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    <dc:date>2009-11-22T06:17:13-05:00</dc:date>
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    <title>Noether symmetry approach in phantom quintessence cosmology</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104030</link>
    <description>Author(s): S. Capozziello, E. Piedipalumbo, C. Rubano, and P. Scudellaro&lt;br/&gt;In the framework of phantom quintessence cosmology, we use the Noether Symmetry Approach to obtain general exact solutions for the cosmological equations. This result is achieved by the quintessential (phantom) potential determined by the existence of the symmetry itself. A comparison between the th...&lt;br/&gt;[Phys. Rev. D 80, 104030] Published Fri Nov 20, 2009</description>
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    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
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    <title>Lifshitz black hole in three dimensions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104029</link>
    <description>Author(s): Eloy Ay&#243;n-Beato, Alan Garbarz, Gaston Giribet, and Mokhtar Hassa&#239;ne&lt;br/&gt;We show that three-dimensional massive gravity admits Lifshitz metrics with generic values of the dynamical exponent z as exact solutions. At the point z=3, exact black hole solutions that are asymptotically Lifshitz arise. These spacetimes are three-dimensional analogues of those that were recently...&lt;br/&gt;[Phys. Rev. D 80, 104029] Published Fri Nov 20, 2009</description>
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    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
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    <title>Spin-spin interaction in the spin-precession equations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104028</link>
    <description>Author(s): J&#225;nos Maj&#225;r&lt;br/&gt;One of the most active field of research in general relativity is the description of the spin properties of astrophysical objects. The main tool in the description of the gravitational waves emitted by compact binary systems in the inspiral era is the post-Newtonian (PN) approximation, where spin ef...&lt;br/&gt;[Phys. Rev. D 80, 104028] Published Thu Nov 19, 2009</description>
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    <dc:date>2009-11-19T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104028</dc:identifier>
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    <title>Quantization of higher spin fields</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104027</link>
    <description>Author(s): J. W. Wagenaar and T. A. Rijken&lt;br/&gt;In this article we quantize (massive) higher spin (1&#8804;j&#8804;2) fields by means of Dirac&#8217;s constrained Hamilton procedure both in the situation were they are totally free and were they are coupled to (an) auxiliary field(s). A full constraint analysis and quantization is presented by determining and...&lt;br/&gt;[Phys. Rev. D 80, 104027] Published Wed Nov 18, 2009</description>
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    <dc:date>2009-11-18T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104026" 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>Electromagnetic absorption cross section of Reissner-Nordstr&#246;m black holes revisited</title>
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    <description>Author(s): Lu&#237;s C. B. Crispino, Atsushi Higuchi, and Ednilton S. Oliveira&lt;br/&gt;The absorption cross section of Reissner-Nordstr&#246;m black holes for the electromagnetic field is computed numerically for arbitrary frequencies, taking into account the coupling of the electromagnetic and gravitational perturbations. We also compute the conversion coefficients of electromagnetic to ...&lt;br/&gt;[Phys. Rev. D 80, 104026] Published Tue Nov 17, 2009</description>
    <dc:creator>Lu&#237;s C. B. Crispino, Atsushi Higuchi, and Ednilton S. Oliveira</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104026</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104026</dc:source>
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    <title>Hamiltonian of a spinning test particle in curved spacetime</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104025</link>
    <description>Author(s): Enrico Barausse, Etienne Racine, and Alessandra Buonanno&lt;br/&gt;Using a Legendre transformation, we compute the unconstrained Hamiltonian of a spinning test particle in a curved spacetime at linear order in the particle spin. The equations of motion of this unconstrained Hamiltonian coincide with the Mathisson-Papapetrou-Pirani equations. We then use the formali...&lt;br/&gt;[Phys. Rev. D 80, 104025] Published Tue Nov 17, 2009</description>
    <dc:creator>Enrico Barausse, Etienne Racine, and Alessandra Buonanno</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104025</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104025</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104024" 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>Emergence of scalar matter from spin foam model</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104024</link>
    <description>Author(s): Peng Xu and Yongge Ma&lt;br/&gt;A spin foam model of three dimensional gravity nonminimally coupled with a scalar field is studied. By discretization of the scalar field, the model is worked out precisely in a purely combinational way. It is shown that the quantum physics of the scalar matter is totally encoded into the modified d...&lt;br/&gt;[Phys. Rev. D 80, 104024] Published Tue Nov 17, 2009</description>
    <dc:creator>Peng Xu and Yongge Ma</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104024</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104024</dc:source>
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    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:publicationDate>2009-11-17T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104024</prism:startingPage>
    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104023" 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>Accretion process onto super-spinning objects</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104023</link>
    <description>Author(s): Cosimo Bambi, Katherine Freese, Tomohiro Harada, Rohta Takahashi, and Naoki Yoshida&lt;br/&gt;The accretion process onto spinning objects in Kerr spacetimes is studied with numerical simulations. Our results show that accretion onto compact objects with Kerr parameter (characterizing the spin) |a|&lt;M and |a|&gt;M is very different. In the superspinning case, for |a| moderately larger than M, the accretion ...&lt;br/&gt;[Phys. Rev. D 80, 104023] Published Tue Nov 17, 2009</description>
    <dc:creator>Cosimo Bambi, Katherine Freese, Tomohiro Harada, Rohta Takahashi, and Naoki Yoshida</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104023</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104023</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:startingPage>104023</prism:startingPage>
    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104022" 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>Einstein-Maxwell system in 3+1 form and initial data for multiple charged black holes</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104022</link>
    <description>Author(s): Miguel Alcubierre, Juan Carlos Degollado, and Marcelo Salgado&lt;br/&gt;We consider the Einstein-Maxwell system as a Cauchy initial value problem taking the electric and magnetic fields as independent variables. Maxwell&#8217;s equations in curved spacetimes are derived in detail using a 3+1 formalism and their hyperbolic properties are analyzed, showing that the resulting ...&lt;br/&gt;[Phys. Rev. D 80, 104022] Published Mon Nov 16, 2009</description>
    <dc:creator>Miguel Alcubierre, Juan Carlos Degollado, and Marcelo Salgado</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.80.104022</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104022</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>2009-11-16T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104022</prism:startingPage>
    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104021" 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 small Lovelock black holes in even dimensions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104021</link>
    <description>Author(s): Tomohiro Takahashi and Jiro Soda&lt;br/&gt;We study the stability of static black holes in Lovelock theory, which is a natural higher dimensional generalization of Einstein theory. We derive a master equation for tensor perturbations in general Lovelock theory. It turns out that the resultant equation is characterized by one functional which...&lt;br/&gt;[Phys. Rev. D 80, 104021] Published Mon Nov 16, 2009</description>
    <dc:creator>Tomohiro Takahashi and Jiro Soda</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.80.104021</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104021</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
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    <prism:publicationDate>2009-11-16T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104021</prism:startingPage>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104020" 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>Towards a supersymmetric generalization of the Schwarzschild black hole</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104020</link>
    <description>Author(s): J. C. L&#243;pez-Dom&#237;nguez, O. Obreg&#243;n, and S. Zacar&#237;as&lt;br/&gt;The Wheeler-DeWitt (WDW) equation for the Kantowski-Sachs model can also be understood as the WDW equation corresponding to the Schwarzschild black hole due to the well known diffeomorphism between these two metrics. The WDW equation and its solutions are ignorant of the coordinate patch one is usin...&lt;br/&gt;[Phys. Rev. D 80, 104020] Published Mon Nov 16, 2009</description>
    <dc:creator>J. C. L&#243;pez-Dom&#237;nguez, O. Obreg&#243;n, and S. Zacar&#237;as</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.80.104020</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104020</dc:source>
    <dc:format>text/html</dc:format>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104019" 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>Shear viscosity and instability from third order Lovelock gravity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104019</link>
    <description>Author(s): Xian-Hui Ge, Sang-Jin Sin, Shao-Feng Wu, and Guo-Hong Yang&lt;br/&gt;We calculate the ratio of shear viscosity to entropy density for charged black branes in third order Lovelock theory. For chargeless black branes, the result turns out to be consistent with the prediction made by Brustein and Medved [Phys. Rev. D 79, 021901 (2009)].. We find that the third order Lov...&lt;br/&gt;[Phys. Rev. D 80, 104019] Published Mon Nov 16, 2009</description>
    <dc:creator>Xian-Hui Ge, Sang-Jin Sin, Shao-Feng Wu, and Guo-Hong Yang</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.80.104019</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104019</dc:source>
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    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:publicationDate>2009-11-16T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104019</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.80.107502" 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>More on the covariant retarded Green&#8217;s function for the electromagnetic field in de Sitter spacetime</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.107502</link>
    <description>Author(s): Atsushi Higuchi, Lee Yen Cheong, and Jack R. Nicholas&lt;br/&gt;In a recent paper it was shown in examples that the covariant retarded Green&#8217;s functions in certain gauges for electromagnetism and linearized gravity can be used to reproduce field configurations correctly in spite of the spacelike nature of past infinity in de&#160;Sitter spacetime. In this paper we...&lt;br/&gt;[Phys. Rev. D 80, 107502] Published Fri Nov 13, 2009</description>
    <dc:creator>Atsushi Higuchi, Lee Yen Cheong, and Jack R. Nicholas</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.80.107502</dc:identifier>
    <dc:source>Phys. Rev. D 80, 107502</dc:source>
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    <dc:type>article</dc:type>
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    <prism:startingPage>107502</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.80.104018" 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>Accretion of nonminimally coupled scalar fields into black holes</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104018</link>
    <description>Author(s): Manuela G. Rodrigues and Alberto Saa&lt;br/&gt;By using a quasistationary approach, we consider the mass evolution of Schwarzschild black holes in the presence of a nonminimally coupled cosmological scalar field. The mass evolution equation is analytically solved for generic coupling, revealing a qualitatively distinct behavior from the minimal ...&lt;br/&gt;[Phys. Rev. D 80, 104018] Published Fri Nov 13, 2009</description>
    <dc:creator>Manuela G. Rodrigues and Alberto Saa</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.80.104018</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104018</dc:source>
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    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:startingPage>104018</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.80.104017" 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>Curvature corrections and topology change transition in brane-black hole systems: A perturbative approach</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104017</link>
    <description>Author(s): Viktor G. Czinner and Antonino Flachi&lt;br/&gt;We consider curvature corrections to static, axisymmetric Dirac-Nambu-Goto membranes embedded into a spherically symmetric black hole spacetime with arbitrary number of dimensions. Since the next to leading order corrections in the effective brane action are quadratic in the brane thickness &#8467;, we ...&lt;br/&gt;[Phys. Rev. D 80, 104017] Published Fri Nov 13, 2009</description>
    <dc:creator>Viktor G. Czinner and Antonino Flachi</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.80.104017</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104017</dc:source>
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    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
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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.80.104016" 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>Generalized Misner-Sharp energy in f(R) gravity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104016</link>
    <description>Author(s): Rong-Gen Cai, Li-Ming Cao, Ya-Peng Hu, and Nobuyoshi Ohta&lt;br/&gt;We study generalized Misner-Sharp energy in f(R) gravity in a spherically symmetric space-time. We find that unlike the cases of Einstein gravity and Gauss-Bonnet gravity, the existence of the generalized Misner-Sharp energy depends on a constraint condition in the f(R) gravity. When the constraint ...&lt;br/&gt;[Phys. Rev. D 80, 104016] Published Fri Nov 13, 2009</description>
    <dc:creator>Rong-Gen Cai, Li-Ming Cao, Ya-Peng Hu, and Nobuyoshi Ohta</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.80.104016</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104016</dc:source>
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    <prism:startingPage>104016</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.80.107501" 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>General features of Bianchi-I cosmological models in Lovelock gravity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.107501</link>
    <description>Author(s): S. A. Pavluchenko&lt;br/&gt;We derived equations of motion corresponding to Bianchi-I cosmological models in the Lovelock gravity. Equations derived in the general case, without any specific ansatz for any number of spatial dimensions and any order of the Lovelock correction. We also analyzed the equations of motion solely tak...&lt;br/&gt;[Phys. Rev. D 80, 107501] Published Thu Nov 12, 2009</description>
    <dc:creator>S. A. Pavluchenko</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.80.107501</dc:identifier>
    <dc:source>Phys. Rev. D 80, 107501</dc:source>
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    <prism:publicationName>Physical Review D</prism:publicationName>
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    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104015" 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>Further improvements in the understanding of isotropic loop quantum cosmology</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104015</link>
    <description>Author(s): M. Mart&#237;n-Benito, G. A. Mena Marug&#225;n, and J. Olmedo&lt;br/&gt;The flat, homogeneous, and isotropic universe with a massless scalar field is a paradigmatic model in loop quantum cosmology. In spite of the prominent role that the model has played in the development of this branch of physics, there still remain some aspects of its quantization which deserve a mor...&lt;br/&gt;[Phys. Rev. D 80, 104015] Published Thu Nov 12, 2009</description>
    <dc:creator>M. Mart&#237;n-Benito, G. A. Mena Marug&#225;n, and J. Olmedo</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.80.104015</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104015</dc:source>
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    <dc:type>article</dc:type>
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    <prism:startingPage>104015</prism:startingPage>
    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104014" 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>Stochastic template placement algorithm for gravitational wave data analysis</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104014</link>
    <description>Author(s): I. W. Harry, B. Allen, and B. S. Sathyaprakash&lt;br/&gt;This paper presents an algorithm for constructing matched-filter template banks in an arbitrary parameter space. The method places templates at random, then removes those which are &#8220;too close&#8221; together. The properties and optimality of stochastic template banks generated in this manner are inves...&lt;br/&gt;[Phys. Rev. D 80, 104014] Published Thu Nov 12, 2009</description>
    <dc:creator>I. W. Harry, B. Allen, and B. S. Sathyaprakash</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.80.104014</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104014</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:startingPage>104014</prism:startingPage>
    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104013" 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>One-loop corrections to the photon propagator in curved-space QED</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104013</link>
    <description>Author(s): Bruno Gon&#231;alves, Guilherme de Berredo-Peixoto, and Ilya L. Shapiro&lt;br/&gt;We calculate and discuss the one-loop corrections to the photon sector of QED interacting to a background gravitational field. At high energies the fermion field can be taken as massless and the quantum terms can be obtained by integrating conformal anomaly. We present a covariant local expression f...&lt;br/&gt;[Phys. Rev. D 80, 104013] Published Thu Nov 12, 2009</description>
    <dc:creator>Bruno Gon&#231;alves, Guilherme de Berredo-Peixoto, and Ilya L. Shapiro</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.80.104013</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104013</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:startingPage>104013</prism:startingPage>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104012" 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>Wormhole geometries in f(R) modified theories of gravity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104012</link>
    <description>Author(s): Francisco S. N. Lobo and Miguel A. Oliveira&lt;br/&gt;In this work, we construct traversable wormhole geometries in the context of f(R) modified theories of gravity. We impose that the matter threading the wormhole satisfies the energy conditions, so that it is the effective stress-energy tensor containing higher order curvature derivatives that is res...&lt;br/&gt;[Phys. Rev. D 80, 104012] Published Wed Nov 11, 2009</description>
    <dc:creator>Francisco S. N. Lobo and Miguel A. Oliveira</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.80.104012</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104012</dc:source>
    <dc:format>text/html</dc:format>
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    <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>
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    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104011" 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>No-go theorem for bimetric gravity with positive and negative mass</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104011</link>
    <description>Author(s): Manuel Hohmann and Mattias N. R. Wohlfarth&lt;br/&gt;We argue that the most conservative geometric extension of Einstein gravity describing both positive and negative mass sources and observers is bimetric gravity and contains two copies of standard model matter which interact only gravitationally. Matter fields related to one of the metrics then appe...&lt;br/&gt;[Phys. Rev. D 80, 104011] Published Tue Nov 10, 2009</description>
    <dc:creator>Manuel Hohmann and Mattias N. R. Wohlfarth</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.80.104011</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104011</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>2009-11-10T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104011</prism:startingPage>
    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104010" 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>Higher-dimensional solitons and black holes with a nonminimally coupled scalar field</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104010</link>
    <description>Author(s): Dominic Hosler and Elizabeth Winstanley&lt;br/&gt;We study higher-dimensional soliton and hairy black hole solutions of the Einstein equations nonminimally coupled to a scalar field. The scalar field has no self-interaction potential but a cosmological constant is included. Nontrivial solutions exist only when the cosmological constant is negative ...&lt;br/&gt;[Phys. Rev. D 80, 104010] Published Mon Nov 09, 2009</description>
    <dc:creator>Dominic Hosler and Elizabeth Winstanley</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.80.104010</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104010</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>104010</prism:startingPage>
    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104009" 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>Ultrahigh precision cosmology from gravitational waves</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104009</link>
    <description>Author(s): Curt Cutler and Daniel E. Holz&lt;br/&gt;We show that the Big Bang Observer (BBO), a proposed space-based gravitational-wave (GW) detector, would provide ultraprecise measurements of cosmological parameters. By detecting &#226;&#710;&#188;3&#195;&#8212;10^{5} compact-star binaries, and utilizing them as standard sirens, BBO would determine the Hubble constant to &#226;&#710;...&lt;br/&gt;[Phys. Rev. D 80, 104009] Published Mon Nov 09, 2009</description>
    <dc:creator>Curt Cutler and Daniel E. Holz</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.80.104009</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104009</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2009-11-09T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104009</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.80.104008" 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>Thermodynamics of charged black holes with a nonlinear electrodynamics source</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104008</link>
    <description>Author(s): Hern&#225;n A. Gonz&#225;lez, Mokhtar Hassa&#239;ne, and Cristi&#225;n Mart&#237;nez&lt;br/&gt;We study the thermodynamical properties of electrically charged black hole solutions of a nonlinear electrodynamics theory defined by a power p of the Maxwell invariant, which is coupled to Einstein gravity in four and higher spacetime dimensions. Depending on the range of the parameter p, these sol...&lt;br/&gt;[Phys. Rev. D 80, 104008] Published Mon Nov 09, 2009</description>
    <dc:creator>Hern&#225;n A. Gonz&#225;lez, Mokhtar Hassa&#239;ne, and Cristi&#225;n Mart&#237;nez</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.80.104008</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104008</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>2009-11-09T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104008</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104007" 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>Interaction of the Barbero-Immirzi field with matter and pseudoscalar perturbations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104007</link>
    <description>Author(s): Simone Mercuri and Victor Taveras&lt;br/&gt;In loop quantum gravity the classical point of departure is the Einstein-Hilbert action modified by the addition of the so-called Holst term. Classically, this term does not affect the equations of motion, but it induces a well-known quantization ambiguity in the quantum theory, parametrized by the ...&lt;br/&gt;[Phys. Rev. D 80, 104007] Published Fri Nov 06, 2009</description>
    <dc:creator>Simone Mercuri and Victor Taveras</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.80.104007</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104007</dc:source>
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    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2009-11-06T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104007</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104006" 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>Large-scale structure in brane-induced gravity. I. Perturbation theory</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104006</link>
    <description>Author(s): Rom&#225;n Scoccimarro&lt;br/&gt;We study the growth of subhorizon perturbations in brane-induced gravity using perturbation theory. We solve for the linear evolution of perturbations taking advantage of the symmetry under gauge transformations along the extra-dimension to decouple the bulk equations in the quasistatic approximatio...&lt;br/&gt;[Phys. Rev. D 80, 104006] Published Fri Nov 06, 2009</description>
    <dc:creator>Rom&#225;n Scoccimarro</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.80.104006</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104006</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>2009-11-06T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104006</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.80.104005" 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>Large-scale structure in brane-induced gravity. II. Numerical simulations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104005</link>
    <description>Author(s): Kwan Chuen Chan and Rom&#225;n Scoccimarro&lt;br/&gt;We use N-body simulations to study the nonlinear structure formation in brane-induced gravity, developing a new method that requires alternate use of Fast Fourier Transforms and relaxation. This enables us to compute the nonlinear matter power spectrum and bispectrum, the halo mass function, and the...&lt;br/&gt;[Phys. Rev. D 80, 104005] Published Fri Nov 06, 2009</description>
    <dc:creator>Kwan Chuen Chan and Rom&#225;n Scoccimarro</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.80.104005</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104005</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>2009-11-06T00:00:00-05:00</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.80.104004" 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>Smooth lattice construction of the Oppenheimer-Snyder spacetime</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104004</link>
    <description>Author(s): Leo Brewin and Jules Kajtar&lt;br/&gt;We present test results for the smooth lattice method using an Oppenheimer-Snyder spacetime. The results are in excellent agreement with theory and numerical results from other authors.&lt;br/&gt;[Phys. Rev. D 80, 104004] Published Thu Nov 05, 2009</description>
    <dc:creator>Leo Brewin and Jules Kajtar</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.80.104004</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104004</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>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104004</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104003" 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>Asymptotically free scalar curvature-ghost coupling in quantum Einstein gravity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104003</link>
    <description>Author(s): Astrid Eichhorn, Holger Gies, and Michael M. Scherer&lt;br/&gt;We consider the asymptotic-safety scenario for quantum gravity which constructs a nonperturbatively renormalizable quantum gravity theory with the help of the functional renormalization group (RG). We verify the existence of a non-Gaussian fixed point and include a running curvature-ghost coupling a...&lt;br/&gt;[Phys. Rev. D 80, 104003] Published Thu Nov 05, 2009</description>
    <dc:creator>Astrid Eichhorn, Holger Gies, and Michael M. Scherer</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.80.104003</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104003</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>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104003</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
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