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    <title>Gamma Rays from Ultracompact Primordial Dark Matter Minihalos</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.211301</link>
    <description>Author(s): Pat Scott and Sofia Sivertsson&lt;br/&gt;Ultracompact minihalos have been proposed as a new class of dark matter structure. They would be produced by phase transitions in the early Universe or features in the inflaton potential, and constitute nonbaryonic massive compact halo objects today. We examine the prospects of detecting these minih...&lt;br/&gt;[Phys. Rev. Lett. 103, 211301] Published Fri Nov 20, 2009</description>
    <dc:creator>Pat Scott and Sofia Sivertsson</dc:creator>
    <dc:date>2009-11-20T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.211301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 211301</dc:source>
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    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>21</prism:issueIdentifier>
    <prism:publicationDate>2009-11-20T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>211301</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.103.211102" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Supersoft Symmetry Energy Encountering Non-Newtonian Gravity in Neutron Stars</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.211102</link>
    <description>Author(s): De-Hua Wen, Bao-An Li, and Lie-Wen Chen&lt;br/&gt;Considering the non-Newtonian gravity proposed in grand unification theories, we show that the stability and observed global properties of neutron stars cannot rule out the supersoft nuclear symmetry energies at suprasaturation densities. The degree of possible violation of the inverse-square law of...&lt;br/&gt;[Phys. Rev. Lett. 103, 211102] Published Mon Nov 16, 2009</description>
    <dc:creator>De-Hua Wen, Bao-An Li, and Lie-Wen Chen</dc:creator>
    <dc:date>2009-11-16T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.211102</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 211102</dc:source>
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    <prism:publicationDate>2009-11-16T00:00:00-05:00</prism:publicationDate>
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    <title>Magnetic Fluctuation Power Near Proton Temperature Anisotropy Instability Thresholds in the Solar Wind</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.211101</link>
    <description>Author(s): S. D. Bale, J. C. Kasper, G. G. Howes, E. Quataert, C. Salem, and D. Sundkvist&lt;br/&gt;The proton temperature anisotropy in the solar wind is known to be constrained by the theoretical thresholds for pressure-anisotropy-driven instabilities. Here, we use approximately 1&#215;10^{6} independent measurements of gyroscale magnetic fluctuations in the solar wind to show for the first time tha...&lt;br/&gt;[Phys. Rev. Lett. 103, 211101] Published Mon Nov 16, 2009</description>
    <dc:creator>S. D. Bale, J. C. Kasper, G. G. Howes, E. Quataert, C. Salem, and D. Sundkvist</dc:creator>
    <dc:date>2009-11-16T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.211101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 211101</dc:source>
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    <title>Recovering General Relativity from Massive Gravity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.201102</link>
    <description>Author(s): E. Babichev, C. Deffayet, and R. Ziour&lt;br/&gt;We obtain static, spherically symmetric, and asymptotically flat numerical solutions of massive gravity with a source. Those solutions show, for the first time explicitly, a recovery of the Schwarzschild solution of general relativity via the so-called Vainshtein mechanism.&lt;br/&gt;[Phys. Rev. Lett. 103, 201102] Published Thu Nov 12, 2009</description>
    <dc:creator>E. Babichev, C. Deffayet, and R. Ziour</dc:creator>
    <dc:date>2009-11-12T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.201102</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 201102</dc:source>
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    <prism:publicationName>Physical Review Letters</prism:publicationName>
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    <prism:publicationDate>2009-11-12T00:00:00-05:00</prism:publicationDate>
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    <title>Turbulent Cascade at 1&#160;AU in High Cross-Helicity Flows</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.201101</link>
    <description>Author(s): Charles W. Smith, Joshua E. Stawarz, Bernard J. Vasquez, Miriam A. Forman, and Benjamin T. MacBride&lt;br/&gt;Analysis of the scaling of the mixed third moments of velocity and magnetic fluctuations in the solar wind plasma, and the energy cascade rates derived from the scaling, reveal a strong dependence on the amount of cross-field correlation between the velocity and magnetic field fluctuations. When the...&lt;br/&gt;[Phys. Rev. Lett. 103, 201101] Published Tue Nov 10, 2009</description>
    <dc:creator>Charles W. Smith, Joshua E. Stawarz, Bernard J. Vasquez, Miriam A. Forman, and Benjamin T. MacBride</dc:creator>
    <dc:date>2009-11-10T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.201101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 201101</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:publicationName>Physical Review Letters</prism:publicationName>
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    <prism:publicationDate>2009-11-10T00:00:00-05:00</prism:publicationDate>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.103.191301" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Improved Flux Limits for Neutrinos with Energies above 10^{22} &#8201;&#8201;eV from Observations with the Westerbork Synthesis Radio Telescope</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.191301</link>
    <description>Author(s): O. Scholten, S. Buitink, J. Bacelar, R. Braun, A. G. de Bruyn, H. Falcke, K. Singh, B. Stappers, R. G. Strom, and R. al Yahyaoui&lt;br/&gt;Particle cascades initiated by ultrahigh energy neutrinos in the lunar regolith will emit an electromagnetic pulse with a time duration of the order of nanoseconds through a process known as the Askaryan effect. It has been shown that in an observing window around 150&#160;MHz there is a maximum chance ...&lt;br/&gt;[Phys. Rev. Lett. 103, 191301] Published Fri Nov 06, 2009</description>
    <dc:creator>O. Scholten, S. Buitink, J. Bacelar, R. Braun, A. G. de Bruyn, H. Falcke, K. Singh, B. Stappers, R. G. Strom, and R. al Yahyaoui</dc:creator>
    <dc:date>2009-11-06T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.191301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 191301</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
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    <prism:publicationDate>2009-11-06T00:00:00-05:00</prism:publicationDate>
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    <title>Gamma Rays from Dark Matter Annihilations Strongly Constrain the Substructure in Halos</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.181302</link>
    <description>Author(s): Anders Pinzke, Christoph Pfrommer, and Lars Bergstr&#246;m&lt;br/&gt;To fit recent data, e^{&#177;} from dark matter (DM) needs a boosted annihilation rate. This may imply an observable level of gamma rays from nearby galaxy clusters for the Fermi satellite. Using EGRET data, we limit the minimum mass of DM substructures to be about 5&#215;10^{3} times larger than for cold D...&lt;br/&gt;[Phys. Rev. Lett. 103, 181302] Published Thu Oct 29, 2009</description>
    <dc:creator>Anders Pinzke, Christoph Pfrommer, and Lars Bergstr&#246;m</dc:creator>
    <dc:date>2009-10-29T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.181302</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 181302</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:publicationName>Physical Review Letters</prism:publicationName>
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    <title>Rotation of Galaxies as a Signature of Cosmic Strings in Weak Lensing Surveys</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.181301</link>
    <description>Author(s): Daniel B. Thomas, Carlo R. Contaldi, and Jo&#227;o Magueijo&lt;br/&gt;Vector perturbations sourced by topological defects can generate rotations in the lensing of background galaxies. This is a potential smoking gun for the existence of defects since rotation generates a curl-like component in the weak lensing signal which is not generated by standard density perturba...&lt;br/&gt;[Phys. Rev. Lett. 103, 181301] Published Wed Oct 28, 2009</description>
    <dc:creator>Daniel B. Thomas, Carlo R. Contaldi, and Jo&#227;o Magueijo</dc:creator>
    <dc:date>2009-10-28T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.181301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 181301</dc:source>
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    <title>Exploiting Large-Scale Correlations to Detect Continuous Gravitational Waves</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.181102</link>
    <description>Author(s): Holger J. Pletsch and Bruce Allen&lt;br/&gt;Fully coherent searches (over realistic ranges of parameter space and year-long observation times) for unknown sources of continuous gravitational waves are computationally prohibitive. Less expensive hierarchical searches divide the data into shorter segments which are analyzed coherently, then det...&lt;br/&gt;[Phys. Rev. Lett. 103, 181102] Published Tue Oct 27, 2009</description>
    <dc:creator>Holger J. Pletsch and Bruce Allen</dc:creator>
    <dc:date>2009-10-27T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.181102</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 181102</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
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    <prism:publicationDate>2009-10-27T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>181102</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.103.181101" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Constraints on Neutron Star Crusts from Oscillations in Giant Flares</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.181101</link>
    <description>Author(s): Andrew W. Steiner and Anna L. Watts&lt;br/&gt;We show that the fundamental seismic shear mode, observed as a quasiperiodic oscillation in giant flares emitted by highly magnetized neutron stars, is particularly sensitive to the nuclear physics of the crust. The identification of an oscillation at &#8776;30&#8201;&#8201;Hz as the fundamental crustal shear m...&lt;br/&gt;[Phys. Rev. Lett. 103, 181101] Published Mon Oct 26, 2009</description>
    <dc:creator>Andrew W. Steiner and Anna L. Watts</dc:creator>
    <dc:date>2009-10-26T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.181101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 181101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
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    <prism:publicationDate>2009-10-26T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>181101</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.103.171102" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>New Possible Quark-Hadron Mixed Phase in Protoneutron Stars</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.171102</link>
    <description>Author(s): G. Pagliara, M. Hempel, and J. Schaffner-Bielich&lt;br/&gt;The transition from hadronic to quark matter at high density is a strong first order phase transition if the surface tension between the two phases is large. While this implies a constant-pressure mixed phase in cold neutron star matter this is not the case for the hot and lepton rich matter of prot...&lt;br/&gt;[Phys. Rev. Lett. 103, 171102] Published Fri Oct 23, 2009</description>
    <dc:creator>G. Pagliara, M. Hempel, and J. Schaffner-Bielich</dc:creator>
    <dc:date>2009-10-23T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.171102</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 171102</dc:source>
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    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>17</prism:issueIdentifier>
    <prism:publicationDate>2009-10-23T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>171102</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.103.171101" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Development of a Displacement- and Frequency-Noise-Free Interferometer in a 3D Configuration for Gravitational Wave Detection</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.171101</link>
    <description>Author(s): Keiko Kokeyama, Shuichi Sato, Atsushi Nishizawa, Seiji Kawamura, Yanbei Chen, and Akio Sugamoto&lt;br/&gt;The displacement- and frequency-noise-free interferometer (DFI) is a multiple laser interferometer array for gravitational-wave detection free from both the displacement noise of optics and laser frequency noise. So far, partial experimental demonstrations of the DFI have been done in 2D table top e...&lt;br/&gt;[Phys. Rev. Lett. 103, 171101] Published Thu Oct 22, 2009</description>
    <dc:creator>Keiko Kokeyama, Shuichi Sato, Atsushi Nishizawa, Seiji Kawamura, Yanbei Chen, and Akio Sugamoto</dc:creator>
    <dc:date>2009-10-22T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.171101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 171101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>17</prism:issueIdentifier>
    <prism:publicationDate>2009-10-22T00:00:00-04:00</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.103.171302" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Constraining the Energy-Momentum Dispersion Relation with Planck-Scale Sensitivity Using Cold Atoms</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.171302</link>
    <description>Author(s): Giovanni Amelino-Camelia, Claus Laemmerzahl, Flavio Mercati, and Guglielmo M. Tino&lt;br/&gt;We use the results of ultraprecise cold-atom-recoil experiments to constrain the form of the energy-momentum dispersion relation, a structure that is expected to be modified in several quantum-gravity approaches. Our strategy of analysis applies to the nonrelativistic (small speeds) limit of the dis...&lt;br/&gt;[Phys. Rev. Lett. 103, 171302] Published Wed Oct 21, 2009</description>
    <dc:creator>Giovanni Amelino-Camelia, Claus Laemmerzahl, Flavio Mercati, and Guglielmo M. Tino</dc:creator>
    <dc:date>2009-10-21T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.171302</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 171302</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>17</prism:issueIdentifier>
    <prism:publicationDate>2009-10-21T00:00:00-04:00</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.103.171301" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Cosmic Neutrino Last Scattering Surface</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.171301</link>
    <description>Author(s): Scott Dodelson and Mika Vesterinen&lt;br/&gt;Neutrinos decoupled from the rest of the cosmic plasma when the Universe was less than one second old, far earlier than the photons, which decoupled at t=380&#8201;000 years. Surprisingly, though, the last scattering surface of massive neutrinos is much closer to us than that of the photons. Here we cal...&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. 103, 171301] Published Mon Oct 19, 2009</description>
    <dc:creator>Scott Dodelson and Mika Vesterinen</dc:creator>
    <dc:date>2009-10-19T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.171301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 171301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>17</prism:issueIdentifier>
    <prism:publicationDate>2009-10-19T00:00:00-04:00</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.103.161301" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Intermediate Mass Black Holes and Nearby Dark Matter Point Sources: A Critical Reassessment</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.161301</link>
    <description>Author(s): Torsten Bringmann, Julien Lavalle, and Pierre Salati&lt;br/&gt;Dark matter (DM) &#8220;minispikes&#8221; around intermediate mass black holes are sometimes quoted as one of the most promising targets for indirect DM searches. Here, we stress that existing cosmic ray data place severe constraints on the possibility to detect DM annihilation signals from these objects in...&lt;br/&gt;[Phys. Rev. Lett. 103, 161301] Published Fri Oct 16, 2009</description>
    <dc:creator>Torsten Bringmann, Julien Lavalle, and Pierre Salati</dc:creator>
    <dc:date>2009-10-16T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.161301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 161301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>16</prism:issueIdentifier>
    <prism:publicationDate>2009-10-16T00:00:00-04:00</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.103.161101" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Instability of Higher-Dimensional Charged Black Holes in the de&#160;Sitter World</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.161101</link>
    <description>Author(s): R. A. Konoplya and A. Zhidenko&lt;br/&gt;We have shown that higher-dimensional Reissner&#8211;Nordstr&#246;m&#8211;de&#160;Sitter black holes are gravitationally unstable for large values of the electric charge and cosmological constant in D&#8805;7 space-time dimensions. We have found the shape of the slightly perturbed black hole at the threshold point of i...&lt;br/&gt;[Phys. Rev. Lett. 103, 161101] Published Mon Oct 12, 2009</description>
    <dc:creator>R. A. Konoplya and A. Zhidenko</dc:creator>
    <dc:date>2009-10-12T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.161101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 161101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>16</prism:issueIdentifier>
    <prism:publicationDate>2009-10-12T00:00:00-04:00</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.103.151303" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Roles of Dark Energy Perturbations in Dynamical Dark Energy Models: Can We Ignore Them?</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.151303</link>
    <description>Author(s): Chan-Gyung Park, Jai-chan Hwang, Jae-heon Lee, and Hyerim Noh&lt;br/&gt;We show the importance of properly including the perturbations of the dark energy component in the dynamical dark energy models based on a scalar field and modified gravity theories in order to meet with present and future observational precisions. Based on a simple scaling scalar field dark energy ...&lt;br/&gt;[Phys. Rev. Lett. 103, 151303] Published Fri Oct 09, 2009</description>
    <dc:creator>Chan-Gyung Park, Jai-chan Hwang, Jae-heon Lee, and Hyerim Noh</dc:creator>
    <dc:date>2009-10-09T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.151303</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 151303</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>15</prism:issueIdentifier>
    <prism:publicationDate>2009-10-09T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>151303</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.103.151302" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Limits on the Spin-Dependent WIMP-Nucleon Cross Sections from the First Science Run of the ZEPLIN-III Experiment</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.151302</link>
    <description>Author(s): V. N. Lebedenko et al.&lt;br/&gt;We present new experimental constraints on the WIMP-nucleon spin-dependent elastic cross sections using data from the first science run of ZEPLIN-III, a two-phase xenon experiment searching for galactic dark matter weakly interacting massive particles based at the Boulby mine. Analysis of &#226;&#710;&#188;450&#226;&#8364;&#8240;&#226;...&lt;br/&gt;[Phys. Rev. Lett. 103, 151302] Published Thu Oct 08, 2009</description>
    <dc:creator>V. N. Lebedenko et al.</dc:creator>
    <dc:date>2009-10-08T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.151302</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 151302</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>15</prism:issueIdentifier>
    <prism:publicationDate>2009-10-08T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>151302</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.103.151301" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Enhanced Dark Matter Annihilation Rate for Positron and Electron Excesses from Q-Ball Decay</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.151301</link>
    <description>Author(s): John McDonald&lt;br/&gt;We show that Q-ball decay in Affleck-Dine baryogenesis models can account for dark matter when the annihilation cross section is sufficiently enhanced to explain the positron and electron excesses observed by PAMELA, ATIC, and PPB-BETS. For Affleck-Dine baryogenesis along a d=6 flat direction, the r...&lt;br/&gt;[Phys. Rev. Lett. 103, 151301] Published Tue Oct 06, 2009</description>
    <dc:creator>John McDonald</dc:creator>
    <dc:date>2009-10-06T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.151301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 151301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>15</prism:issueIdentifier>
    <prism:publicationDate>2009-10-06T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>151301</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.103.141101" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Overspinning a Black Hole with a Test Body</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.141101</link>
    <description>Author(s): Ted Jacobson and Thomas P. Sotiriou&lt;br/&gt;It has long been known that a maximally spinning black hole cannot be overspun by tossing in a test body. Here we show that if instead the black hole starts out with below maximal spin, then indeed overspinning can be achieved. We find that requirements on the size and internal structure of the test...&lt;br/&gt;[Phys. Rev. Lett. 103, 141101] Published Mon Sep 28, 2009</description>
    <dc:creator>Ted Jacobson and Thomas P. Sotiriou</dc:creator>
    <dc:date>2009-09-28T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.141101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 141101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>14</prism:issueIdentifier>
    <prism:publicationDate>2009-09-28T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>141101</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.103.131301" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Black Hole Berry Phase</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.131301</link>
    <description>Author(s): Jan de Boer, Kyriakos Papadodimas, and Erik Verlinde&lt;br/&gt;Supersymmetric black holes are characterized by a large number of degenerate ground states. We argue that these black holes, like other quantum mechanical systems with such a degeneracy, are subject to a phenomenon which is called the geometric or Berry&#8217;s phase: under adiabatic variations of the b...&lt;br/&gt;[Phys. Rev. Lett. 103, 131301] Published Tue Sep 22, 2009</description>
    <dc:creator>Jan de Boer, Kyriakos Papadodimas, and Erik Verlinde</dc:creator>
    <dc:date>2009-09-22T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.131301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 131301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>13</prism:issueIdentifier>
    <prism:publicationDate>2009-09-22T00:00:00-04:00</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.103.131102" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Cross Section, Final Spin, and Zoom-Whirl Behavior in High-Energy Black-Hole Collisions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.131102</link>
    <description>Author(s): Ulrich Sperhake, Vitor Cardoso, Frans Pretorius, Emanuele Berti, Tanja Hinderer, and Nicolas Yunes&lt;br/&gt;We study the collision of two highly boosted equal-mass, nonrotating black holes with generic impact parameter. We find such systems to exhibit zoom-whirl behavior when fine-tuning the impact parameter. Near the threshold of immediate merger the remnant black-hole Kerr parameter can be near maximal ...&lt;br/&gt;[Phys. Rev. Lett. 103, 131102] Published Tue Sep 22, 2009</description>
    <dc:creator>Ulrich Sperhake, Vitor Cardoso, Frans Pretorius, Emanuele Berti, Tanja Hinderer, and Nicolas Yunes</dc:creator>
    <dc:date>2009-09-22T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.131102</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 131102</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>13</prism:issueIdentifier>
    <prism:publicationDate>2009-09-22T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>131102</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.103.131101" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Zoom-Whirl Orbits in Black Hole Binaries</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.131101</link>
    <description>Author(s): James Healy, Janna Levin, and Deirdre Shoemaker&lt;br/&gt;Zoom-whirl behavior has the reputation of being a rare phenomenon. The concern has been that gravitational radiation would drain angular momentum so rapidly that generic orbits would circularize before zoom-whirl behavior could play out, and only rare highly tuned orbits would retain their imprint. ...&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. 103, 131101] Published Tue Sep 22, 2009</description>
    <dc:creator>James Healy, Janna Levin, and Deirdre Shoemaker</dc:creator>
    <dc:date>2009-09-22T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.131101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 131101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>13</prism:issueIdentifier>
    <prism:publicationDate>2009-09-22T00:00:00-04:00</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.103.121102" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Cosmic-Ray Electron Injection from the Ionization of Nuclei</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.121102</link>
    <description>Author(s): Giovanni Morlino&lt;br/&gt;We show that the secondary electrons ejected from the ionization of heavy ions can be injected into the acceleration process that occurs at supernova remnant shocks. This electron injection mechanism works since ions are ionized during the acceleration when they move already with relativistic speed,...&lt;br/&gt;[Phys. Rev. Lett. 103, 121102] Published Tue Sep 15, 2009</description>
    <dc:creator>Giovanni Morlino</dc:creator>
    <dc:date>2009-09-15T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.121102</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 121102</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-09-15T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>121102</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.103.121301" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Galactic Substructure and Energetic Neutrinos from the Sun and Earth</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.121301</link>
    <description>Author(s): Savvas M. Koushiappas and Marc Kamionkowski&lt;br/&gt;We consider the effects of Galactic substructure on energetic neutrinos from annihilation of weakly interacting massive particles that have been captured by the Sun and Earth. Substructure gives rise to a time-varying capture rate and thus to time variation in the annihilation rate and resulting ene...&lt;br/&gt;[Phys. Rev. Lett. 103, 121301] Published Mon Sep 14, 2009</description>
    <dc:creator>Savvas M. Koushiappas and Marc Kamionkowski</dc:creator>
    <dc:date>2009-09-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.121301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 121301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-09-14T00:00:00-04:00</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.103.121101" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Formation of Nuclear &#8220;Pasta&#8221; in Supernovae</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.121101</link>
    <description>Author(s): Gentaro Watanabe, Hidetaka Sonoda, Toshiki Maruyama, Katsuhiko Sato, Kenji Yasuoka, and Toshikazu Ebisuzaki&lt;br/&gt;In supernova cores, nuclear &#8220;pasta&#8221; phases such as a triangular lattice of rodlike nuclei and layered structure of slablike nuclei are considered to exist. However, it is still unclear whether or not they are actually formed in collapsing supernova cores. Using ab&#160;initio simulations called quan...&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. 103, 121101] Published Mon Sep 14, 2009</description>
    <dc:creator>Gentaro Watanabe, Hidetaka Sonoda, Toshiki Maruyama, Katsuhiko Sato, Kenji Yasuoka, and Toshikazu Ebisuzaki</dc:creator>
    <dc:date>2009-09-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.121101</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 121101</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-09-14T00:00:00-04:00</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.103.111303" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Grand Unification Scale Primordial Black Holes: Consequences and Constraints</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.111303</link>
    <description>Author(s): Richard Anantua, Richard Easther, and John T. Giblin&lt;br/&gt;A population of very light primordial black holes which evaporate before nucleosynthesis begins is unconstrained unless the decaying black holes leave stable relics. We show that gravitons Hawking radiated from these black holes would source a substantial stochastic background of high frequency grav...&lt;br/&gt;[Phys. Rev. Lett. 103, 111303] Published Thu Sep 10, 2009</description>
    <dc:creator>Richard Anantua, Richard Easther, and John T. Giblin</dc:creator>
    <dc:date>2009-09-10T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.111303</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 111303</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>11</prism:issueIdentifier>
    <prism:publicationDate>2009-09-10T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>111303</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.103.111302" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Inhomogeneity in Cosmic Ray Sources as the Origin of the Electron Spectrum and the PAMELA Anomaly</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.111302</link>
    <description>Author(s): Nir J. Shaviv, Ehud Nakar, and Tsvi Piran&lt;br/&gt;We show that inhomogeneity of cosmic ray (CR) sources, due to the concentration of supernova remnants (SNRs) towards the galactic spiral arms, can naturally explain the anomalous increase in the positron/electron ratio observed by PAMELA. We consistently recover the observed positron fraction betwee...&lt;br/&gt;[Phys. Rev. Lett. 103, 111302] Published Thu Sep 10, 2009</description>
    <dc:creator>Nir J. Shaviv, Ehud Nakar, and Tsvi Piran</dc:creator>
    <dc:date>2009-09-10T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.111302</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 111302</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>11</prism:issueIdentifier>
    <prism:publicationDate>2009-09-10T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>111302</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.103.111102" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Kerr Black Holes as Particle Accelerators to Arbitrarily High Energy</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.111102</link>
    <description>Author(s): M&#225;ximo Ba&#241;ados, Joseph Silk, and Stephen M. West&lt;br/&gt;We show that intermediate mass black holes conjectured to be the early precursors of supermassive black holes and surrounded by relic cold dark matter density spikes can act as particle accelerators with collisions, in principle, at arbitrarily high center-of-mass energies in the case of Kerr black ...&lt;br/&gt;[Phys. Rev. Lett. 103, 111102] Published Thu Sep 10, 2009</description>
    <dc:creator>M&#225;ximo Ba&#241;ados, Joseph Silk, and Stephen M. West</dc:creator>
    <dc:date>2009-09-10T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.111102</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 111102</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>11</prism:issueIdentifier>
    <prism:publicationDate>2009-09-10T00:00:00-04:00</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.103.111301" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Bose-Einstein Condensation of Dark Matter Axions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevLett.103.111301</link>
    <description>Author(s): P. Sikivie and Q. Yang&lt;br/&gt;We show that cold dark matter axions thermalize and form a Bose-Einstein condensate (BEC). We obtain the axion state in a homogeneous and isotropic universe, and derive the equations governing small axion perturbations. Because they form a BEC, axions differ from ordinary cold dark matter in the non...&lt;br/&gt;[Phys. Rev. Lett. 103, 111301] Published Wed Sep 09, 2009</description>
    <dc:creator>P. Sikivie and Q. Yang</dc:creator>
    <dc:date>2009-09-09T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevLett.103.111301</dc:identifier>
    <dc:source>Phys. Rev. Lett. 103, 111301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review Letters</prism:publicationName>
    <prism:volume>103</prism:volume>
    <prism:issueIdentifier>11</prism:issueIdentifier>
    <prism:publicationDate>2009-09-09T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>111301</prism:startingPage>
    <dc:subject>Gravitation and Astrophysics</dc:subject>
    <prism:section>Gravitation and Astrophysics</prism:section>
  </item>
</rdf:RDF>
