output
19932026
most citedMeasurements of Omega and Lambda from 42 High-Redshift Supernovae

18.1k citations

Showing 2013 · gr-qcShow all

47 papers · 2 filters

gr-qc2013★ 8 cited

Braneworlds with field derivative coupling to the Einstein tensor

Masato Minamitsuji

In this paper, we investigate the Randall-Sundrum type braneworld models in the scalar-tensor theory with field derivative coupling to the Einstein tensor. We first formulate the g…

gr-qc2013★ 140 cited

Solutions in the scalar-tensor theory with nonminimal derivative coupling

Masato Minamitsuji

We present black hole type solutions in the scalar-tensor theory with nonminimal derivative coupling to the Einstein tensor. The effects of the nonminimal derivative coupling appea…

gr-qc2013★ 10 cited

Covariant and gauge-invariant linear scalar perturbations in multiple scalar field cosmologies

Artur Alho, Filipe C. Mena

We derive a set of equations monitoring the evolution of covariant and gauge-invariant linear scalar perturbations of Friedman-Lemaître-Robertson-Walker models with multiple intera…

gr-qc2013★ 127 cited

I-Q relation for rapidly rotating neutron stars

Sayan Chakrabarti, Térence Delsate, Norman Gürlebeck +1

We consider a universal relation between moment of inertia and quadrupole moment of arbitrarily fast rotating neutron stars. Recent studies suggest that this relation breaks down f…

gr-qc2013★ 43 cited

Collisions of oppositely charged black holes

Miguel Zilhão, Vitor Cardoso, Carlos Herdeiro +2

The first fully non-linear numerical simulations of colliding charged black holes in D=4 Einstein-Maxwell theory were recently reported arXiv:1205.1063. These collisions were perfo…

gr-qc2013★ 33 cited

Collapse of self-interacting fields in asymptotically flat spacetimes: do self-interactions render Minkowski spacetime unstable?

Hirotada Okawa, Vitor Cardoso, Paolo Pani

The nonlinear instability of anti-de Sitter spacetime has recently been established with the striking result that generic initial data collapses to form black holes. This outcome s…

gr-qc2013★ 184 cited

Coalescence of binary neutron stars in a scalar-tensor theory of gravity

Masaru Shibata, Keisuke Taniguchi, Hirotada Okawa +1

We carry out numerical-relativity simulations of coalescing binary neutron stars in a scalar-tensor theory that admits spontaneous scalarization. We model neutron stars with realis…

gr-qc2013★ 6 cited

The energy spectrum of gravitational waves in a loop quantum cosmological model

Joao Morais, Mariam Bouhmadi-Lopez, Alfredo B. Henriques

We explore the consequences of loop quantum cosmology (inverse-volume corrections) in the spectrum of the gravitational waves using the method of the Bogoliubov coefficients. These…

gr-qc2013★ 3 cited

The spherically symmetric Einstein-scalar field system with positive and vanishing cosmological constant: a comparison

João L. Costa

We review recent results concerning the spherically symmetric Einstein-scalar field system with positive cosmological constant. We do so by comparing with the classical results of…

gr-qc2013★ 72 cited

Polytropic spheres with electric charge: compact stars, the Oppenheimer-Volkoff and Buchdahl limits, and quasiblack holes

José D. V. Arbañil, José P. S. Lemos, Vilson T. Zanchin

We explore a class of compact charged spheres made of a charged perfect fluid with a polytropic equation of state. The charge density is chosen to be proportional to the energy den…

gr-qc2013★ 1 cited

Parametric instability in scalar gravitational fields

T. B. Davies, C. H. -T. Wang, R. Bingham +1

We present a brief review on a new dynamical mechanism for a strong field effect in scalar tensor theory. Starting with a summary of the essential features of the theory and subseq…

gr-qc2013★ 13 cited

Thermodynamics, entropy, and stability of thin shells in 2+1 flat spacetimes

José P. S. Lemos, Gonçalo M. Quinta

The thermodynamic equilibrium states of a static thin ring shell in a (2+1)-dimensional flat spacetime is analyzed. Inside the ring the spacetime is flat, whereas outside it is con…

gr-qc2013★ 99 cited

Black holes with massive graviton hair

Richard Brito, Vitor Cardoso, Paolo Pani

No-hair theorems exclude the existence of nontrivial scalar and massive vector hair outside four-dimensional, static, asymptotically flat black-hole spacetimes. We show, by explici…

gr-qc2013★ 5 cited

A consistent scalar-tensor cosmology for inflation, dark energy and the Hubble parameter

C. H. -T. Wang, J. A. Reid, A. St J. Murphy +5

A Friedman cosmology is investigated based on scalar-tensor gravitation with general metric coupling and scalar potential functions. We show that for a broad class of such function…

gr-qc2013

Theory of intersecting loops on a torus

J. E. Nelson, R. F. Picken

We continue our investigation into intersections of closed paths on a torus, to further our understanding of the commutator algebra of Wilson loop observables in 2+1 quantum gravit…

gr-qc2013★ 51 cited

Black hole bombs and explosions: from astrophysics to particle physics

Vitor Cardoso

Black holes are the elementary particles of gravity, the final state of sufficiently massive stars and of energetic collisions. With a forty-year long history, black hole physics i…

gr-qc2013★ 11 cited

Initial Conditions for Numerical Relativity -- Introduction to numerical methods for solving elliptic PDEs

Hirotada Okawa

Numerical relativity became a powerful tool to investigate the dynamics of binary problems with black holes or neutron stars as well as the very structure of General Relativity. Al…

gr-qc2013★ 140 cited

Black holes with surrounding matter in scalar-tensor theories

Vitor Cardoso, Isabella P. Carucci, Paolo Pani +1

We uncover two mechanisms that can render Kerr black holes unstable in scalar-tensor gravity, both associated to the presence of matter in the vicinity of the black hole and the fa…

gr-qc2013★ 57 cited

The role of nonmetricity in metric-affine theories of gravity

Vincenzo Vitagliano

The intriguing choice to treat alternative theories of gravity by means of the Palatini approach, namely elevating the affine connection to the role of independent variable, contai…

gr-qc2013★ 93 cited

Scalar, Electromagnetic and Gravitational Perturbations of Kerr-Newman Black Holes in the Slow-Rotation Limit

Paolo Pani, Emanuele Berti, Leonardo Gualtieri

In Einstein-Maxwell theory, according to classic uniqueness theorems, the most general stationary black-hole solution is the axisymmetric Kerr-Newman metric, which is defined by th…

gr-qc2013★ 142 cited

Error-analysis and comparison to analytical models of numerical waveforms produced by the NRAR Collaboration

Ian Hinder, Alessandra Buonanno, Michael Boyle +53

The Numerical-Relativity-Analytical-Relativity (NRAR) collaboration is a joint effort between members of the numerical relativity, analytical relativity and gravitational-wave data…

gr-qc2013★ 159 cited

Astrophysical signatures of boson stars: quasinormal modes and inspiral resonances

Caio F. B. Macedo, Paolo Pani, Vitor Cardoso +1

Compact bosonic field configurations, or boson stars, are promising dark matter candidates which have been invoked as an alternative description for the supermassive compact object…

gr-qc2013★ 61 cited

Solar System constraints to nonminimally coupled gravity

Orfeu Bertolami, Riccardo March, Jorge Páramos

We extend the analysis of Chiba, Smith and Erickcek \cite{CSE} of Solar System constraints on gravity to a class of nonminimally coupled (NMC) theories of gravity. These gen…

gr-qc2013★ 46 cited

Effective action and linear response of compact objects in Newtonian gravity

Sayan Chakrabarti, Térence Delsate, Jan Steinhoff

We apply an effective field theory method for the gravitational interaction of compact stars, developed within the context of general relativity, to Newtonian gravity. In this effe…