Results 91 to 100 of about 94,165 (223)
Numerical Study on the Hydrodynamic Instability of Binary Stars in the First Post Newtonian Approximation of General Relativity [PDF]
M. Shibata, K. Oohara, Takashi Nakamura
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Numerical Relativity in 3+1 Dimensions
AbstractNumerical relativity is finally approaching a state where the evolution of rather general (3+1)‐dimensional data sets can be computed in order to solve the Einstein equations. After a general introduction, three topics of current interest are briefly reviewed: binary black hole mergers, the evolution of strong gravitational waves, and shift ...
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RisingTides: An Analytic Modeling Code of Tidal Effects in Binary Neutron Star Mergers
Gravitational waves produced by binary neutron star mergers offer a unique window into matter behavior under extreme conditions. In this context, we analytically model the effect of matter on gravitational waves from binary neutron star mergers. We start
Alexander O’Dell +1 more
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Improving the NRTidal model for binary neutron star systems
Accurate and fast gravitational waveform (GW) models are essential to extract information about the properties of compact binary systems that generate GWs.
Dietrich, Tim +5 more
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Towards a gauge-polyvalent numerical relativity code [PDF]
Daniela Alic, C. Bona, Carles Bona-Casas
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Suitability of post-Newtonian/numerical-relativity hybrid waveforms for gravitational wave detectors [PDF]
Ilana MacDonald +2 more
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Schwarzschild tests of the Wahlquist-Estabrook-Buchman-Bardeen tetrad formulation for numerical relativity [PDF]
Luisa T. Buchman, J. Bardeen
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Interplay between numerical relativity and perturbation theory : finite size effects [PDF]
Tousif Islam, Gaurav Khanna
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The idea of stable, localized bundles of energy has strong appeal as a model for particles. In the 1950s, John Wheeler envisioned such bundles as smooth configurations of electromagnetic energy that he called geons, but none were found. Instead, particle-
Steven L. Liebling, Carlos Palenzuela
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