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    <title>Cosmology with unparticles</title>
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    <description>Author(s): Bohdan Grzadkowski and Jos&#233; Wudka&lt;br/&gt;We discuss cosmological consequences of the existence of physics beyond the standard model that exhibits Banks-Zaks and unparticle behavior in the UV and IR, respectively. We first derive the equation of state for unparticles and use it to obtain the temperature dependence of the corresponding energ...&lt;br/&gt;[Phys. Rev. D 80, 103518] Published Fri Nov 20, 2009</description>
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    <title>Impact of a strongly first-order phase transition on the abundance of thermal relics</title>
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    <description>Author(s): Carroll Wainwright and Stefano Profumo&lt;br/&gt;We study the impact of a strongly first-order electroweak phase transition on the thermal relic abundance of particle species that could constitute the dark matter and that decoupled before the phase transition occurred. We define a dilution factor induced by generic first-order phase transitions, a...&lt;br/&gt;[Phys. Rev. D 80, 103517] Published Thu Nov 19, 2009</description>
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    <title>CMB lensing constraints on dark energy and modified gravity scenarios</title>
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    <description>Author(s): Erminia Calabrese, Asantha Cooray, Matteo Martinelli, Alessandro Melchiorri, Luca Pagano, An&#382;e Slosar, and George F. Smoot&lt;br/&gt;Weak gravitational lensing leaves a characteristic imprint on the cosmic microwave background temperature and polarization angular power spectra. Here, we investigate the possible constraints on the integrated lensing potential from future cosmic microwave background angular spectra measurements exp...&lt;br/&gt;[Phys. Rev. D 80, 103516] Published Thu Nov 19, 2009</description>
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    <description>Author(s): Andrzej Odrzywo&#322;ek&lt;br/&gt;A spherically symmetric, static model of the cosmological voids is constructed in the framework of the Tolman-Oppenheimer-Volkov equation with the cosmological constant. Extension of the Tooper result (dimensionless form of the TOV equation) is provided for nonzero &#923;. Then, the equation is simplifi...&lt;br/&gt;[Phys. Rev. D 80, 103515] Published Tue Nov 17, 2009</description>
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    <title>Cosmic steps in modeling dark energy</title>
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    <description>Author(s): Tower Wang&lt;br/&gt;Past and recent data analyses gave some hints of steps in dark energy. Considering dark energy as a dynamical scalar field, we investigate several models with various steps: a step in the scalar potential, a step in the kinetic term, a step in the energy density, and a step in the equation-of-state ...&lt;br/&gt;&lt;img src="http://prola.aps.org/graphics/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/&gt;&lt;br/&gt;[Phys. Rev. D 80, 101302] Published Tue Nov 17, 2009</description>
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    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
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    <title>Constraint on coupled dark energy models from observations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103514</link>
    <description>Author(s): Jun-Qing Xia&lt;br/&gt;The coupled dark energy models, in which the quintessence scalar field nontrivially couples to the cold dark matter, have been proposed to explain the coincidence problem. In this paper we study the perturbations of coupled dark energy models and the effects of this interaction on the current observ...&lt;br/&gt;[Phys. Rev. D 80, 103514] Published Mon Nov 16, 2009</description>
    <dc:creator>Jun-Qing Xia</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/PhysRevD.80.103514</dc:identifier>
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    <title>Assisted dark energy</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103513</link>
    <description>Author(s): Junko Ohashi and Shinji Tsujikawa&lt;br/&gt;Cosmological scaling solutions, which give rise to a scalar-field density proportional to a background fluid density during radiation and matter eras, are attractive to alleviate the energy scale problem of dark energy. In the presence of multiple scalar fields, the scaling solution can exit to the ...&lt;br/&gt;[Phys. Rev. D 80, 103513] Published Mon Nov 16, 2009</description>
    <dc:creator>Junko Ohashi and Shinji Tsujikawa</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/PhysRevD.80.103513</dc:identifier>
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    <title>Sensitivity of cosmic-ray experiments to ultrahigh-energy photons: Reconstruction of the spectrum and limits on the superheavy dark matter</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103006</link>
    <description>Author(s): O. E. Kalashev, G. I. Rubtsov, and S. V. Troitsky&lt;br/&gt;We estimate the sensitivity of various experiments detecting ultrahigh-energy cosmic rays to primary photons with energies above 10^{19} &#8201;&#8201;eV. We demonstrate that the energy of a primary photon may be significantly (up to a factor of &#8764;10) underestimated or overestimated for particular primary ...&lt;br/&gt;[Phys. Rev. D 80, 103006] Published Mon Nov 16, 2009</description>
    <dc:creator>O. E. Kalashev, G. I. Rubtsov, and S. V. Troitsky</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/PhysRevD.80.103006</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103006</dc:source>
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    <title>Inflaton two-point correlation in the presence of a cosmic string</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103512</link>
    <description>Author(s): Chien-Yao Tseng and Mark B. Wise&lt;br/&gt;Precise measurements of the microwave background anisotropy have confirmed the inflationary picture of approximately scale invariant, Gaussian primordial adiabatic density perturbations. However, there are some anomalies that suggest a small violation of rotational and/or translational invariance in...&lt;br/&gt;[Phys. Rev. D 80, 103512] Published Fri Nov 13, 2009</description>
    <dc:creator>Chien-Yao Tseng and Mark B. Wise</dc:creator>
    <dc:date>2009-11-13T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103512</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103512</dc:source>
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    <title>Sterile neutrinos produced near the electroweak scale: Mixing angles, MSW resonances, and production rates</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103511</link>
    <description>Author(s): Jun Wu, Chiu Man Ho, and Daniel Boyanovsky&lt;br/&gt;We study the production of sterile neutrinos in the region T&#8764;M_{W} in an extension beyond the standard model with the seesaw mass matrix originating in Yukawa couplings to Higgs-like scalars with masses and vev&#8217;s of the order of the electroweak scale. Sterile neutrinos are produced by the decay ...&lt;br/&gt;[Phys. Rev. D 80, 103511] Published Fri Nov 13, 2009</description>
    <dc:creator>Jun Wu, Chiu Man Ho, and Daniel Boyanovsky</dc:creator>
    <dc:date>2009-11-13T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103511</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103511</dc:source>
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    <title>Multimessenger constraints on the annihilating dark matter interpretation of the positron excess</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103510</link>
    <description>Author(s): Miguel Pato, Lidia Pieri, and Gianfranco Bertone&lt;br/&gt;The rise in the energy spectrum of the positron ratio, observed by the PAMELA satellite above 10&#160;GeV, and other cosmic-ray measurements, have been interpreted as a possible signature of dark matter annihilation in the Galaxy. However, the large number of free parameters, and the large astrophysical...&lt;br/&gt;[Phys. Rev. D 80, 103510] Published Fri Nov 13, 2009</description>
    <dc:creator>Miguel Pato, Lidia Pieri, and Gianfranco Bertone</dc:creator>
    <dc:date>2009-11-13T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103510</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103510</dc:source>
    <dc:format>text/html</dc:format>
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    <title>Inflation and dark energy from three-forms</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103509</link>
    <description>Author(s): Tomi S. Koivisto and Nelson J. Nunes&lt;br/&gt;Three-forms can give rise to viable cosmological scenarios of inflation and dark energy with potentially observable signatures distinct from standard single scalar field models. In this study, the background dynamics and linear perturbations of self-interacting three-form cosmology are investigated....&lt;br/&gt;[Phys. Rev. D 80, 103509] Published Thu Nov 12, 2009</description>
    <dc:creator>Tomi S. Koivisto and Nelson J. Nunes</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/PhysRevD.80.103509</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103509</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2009-11-12T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103509</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103005" 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>Determination of the neutrino flavor ratio at the astrophysical source</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103005</link>
    <description>Author(s): Kwang-Chang Lai, Guey-Lin Lin, and T. C. Liu&lt;br/&gt;We discuss the reconstruction of neutrino flavor ratios at astrophysical sources through the future neutrino-telescope measurements. Taking the ranges of neutrino mixing parameters &#952;_{ij} as those given by the current global fit, we demonstrate by a statistical method that the accuracies in the mea...&lt;br/&gt;[Phys. Rev. D 80, 103005] Published Wed Nov 11, 2009</description>
    <dc:creator>Kwang-Chang Lai, Guey-Lin Lin, and T. C. Liu</dc:creator>
    <dc:date>2009-11-11T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103005</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103005</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
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    <prism:publicationDate>2009-11-11T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103005</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103508" 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>Unified model of k-inflation, dark matter, and dark energy</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103508</link>
    <description>Author(s): Nilok Bose and A. S. Majumdar&lt;br/&gt;We present a k-essence model where a single scalar field is responsible for the early expansion of the Universe through the process of k inflation and at appropriate subsequent stages acts both as dark matter and dark energy. The Lagrangian contains a potential for the scalar field as well as a nonc...&lt;br/&gt;[Phys. Rev. D 80, 103508] Published Tue Nov 10, 2009</description>
    <dc:creator>Nilok Bose and A. S. Majumdar</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/PhysRevD.80.103508</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103508</dc:source>
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    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
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    <prism:startingPage>103508</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.101301" 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>Is cosmic acceleration slowing down?</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.101301</link>
    <description>Author(s): Arman Shafieloo, Varun Sahni, and Alexei A. Starobinsky&lt;br/&gt;We investigate the course of cosmic expansion in its recent past using the Constitution SN Ia sample, along with baryon acoustic oscillations (BAO) and cosmic microwave background (CMB) data. Allowing the equation of state of dark energy (DE) to vary, we find that a coasting model of the universe (q...&lt;br/&gt;&lt;img src="http://prola.aps.org/graphics/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/&gt;&lt;br/&gt;[Phys. Rev. D 80, 101301] Published Mon Nov 09, 2009</description>
    <dc:creator>Arman Shafieloo, Varun Sahni, and Alexei A. Starobinsky</dc:creator>
    <dc:date>2009-11-09T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.101301</dc:identifier>
    <dc:source>Phys. Rev. D 80, 101301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:publicationDate>2009-11-09T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>101301</prism:startingPage>
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    <prism:section>D15</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103507" 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>Gauge-invariant construction of quantum cosmology</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103507</link>
    <description>Author(s): Fumitoshi Amemiya and Tatsuhiko Koike&lt;br/&gt;We present and analyze a gauge-invariant quantum theory of the Friedmann-Robertson-Walker universe with dust. We construct the reduced phase space spanned by gauge-invariant quantities by using the so-called relational formalism at the classical level. The reduced phase space thereby obtained can be...&lt;br/&gt;[Phys. Rev. D 80, 103507] Published Fri Nov 06, 2009</description>
    <dc:creator>Fumitoshi Amemiya and Tatsuhiko Koike</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/PhysRevD.80.103507</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103507</dc:source>
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    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:publicationDate>2009-11-06T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103507</prism:startingPage>
    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103506" 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>Incompatibility of rotation curves with gravitational lensing for TeVeS theory</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103506</link>
    <description>Author(s): Ignacio Ferreras, Nick E. Mavromatos, Mairi Sakellariadou, and Muhammad Furqaan Yusaf&lt;br/&gt;We constrain the one-parameter (&#945;) class of TeVeS models by testing the theory against both rotation curve and strong gravitational lensing data on galactic scales, remaining fully relativistic in our formalism. The upshot of our analysis is that&#8212;at least in its simplest original form, which is t...&lt;br/&gt;[Phys. Rev. D 80, 103506] Published Fri Nov 06, 2009</description>
    <dc:creator>Ignacio Ferreras, Nick E. Mavromatos, Mairi Sakellariadou, and Muhammad Furqaan Yusaf</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/PhysRevD.80.103506</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103506</dc:source>
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    <prism:publicationName>Physical Review D</prism:publicationName>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103004" 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>Present and future gamma-ray probes of the Cygnus OB2 environment</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103004</link>
    <description>Author(s): Luis A. Anchordoqui, Haim Goldberg, Russell D. Moore, Sergio Palomares-Ruiz, Diego F. Torres, and Thomas J. Weiler&lt;br/&gt;The MAGIC Collaboration has provided new observational data pertaining to the TeV J2032+4130 gamma-ray source (within the Cygnus OB2 region), for energies E_{&#947;} &gt;400&#8201;&#8201;GeV. It is then appropriate to update the impact of these data on gamma-ray production mechanisms in stellar associations. We con...&lt;br/&gt;[Phys. Rev. D 80, 103004] Published Fri Nov 06, 2009</description>
    <dc:creator>Luis A. Anchordoqui, Haim Goldberg, Russell D. Moore, Sergio Palomares-Ruiz, Diego F. Torres, and Thomas J. Weiler</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/PhysRevD.80.103004</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103004</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:publicationDate>2009-11-06T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103004</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103505" 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>Exact cosmological solutions with nonminimal derivative coupling</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103505</link>
    <description>Author(s): Sergey V. Sushkov&lt;br/&gt;We consider a gravitational theory of a scalar field &#981; with nonminimal derivative coupling to curvature. The coupling terms have the form &#954;_{1} R&#981;_{,&#956;} &#981;^{,&#956;} and &#954;_{2} R_{&#956;&#957;} &#981;^{,&#956;} &#981;^{,&#957;} , where &#954;_{1} and &#954;_{2} are coupling parameters with dimensions of length squared. In general, ...&lt;br/&gt;[Phys. Rev. D 80, 103505] Published Thu Nov 05, 2009</description>
    <dc:creator>Sergey V. Sushkov</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103505</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103505</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103505</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103504" 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>Inflation, baryogenesis, and gravitino dark matter at ultralow reheat temperatures</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103504</link>
    <description>Author(s): Kazunori Kohri, Anupam Mazumdar, and Narendra Sahu&lt;br/&gt;It is quite possible that the reheat temperature of the Universe is extremely low close to the scale of big bang nucleosynthesis, i.e. T_{R} &#8764;1&#8211;10&#8201;&#8201;MeV. At such low reheat temperatures generating matter, antimatter asymmetry and synthesizing dark matter particles are challenging issues which...&lt;br/&gt;[Phys. Rev. D 80, 103504] Published Thu Nov 05, 2009</description>
    <dc:creator>Kazunori Kohri, Anupam Mazumdar, and Narendra Sahu</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103504</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103504</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103503" 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>Archipelagian cosmology: Dynamics and observables in a universe with discretized matter content</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103503</link>
    <description>Author(s): Timothy Clifton and Pedro G. Ferreira&lt;br/&gt;We consider a model of the Universe in which the matter content is in the form of discrete islands, rather than a continuous fluid. In the appropriate limits the resulting large-scale dynamics approach those of a Friedmann-Robertson-Walker (FRW) universe. The optical properties of such a space-time,...&lt;br/&gt;[Phys. Rev. D 80, 103503] Published Thu Nov 05, 2009</description>
    <dc:creator>Timothy Clifton and Pedro G. Ferreira</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103503</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103503</dc:source>
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    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103503</prism:startingPage>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103003" 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>Reconstructing the neutron-star equation of state from astrophysical measurements</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103003</link>
    <description>Author(s): Feryal &#214;zel and Dimitrios Psaltis&lt;br/&gt;The properties of matter at ultrahigh densities, low temperatures, and with a significant asymmetry between protons and neutrons can be studied exclusively through astrophysical observations of neutron stars. We show that measurements of the masses and radii of neutron stars can lead to tight constr...&lt;br/&gt;[Phys. Rev. D 80, 103003] Published Thu Nov 05, 2009</description>
    <dc:creator>Feryal &#214;zel and Dimitrios Psaltis</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103003</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103003</dc:source>
    <dc:format>text/html</dc:format>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103002" 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>The G&#246;del universe: Exact geometrical optics and analytical investigations on motion</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103002</link>
    <description>Author(s): Frank Grave, Michael Buser, Thomas M&#252;ller, G&#252;nter Wunner, and Wolfgang P. Schleich&lt;br/&gt;In this work we derive the analytical solution of the geodesic equations of G&#246;del&#8217;s universe for both particles and light in a special set of coordinates, which reveals the physical properties of this spacetime in a very transparent way. We also recapitulate the equations of isometric transport f...&lt;br/&gt;[Phys. Rev. D 80, 103002] Published Thu Nov 05, 2009</description>
    <dc:creator>Frank Grave, Michael Buser, Thomas M&#252;ller, G&#252;nter Wunner, and Wolfgang P. Schleich</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103002</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103002</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
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    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103502" 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>Nonthermal production of WIMPs, cosmic e^{&#177;}  excesses, and &#947; rays from the Galactic Center</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103502</link>
    <description>Author(s): Xiao-Jun Bi, Robert Brandenberger, Paolo Gondolo, Tianjun Li, Qiang Yuan, and Xinmin Zhang&lt;br/&gt;In this paper we propose a dark matter model and study aspects of its phenomenology. Our model is based on a new dark matter sector with a U(1)^{&#8242;} gauge symmetry plus a discrete symmetry added to the standard model of particle physics. The new fields of the dark matter sector have no hadronic cha...&lt;br/&gt;[Phys. Rev. D 80, 103502] Published Wed Nov 04, 2009</description>
    <dc:creator>Xiao-Jun Bi, Robert Brandenberger, Paolo Gondolo, Tianjun Li, Qiang Yuan, and Xinmin Zhang</dc:creator>
    <dc:date>2009-11-04T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103502</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103502</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:publicationDate>2009-11-04T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103502</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103501" 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>Effect of long-lived strongly interacting relic particles on big bang nucleosynthesis</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103501</link>
    <description>Author(s): Motohiko Kusakabe, Toshitaka Kajino, Takashi Yoshida, and Grant J. Mathews&lt;br/&gt;It has been suggested that relic long-lived strongly interacting massive particles (SIMPs, or X particles) existed in the early universe. We study effects of such long-lived unstable SIMPs on big bang nucleosynthesis (BBN) assuming that such particles existed during the BBN epoch, but then decayed l...&lt;br/&gt;[Phys. Rev. D 80, 103501] Published Mon Nov 02, 2009</description>
    <dc:creator>Motohiko Kusakabe, Toshitaka Kajino, Takashi Yoshida, and Grant J. Mathews</dc:creator>
    <dc:date>2009-11-02T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103501</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103501</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2009-11-02T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103501</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103001" 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>Demagnified gravitational waves from cosmological double neutron stars and gravitational wave foreground cleaning around 1&#160;Hz</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103001</link>
    <description>Author(s): Naoki Seto&lt;br/&gt;Gravitational waves (GWs) from cosmological double neutron star binaries (NS+NS) can be significantly demagnified by the strong gravitational lensing effect, and the proposed future missions such as the Big Bang Observer or Deci-hertz Interferometer Gravitational Wave Observatory might miss some of ...&lt;br/&gt;[Phys. Rev. D 80, 103001] Published Mon Nov 02, 2009</description>
    <dc:creator>Naoki Seto</dc:creator>
    <dc:date>2009-11-02T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103001</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103001</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2009-11-02T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103001</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.083534" 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>Does dark matter consist of baryons of new stable family quarks?</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.083534</link>
    <description>Author(s): G. Bregar and N. S. Manko&#269; Bor&#353;tnik&lt;br/&gt;We investigate the possibility that the dark matter consists of clusters of the heavy family quarks and leptons with zero Yukawa couplings to the lower families. Such a family is predicted by the approach unifying spin and charges as the fifth family. We make a rough estimation of properties of bary...&lt;br/&gt;[Phys. Rev. D 80, 083534] Published Fri Oct 30, 2009</description>
    <dc:creator>G. Bregar and N. S. Manko&#269; Bor&#353;tnik</dc:creator>
    <dc:date>2009-10-30T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.083534</dc:identifier>
    <dc:source>Phys. Rev. D 80, 083534</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2009-10-30T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>083534</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.083533" 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 dark fluid</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.083533</link>
    <description>Author(s): Martin Kunz, Andrew R. Liddle, David Parkinson, and Changjun Gao&lt;br/&gt;Cosmological observations are normally fit under the assumption that the dark sector can be decomposed into dark matter and dark energy components. However, as long as the probes remain purely gravitational, there is no unique decomposition and observations can only constrain a single dark fluid; th...&lt;br/&gt;[Phys. Rev. D 80, 083533] Published Fri Oct 30, 2009</description>
    <dc:creator>Martin Kunz, Andrew R. Liddle, David Parkinson, and Changjun Gao</dc:creator>
    <dc:date>2009-10-30T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.083533</dc:identifier>
    <dc:source>Phys. Rev. D 80, 083533</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2009-10-30T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>083533</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.083011" 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>Magnetic seed field generation from electroweak bubble collisions with bubble walls of finite thickness</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.083011</link>
    <description>Author(s): Trevor Stevens and Mikkel B. Johnson&lt;br/&gt;Building on earlier work, we develop an equation-of-motion method for calculating magnetic seed fields generated from currents arising from charged W^{&#177;} fields in bubble collisions during a first-order primordial electroweak phase transition allowed in some proposed extensions of the standard mode...&lt;br/&gt;[Phys. Rev. D 80, 083011] Published Fri Oct 30, 2009</description>
    <dc:creator>Trevor Stevens and Mikkel B. Johnson</dc:creator>
    <dc:date>2009-10-30T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.083011</dc:identifier>
    <dc:source>Phys. Rev. D 80, 083011</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2009-10-30T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>083011</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.083532" 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>Null energy condition violation and classical stability in the Bianchi&#160;I metric</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.083532</link>
    <description>Author(s): I. Ya. Aref&#8217;eva, N. V. Bulatov, L. V. Joukovskaya, and S. Yu. Vernov&lt;br/&gt;The stability of isotropic cosmological solutions in the Bianchi&#160;I model is considered. We prove that the stability of isotropic solutions in the Bianchi&#160;I metric for a positive Hubble parameter follows from their stability in the Friedmann-Robertson-Walker metric. This result is applied to models...&lt;br/&gt;[Phys. Rev. D 80, 083532] Published Thu Oct 29, 2009</description>
    <dc:creator>I. Ya. Aref&#8217;eva, N. V. Bulatov, L. V. Joukovskaya, and S. Yu. Vernov</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/PhysRevD.80.083532</dc:identifier>
    <dc:source>Phys. Rev. D 80, 083532</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2009-10-29T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>083532</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
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