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    <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>
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    <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>
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    <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>
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    <title>Equivalence principle implications of modified gravity models</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104002</link>
    <description>Author(s): Lam Hui, Alberto Nicolis, and Christopher W. Stubbs&lt;br/&gt;Theories that attempt to explain the observed cosmic acceleration by modifying general relativity all introduce a new scalar degree of freedom that is active on large scales, but is screened on small scales to match experiments. We demonstrate that if such screening occurs via the chameleon mechanis...&lt;br/&gt;[Phys. Rev. D 80, 104002] Published Thu Nov 05, 2009</description>
    <dc:creator>Lam Hui, Alberto Nicolis, and Christopher W. Stubbs</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>
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    <title>Turning big bang into big bounce. I. Classical dynamics</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104001</link>
    <description>Author(s): Piotr Dzier&#380;ak, Przemys&#322;aw Ma&#322;kiewicz, and W&#322;odzimierz Piechocki&lt;br/&gt;The big bounce (BB) transition within a flat Friedmann-Robertson-Walker model is analyzed in the setting of loop geometry underlying the loop cosmology. We solve the constraint of the theory at the classical level to identify physical phase space and find the Lie algebra of the Dirac observables. We...&lt;br/&gt;[Phys. Rev. D 80, 104001] Published Wed Nov 04, 2009</description>
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    <title>Cuscuton and low-energy limit of Ho&#345;ava-Lifshitz gravity</title>
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    <description>Author(s): Niayesh Afshordi&lt;br/&gt;Ho&#345;ava-Lifshitz theory has been recently put forth as a proposal for a renormalizable theory of quantum gravity . It explicitly breaks Lorentz invariance, introducing an apparent extra scalar degree of freedom. I show that the low energy limit of (non-projectible) Ho&#345;ava-Lifshitz gravity is unique...&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, 081502] Published Fri Oct 30, 2009</description>
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    <dc:date>2009-10-30T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
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    <title>Flavor condensates in brane models and dark energy</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084046</link>
    <description>Author(s): Nick E. Mavromatos, Sarben Sarkar, and Walter Tarantino&lt;br/&gt;In the context of a microscopic model of string-inspired foam, in which foamy structures are provided by brany pointlike defects (D-particles) in space-time, we discuss flavor mixing as a result of flavor nonpreserving interactions of (low-energy) fermionic stringy matter excitations with the defect...&lt;br/&gt;[Phys. Rev. D 80, 084046] Published Thu Oct 29, 2009</description>
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    <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.80.084046</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084046</dc:source>
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    <title>Matter in loop quantum gravity without time gauge: A nonminimally coupled scalar field</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084045</link>
    <description>Author(s): Francesco Cianfrani and Giovanni Montani&lt;br/&gt;We analyze the phase space of gravity nonminimally coupled to a scalar field in a generic local Lorentz frame. We reduce the set of constraints to a first class one by fixing a specific hypersurfaces in the phase space. The main issue of our analysis is to extend the features of the vacuum case to t...&lt;br/&gt;[Phys. Rev. D 80, 084045] Published Thu Oct 29, 2009</description>
    <dc:creator>Francesco Cianfrani and Giovanni Montani</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.80.084045</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084045</dc:source>
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    <title>Dispersion of growth of matter perturbations in f(R) gravity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084044</link>
    <description>Author(s): Shinji Tsujikawa, Radouane Gannouji, Bruno Moraes, and David Polarski&lt;br/&gt;We study the growth of matter density perturbations &#948;_{m} for a number of viable f(R) gravity models that satisfy both cosmological and local gravity constraints, where the Lagrangian density f is a function of the Ricci scalar R. If the parameter m&#8801;Rf_{,RR} /f_{,R} today is larger than the order...&lt;br/&gt;[Phys. Rev. D 80, 084044] Published Thu Oct 29, 2009</description>
    <dc:creator>Shinji Tsujikawa, Radouane Gannouji, Bruno Moraes, and David Polarski</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.80.084044</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084044</dc:source>
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    <title>Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084043</link>
    <description>Author(s): Alessandra Buonanno, Bala R. Iyer, Evan Ochsner, Yi Pan, and B. S. Sathyaprakash&lt;br/&gt;The two-body dynamics in general relativity has been solved perturbatively using the post-Newtonian (PN) approximation. The evolution of the orbital phase and the emitted gravitational radiation are now known to a rather high order up to O(v^{8} ), v being the characteristic velocity of the binary. ...&lt;br/&gt;[Phys. Rev. D 80, 084043] Published Thu Oct 29, 2009</description>
    <dc:creator>Alessandra Buonanno, Bala R. Iyer, Evan Ochsner, Yi Pan, and B. S. Sathyaprakash</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.80.084043</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084043</dc:source>
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    <title>Probing the puncture for black hole simulations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084042</link>
    <description>Author(s): J. David Brown&lt;br/&gt;With the puncture method for black hole simulations, the second infinity of a wormhole geometry is compactified to a single &#8220;puncture point&#8221; on the computational grid. The region surrounding the puncture quickly evolves to a trumpet geometry. The computational grid covers only a portion of the t...&lt;br/&gt;[Phys. Rev. D 80, 084042] Published Thu Oct 29, 2009</description>
    <dc:creator>J. David Brown</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.80.084042</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084042</dc:source>
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    <title>Comment on two recent papers regarding next-to-leading order spin-spin effects in gravitational interaction</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.088501</link>
    <description>Author(s): Jan Steinhoff and Gerhard Sch&#228;fer&lt;br/&gt;It is argued that the tetrad in a recent paper by Porto and Rothstein on gravitational spin-spin coupling should not have the given form. The fixation of that tetrad was suggested by Steinhoff, Hergt, and Sch&#228;fer as a possible source for the disagreement found in the spin-squared dynamics. However,...&lt;br/&gt;[Phys. Rev. D 80, 088501] Published Wed Oct 28, 2009</description>
    <dc:creator>Jan Steinhoff and Gerhard Sch&#228;fer</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/PhysRevD.80.088501</dc:identifier>
    <dc:source>Phys. Rev. D 80, 088501</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084041" 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 flat, algebraically special spacetimes in higher dimensions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084041</link>
    <description>Author(s): M. Ortaggio, V. Pravda, and A. Pravdov&#225;&lt;br/&gt;We analyze asymptotic properties of higher-dimensional vacuum spacetimes admitting a &#8220;nondegenerate&#8221; geodetic multiple Weyl aligned null direction. After imposing a fall-off condition necessary for asymptotic flatness, we determine the behavior of the Weyl tensor as null infinity is approached a...&lt;br/&gt;[Phys. Rev. D 80, 084041] Published Wed Oct 28, 2009</description>
    <dc:creator>M. Ortaggio, V. Pravda, and A. Pravdov&#225;</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/PhysRevD.80.084041</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084041</dc:source>
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    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
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    <prism:publicationDate>2009-10-28T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084041</prism:startingPage>
    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084040" 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>Immirzi parameter from an external scalar field</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084040</link>
    <description>Author(s): Francesco Cianfrani and Giovanni Montani&lt;br/&gt;We promote the Immirzi parameter to be a minimally coupled scalar field and we analyzed the Hamiltonian constraints in the framework of loop quantum gravity without the time gauge. Proper SU(2) connections can be defined and a term containing derivatives of the field &#946; enters into their definition....&lt;br/&gt;[Phys. Rev. D 80, 084040] Published Wed Oct 28, 2009</description>
    <dc:creator>Francesco Cianfrani and Giovanni Montani</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/PhysRevD.80.084040</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084040</dc:source>
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    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:startingPage>084040</prism:startingPage>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084039" 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>Kaluza-Klein theory in the limit of large number of extra dimensions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084039</link>
    <description>Author(s): Fabrizio Canfora, Alex Giacomini, and Alfonso R. Zerwekh&lt;br/&gt;The Kaluza-Klein compactification in the limit of a large number of extra dimensions is studied. The starting point is the Einstein-Hilbert action plus cosmological constant in 4+D dimensions. It is shown that in the large D limit the effective four-dimensional cosmological constant is of order 1/D,...&lt;br/&gt;[Phys. Rev. D 80, 084039] Published Wed Oct 28, 2009</description>
    <dc:creator>Fabrizio Canfora, Alex Giacomini, and Alfonso R. Zerwekh</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/PhysRevD.80.084039</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084039</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.80.084038" 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>Physical evolution in loop quantum cosmology: The example of the vacuum Bianchi I model</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084038</link>
    <description>Author(s): Mercedes Mart&#237;n-Benito, Guillermo A. Mena Marug&#225;n, and Tomasz Pawlowski&lt;br/&gt;We use the vacuum Bianchi I model as an example to investigate the concept of physical evolution in loop quantum cosmology (LQC) in the absence of the massless scalar field which has been used so far in the literature as an internal time. In order to retrieve the system dynamics when no such a suita...&lt;br/&gt;[Phys. Rev. D 80, 084038] Published Tue Oct 27, 2009</description>
    <dc:creator>Mercedes Mart&#237;n-Benito, Guillermo A. Mena Marug&#225;n, and Tomasz Pawlowski</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/PhysRevD.80.084038</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084038</dc:source>
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    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:publicationDate>2009-10-27T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084038</prism:startingPage>
    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084037" 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>Backreaction of frame dragging</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084037</link>
    <description>Author(s): Carlos A. R. Herdeiro, Carmen Rebelo, and Claude M. Warnick&lt;br/&gt;The backreaction on black holes due to dragging heavy, rather than test, objects is discussed. As a case study, a five-dimensional regular black Saturn system where the central black hole has vanishing intrinsic angular momentum, J^{BH} =0, is considered. It is shown that there is a correlation betw...&lt;br/&gt;[Phys. Rev. D 80, 084037] Published Mon Oct 26, 2009</description>
    <dc:creator>Carlos A. R. Herdeiro, Carmen Rebelo, and Claude M. Warnick</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/PhysRevD.80.084037</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084037</dc:source>
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    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
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    <prism:publicationDate>2009-10-26T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084037</prism:startingPage>
    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084036" 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>Possibility of catastrophic black hole growth in the warped brane-world scenario at the LHC</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084036</link>
    <description>Author(s): Roberto Casadio, Sergio Fabi, and Benjamin Harms&lt;br/&gt;In this paper, we present the results of our analysis of the growth and decay of black holes possibly produced at the Large Hadron Collider, based on our previous study of black holes in the context of the warped brane-world scenario. The black hole mass accretion and decay is obtained as a function...&lt;br/&gt;[Phys. Rev. D 80, 084036] Published Mon Oct 26, 2009</description>
    <dc:creator>Roberto Casadio, Sergio Fabi, and Benjamin Harms</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/PhysRevD.80.084036</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084036</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>2009-10-26T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084036</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.80.084035" 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>Relativistic tidal properties of neutron stars</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084035</link>
    <description>Author(s): Thibault Damour and Alessandro Nagar&lt;br/&gt;We study the various linear responses of neutron stars to external relativistic tidal fields. We focus on three different tidal responses, associated to three different tidal coefficients: (i)&#160;a gravito-electric-type coefficient G&#956;_{&#8467;} =[length]^{2&#8467;+1} measuring the &#8467;th-order mass multipolar...&lt;br/&gt;[Phys. Rev. D 80, 084035] Published Fri Oct 23, 2009</description>
    <dc:creator>Thibault Damour and Alessandro Nagar</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/PhysRevD.80.084035</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084035</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>2009-10-23T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084035</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084034" 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>Hawking fluxes, fermionic currents, W_{1+&#8734;}  algebra, and anomalies</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084034</link>
    <description>Author(s): L. Bonora, M. Cvitan, S. Pallua, and I. Smoli&#263;&lt;br/&gt;We complete the analysis carried out in previous papers by studying the Hawking radiation for a Kerr black hole carried to infinity by fermionic currents of any spin. We find agreement with the thermal spectrum of the Hawking radiation for fermionic degrees of freedom. We start by showing that the n...&lt;br/&gt;[Phys. Rev. D 80, 084034] Published Fri Oct 23, 2009</description>
    <dc:creator>L. Bonora, M. Cvitan, S. Pallua, and I. Smoli&#263;</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/PhysRevD.80.084034</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084034</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>2009-10-23T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084034</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.80.084033" 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>de Sitter spacetimes with torsion in the model of de Sitter gauge theory of gravity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084033</link>
    <description>Author(s): Chao-Guang Huang and Meng-Sen Ma&lt;br/&gt;In the model of the de&#160;Sitter gauge theory of gravity, the empty homogenous and isotropic spacetimes with constant curvature scalar and nonvanishing homogenous and isotropic torsion must have de&#160;Sitter metrics. The static de&#160;Sitter spacetime with static, O(3)-symmetric, vector torsion is the only...&lt;br/&gt;[Phys. Rev. D 80, 084033] Published Fri Oct 23, 2009</description>
    <dc:creator>Chao-Guang Huang and Meng-Sen Ma</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/PhysRevD.80.084033</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084033</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>2009-10-23T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084033</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084032" 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>Various Hamiltonian formulations of f(R) gravity and their canonical relationships</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084032</link>
    <description>Author(s): Nathalie Deruelle, Yuuiti Sendouda, and Ahmed Youssef&lt;br/&gt;Various Hamiltonian formulations of f(R) gravity can be found in the literature. Some authors follow the Ostrogradsky treatment of higher derivative theories and introduce as extra variables first order time derivatives of the metric (typically the extrinsic curvature). Some others take advantage of...&lt;br/&gt;[Phys. Rev. D 80, 084032] Published Thu Oct 22, 2009</description>
    <dc:creator>Nathalie Deruelle, Yuuiti Sendouda, and Ahmed Youssef</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/PhysRevD.80.084032</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084032</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>2009-10-22T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084032</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084031" 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>Rotating holographic superconductor</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084031</link>
    <description>Author(s): Julian Sonner&lt;br/&gt;In this paper we initiate the study of spontaneous symmetry breaking in 3+1 dimensional rotating, charged, asymptotically AdS black holes. The theory living on their boundary, R&#215;S^{2} , has the interpretation of a 2+1 dimensional rotating holographic superconductor. We study the appearance of a mar...&lt;br/&gt;[Phys. Rev. D 80, 084031] Published Thu Oct 22, 2009</description>
    <dc:creator>Julian Sonner</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/PhysRevD.80.084031</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084031</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>2009-10-22T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084031</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084030" 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>Deriving the ADM 3+1 evolution equations from the second variation of arclength</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084030</link>
    <description>Author(s): Leo Brewin&lt;br/&gt;We will show that the ADM 3+1 evolution equations, for a zero shift vector, arise naturally from the equations for the second variation of arclength.&lt;br/&gt;[Phys. Rev. D 80, 084030] Published Thu Oct 22, 2009</description>
    <dc:creator>Leo Brewin</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/PhysRevD.80.084030</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084030</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>2009-10-22T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084030</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084029" 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>Extended Palatini action for general relativity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084029</link>
    <description>Author(s): Eran Rosenthal&lt;br/&gt;In the Palatini action of general relativity, the connection and the metric are treated as independent dynamical variables. Instead of assuming a relation between these quantities, the desired relation between them is derived through the Euler-Lagrange equations of the Palatini action. In this manus...&lt;br/&gt;[Phys. Rev. D 80, 084029] Published Thu Oct 22, 2009</description>
    <dc:creator>Eran Rosenthal</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/PhysRevD.80.084029</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084029</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>2009-10-22T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084029</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084028" 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>Maximal slicing of D-dimensional spherically symmetric vacuum spacetime</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084028</link>
    <description>Author(s): Ken-ichi Nakao, Hiroyuki Abe, Hirotaka Yoshino, and Masaru Shibata&lt;br/&gt;We study the foliation of a D-dimensional spherically symmetric black-hole spacetime with D&#8805;5 by two kinds of one-parameter families of maximal hypersurfaces: a reflection-symmetric foliation with respect to the wormhole slot and a stationary foliation that has an infinitely long trumpetlike shape...&lt;br/&gt;[Phys. Rev. D 80, 084028] Published Wed Oct 21, 2009</description>
    <dc:creator>Ken-ichi Nakao, Hiroyuki Abe, Hirotaka Yoshino, and Masaru Shibata</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/PhysRevD.80.084028</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084028</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>2009-10-21T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084028</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084027" 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>Quasilocal energy in loop quantum gravity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084027</link>
    <description>Author(s): Jinsong Yang and Yongge Ma&lt;br/&gt;Although there is no known meaningful notion of the energy density of the gravitational field in general relativity, a few notions of quasilocal energy of gravity associated to extended but finite domains have been proposed. In this paper, the notions of quasilocal energy are studied in the framewor...&lt;br/&gt;[Phys. Rev. D 80, 084027] Published Wed Oct 21, 2009</description>
    <dc:creator>Jinsong Yang and Yongge Ma</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/PhysRevD.80.084027</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084027</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>2009-10-21T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084027</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084026" 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>Smeared hair and black holes in three-dimensional de&#160;Sitter spacetime</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084026</link>
    <description>Author(s): Mu-In Park&lt;br/&gt;It is known that there is no three-dimensional analog of de&#160;Sitter black holes. I show that the analog does exist when non-Gaussian (i.e., ring-type) smearings of point matter hairs are considered. This provides a new way of constructing black hole solutions from hairs. I find that the obtained bla...&lt;br/&gt;[Phys. Rev. D 80, 084026] Published Wed Oct 21, 2009</description>
    <dc:creator>Mu-In Park</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/PhysRevD.80.084026</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084026</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>2009-10-21T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084026</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084025" 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 numerical relativity: Formulation and code tests</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084025</link>
    <description>Author(s): Hirotaka Yoshino and Masaru Shibata&lt;br/&gt;We derive a formalism of numerical relativity for higher-dimensional spacetimes and develop numerical codes for simulating a wide variety of five-dimensional (5D) spacetimes for the first time. First, the Baumgarte-Shapiro-Shibata-Nakamura formalism is extended for arbitrary spacetime dimensions D&#226;&#8240;...&lt;br/&gt;[Phys. Rev. D 80, 084025] Published Mon Oct 19, 2009</description>
    <dc:creator>Hirotaka Yoshino and Masaru Shibata</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/PhysRevD.80.084025</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084025</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>2009-10-19T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084025</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.084024" 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 initial data on hyperboloidal slices</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.084024</link>
    <description>Author(s): Luisa T. Buchman, Harald P. Pfeiffer, and James M. Bardeen&lt;br/&gt;We generalize Bowen-York black hole initial data to hyperboloidal constant mean curvature slices which extend to future null infinity. We solve this initial value problem numerically for several cases, including unequal mass binary black holes with spins and boosts. The singularity at null infinity ...&lt;br/&gt;[Phys. Rev. D 80, 084024] Published Mon Oct 19, 2009</description>
    <dc:creator>Luisa T. Buchman, Harald P. Pfeiffer, and James M. Bardeen</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/PhysRevD.80.084024</dc:identifier>
    <dc:source>Phys. Rev. D 80, 084024</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>2009-10-19T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084024</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.087501" 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>Tidal interaction of a small black hole in the field of a large Kerr black hole</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.087501</link>
    <description>Author(s): Simon Comeau and Eric Poisson&lt;br/&gt;The rates at which the mass and angular momentum of a small black hole change as a result of a tidal interaction with a much larger black hole are calculated to leading order in the small mass ratio. The small black hole is either rotating or nonrotating, and it moves on a circular orbit in the equa...&lt;br/&gt;[Phys. Rev. D 80, 087501] Published Thu Oct 15, 2009</description>
    <dc:creator>Simon Comeau and Eric Poisson</dc:creator>
    <dc:date>2009-10-15T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.087501</dc:identifier>
    <dc:source>Phys. Rev. D 80, 087501</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>2009-10-15T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>087501</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
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