Results 21 to 30 of about 1,893 (155)

New Formalism for Numerical Relativity [PDF]

open access: yesPhysical Review Letters, 1995
uucompresed PS file. 4 pages including 1 figure. Revised version adds a figure showing a comparison between the standard ADM approach and the new formulation. Also available at http://jean-luc.ncsa.uiuc.edu/Papers/ Appeared in Physical Review Letters 75, 600 (1995)
Bona, Carles   +3 more
openaire   +3 more sources

VISTAS IN NUMERICAL RELATIVITY [PDF]

open access: yesBlack Hole Astrophysics 2002, 2002
Upcoming gravitational wave-experiments promise a window for discovering new physics in astronomy. Detection sensitivity of the broadband laser interferometric detectors LIGO/VIRGO may be enhanced by matched filtering with accurate wave-form templates. Where analytic methods break down, we have to resort to numerical relativity, often in Hamiltonian or
openaire   +2 more sources

Numerical relativity and compact binaries [PDF]

open access: yesPhysics Reports, 2003
122 pages, 19 figures; review article to appear in Physics ...
Baumgarte, Thomas W., Shapiro, Stuart L.
openaire   +3 more sources

Lattice Boltzmann model for numerical relativity [PDF]

open access: yesPhysical Review E, 2016
In the Bona-Masso formulation, Einstein equations are written as a set of flux conservative first order hyperbolic equations that resemble fluid dynamics equations. Based on this formulation, we construct a lattice Boltzmann model for Numerical Relativity.
Ilseven, E., Mendoza, M.
openaire   +3 more sources

A Radiation Scalar for Numerical Relativity [PDF]

open access: yesPhysical Review Letters, 2002
This letter describes a scalar curvature invariant for general relativity with a certain, distinctive feature. While many such invariants exist, this one vanishes in regions of space-time which can be said unambiguously to contain no gravitational radiation.
Beetle, Christopher, Burko, Lior M.
openaire   +4 more sources

The 3+1 formalism in teleparallel and symmetric teleparallel gravity

open access: yesEuropean Physical Journal C: Particles and Fields, 2021
Teleparallel and symmetric teleparallel gravity offer platforms in which gravity can be formulated in interesting geometric approaches, respectively given by torsion and nonmetricity. In this vein, general relativity can be expressed in three dynamically
Salvatore Capozziello   +3 more
doaj   +1 more source

Towards standard testbeds for numerical relativity [PDF]

open access: yesClassical and Quantum Gravity, 2003
In recent years, many different numerical evolution schemes for Einstein's equations have been proposed to address stability and accuracy problems that have plagued the numerical relativity community for decades. Some of these approaches have been tested on different spacetimes, and conclusions have been drawn based on these tests. However, differences
Alcubierre, Miguel   +20 more
openaire   +4 more sources

A Brief Overview of Black Hole-Neutron Star Mergers

open access: yesFrontiers in Astronomy and Space Sciences, 2020
Of the three main types of binaries detectable through ground-based gravitational wave observations, black hole-neutron star (BHNS) mergers remain the most elusive.
Francois Foucart
doaj   +1 more source

Fundamental Tone and Overtones of Quasinormal Modes in Ringdown Gravitational Waves: A Detailed Study in Black Hole Perturbation

open access: yesUniverse, 2021
Ringdown gravitational waves of compact object binaries observed by ground-based gravitational-wave detectors encapsulate rich information to understand remnant objects after the merger and to test general relativity in the strong field. In this work, we
Norichika Sago   +2 more
doaj   +1 more source

Relative numerical ranges

open access: yesLinear Algebra and its Applications, 2015
Let \(H\) be a separable complex Hilbert space and let \(B(H)\) be the Banach algebra of all bounded linear operators on \(H\). The numerical range of \(S\in B(H)\) is the set \(W(S)=\left\{(Sx,x):\; ||x||\; =1\right\}\). It is known that the spectrum \(\sigma (S)\) of \(S\) is contained in \(W(S)\). In this paper, the authors define a more general set,
Bracic, J., Diogo, C.
openaire   +2 more sources

Home - About - Disclaimer - Privacy