Results 41 to 50 of about 170,936 (294)
Can We Prescribe the Physical Parameters of Multiple Black Holes?
Mathematics, 2021 The parabolic-hyperbolic form of the constraints and superposed Kerr-Schild black holes have already been used to provide a radically new initialization of binary black hole configurations.
István Rácz
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Tracing Black Hole Signatures in Several Black Hole Candidates Based on Their X-Ray Spectral Evolution [PDF]
EPJ Web of Conferences, 2020 Investigation of spectral evolution of four black hole candidates was carried out by using color-color diagram as well as spectral fitting on Swift/XRT data.
Alfarizki Fahmi Iman, Vierdayanti Kiki
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Hydrodynamical simulations of the tidal stripping of binary stars by massive black holes [PDF]
, 2016 In a galactic nucleus, a star on a low angular momentum orbit around the central massive black hole can be fully or partially disrupted by the black hole tidal field, lighting up the compact object via gas accretion.
Campana, Sergio +3 more
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LAST ORBITS OF BINARY BLACK HOLES [PDF]
International Journal of Modern Physics A, 2002 Binary black hole systems in the pre-coalescence stage are numerically constructed by demanding that the associated spacetime admits a helical Killing vector. Comparison with third order post-Newtonian calculations indicates a rather good agreement until the innermost stable circular orbit.
Gourgoulhon, Eric +2 more
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Dynamical Descalarization in Binary Black Hole Mergers [PDF]
Physical Review Letters, 2021 Scalar fields coupled to the Gauss-Bonnet invariant can undergo a tachyonic instability, leading to spontaneous scalarization of black holes. Studies of this effect have so far been restricted to single black hole spacetimes. We present the first results on dynamical scalarization in head-on collisions and quasicircular inspirals of black hole binaries
Hector O. Silva +3 more
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Hypervelocity binary stars: smoking gun of massive binary black holes
, 2007 The hypervelocity stars recently found in the Galactic halo are expelled from the Galactic center through interactions between binary stars and the central massive black hole or between single stars and a hypothetical massive binary black hole.
D. N. C. Lin +4 more
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When can gravitational-wave observations distinguish between black holes and neutron stars? [PDF]
, 2013 Gravitational-wave observations of compact binaries have the potential to uncover the distribution of masses and angular momenta of black holes and neutron stars in the universe.
Brown, Duncan A. +4 more
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, 2015 We analyze the distinguishability of populations of coalescing binary neutron stars, neutron-star black-hole binaries, and binary black holes, whose gravitational-wave signatures are expected to be observed by the advanced network of ground-based ...
Belczynski, Krzysztof +3 more
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Star Clusters with Primordial Binaries: III. Dynamical Interaction between Binaries and an Intermediate Mass Black Hole [PDF]
, 2006 We present the first study of the dynamical evolution of an isolated star cluster that combines a significant population of primordial binaries with the presence of a central black hole.
Ardi, E. +3 more
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Approximate binary-black-hole metric [PDF]
Physical Review D, 2000 20 pages, 1 figure; some changes in Sec.
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