fri Feb 29, 2008</description>
    <dc:creator>A. A. Schekochihin, S. C. Cowley, R. M. Kulsrud, M. S. Rosin, and T. Heinemann</dc:creator>
    <dc:date>2008-02-29T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.081301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 081301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-02-29T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>081301</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.081102">
    <title>Deformations of the Constraint Algebra of Ashtekar&#8217;s Hamiltonian Formulation of General Relativity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.081102</link>
    <description>Author(s): Kirill Krasnov&lt;br/&gt;We show that the constraint algebra of Ashtekar&#8217;s Hamiltonian formulation of general relativity can be nontrivially deformed by allowing the cosmological constant to become an arbitrary function of the (Weyl) curvature. Our result implies that there is not one but infinitely many (parametrized by ...&lt;br/&gt;[Phys. Rev. Lett. 100, 081102] Published Wed Feb 27, 2008</description>
    <dc:creator>Kirill Krasnov</dc:creator>
    <dc:date>2008-02-27T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.081102</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 081102</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-02-27T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>081102</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.081101">
    <title>Stability of Precessing Superfluid Neutron Stars</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.081101</link>
    <description>Author(s): K. Glampedakis, N. Andersson, and D. I. Jones&lt;br/&gt;We discuss a new superfluid instability occurring in the interior of mature neutron stars with implications for free precession. This instability is similar to the instability which is responsible for the formation of turbulence in superfluid helium. We demonstrate that the instability is unlikely t...&lt;br/&gt;&lt;img src="http://prola.aps.org/graphics/prlsugg30x30.gif" width="30" height="30" alt="PRL Editors' Suggestion"/&gt;&lt;br/&gt;[Phys. Rev. Lett. 100, 081101] Published Tue Feb 26, 2008</description>
    <dc:creator>K. Glampedakis, N. Andersson, and D. I. Jones</dc:creator>
    <dc:date>2008-02-26T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.081101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 081101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-02-26T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>081101</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.071301">
    <title>Nonlinear Evolution of Anisotropic Cosmological Power</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.071301</link>
    <description>Author(s): Shin&#8217;ichiro Ando and Marc Kamionkowski&lt;br/&gt;There has been growing interest in the possibility of testing more precisely the assumption of statistical isotropy of primordial density perturbations. If it is to be tested with galaxy surveys at distance scales &#8818;10&#8201;&#8201;Mpc, then nonlinear evolution of anisotropic power must be understood. To t...&lt;br/&gt;[Phys. Rev. Lett. 100, 071301] Published Thu Feb 21, 2008</description>
    <dc:creator>Shin&#8217;ichiro Ando and Marc Kamionkowski</dc:creator>
    <dc:date>2008-02-21T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.071301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 071301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>7</prism:issueIdentifier>
    <prism:publicationDate>2008-02-21T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>071301</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.061301">
    <title>Gamma-Ray Spectrum from Gravitino Dark Matter Decay</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.061301</link>
    <description>Author(s): Alejandro Ibarra and David Tran&lt;br/&gt;Gravitinos are very promising candidates for the cold dark matter of the Universe. Interestingly, to achieve a sufficiently long gravitino lifetime, R parity conservation is not required, thus preventing any dangerous cosmological influence of the next-to-lightest supersymmetric particle. When R par...&lt;br/&gt;[Phys. Rev. Lett. 100, 061301] Published Wed Feb 13, 2008</description>
    <dc:creator>Alejandro Ibarra and David Tran</dc:creator>
    <dc:date>2008-02-13T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.061301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 061301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>6</prism:issueIdentifier>
    <prism:publicationDate>2008-02-13T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>061301</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.100.051101">
    <title>Dark Matter and the First Stars: A New Phase of Stellar Evolution</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.100.051101</link>
    <description>Author(s): Douglas Spolyar, Katherine Freese, and Paolo Gondolo&lt;br/&gt;A mechanism is identified whereby dark matter (DM) in protostellar halos dramatically alters the current theoretical framework for the formation of the first stars. Heat from neutralino DM annihilation is shown to overwhelm any cooling mechanism, consequently impeding the star formation process and ...&lt;br/&gt;&lt;img src="http://prola.aps.org/graphics/prlsugg30x30.gif" width="30" height="30" alt="PRL Editors' Suggestion"/&gt;&lt;br/&gt;[Phys. Rev. Lett. 100, 051101] Published Mon Feb 04, 2008</description>
    <dc:creator>Douglas Spolyar, Katherine Freese, and Paolo Gondolo</dc:creator>
    <dc:date>2008-02-04T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.100.051101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 100, 051101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>100</prism:volume>
    <prism:issueIdentifier>5</prism:issueIdentifier>
    <prism:publicationDate>2008-02-04T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>051101</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
</rdf:RDF>
