Results 281 to 290 of about 28,835 (313)
Estimating the hole surface area of insecticide-treated nets using image analysis, manual hole counting and exact hole measurements. [PDF]
Malar JMbuba E +14 more
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Development and validation of a machine learning-based model for 90-day prognosis outcome in spontaneous intracerebral hemorrhage patients based on non-contrast computed tomography: a multicenter retrospective observational study. [PDF]
EClinicalMedicineWei L +11 more
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Stratified wind from a super-Eddington X-ray binary is slower than expected. [PDF]
NatureXRISM collaboration.
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Interfacial charge transfer-driven UV-activated photocatalytic degradation of metronidazole <i>via</i> δ-MnO<sub>2</sub>/WO<sub>3</sub> heterojunction in aqueous media. [PDF]
RSC AdvIslam MS +6 more
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Accelerating binary black hole system
International Journal of Modern Physics A, 2022Recently, by the end of their second observing run, advanced LIGO and Virgo have detected some binary black hole mergers. In this paper, we show that the acceleration of black holes around each other causes the emergence of two Rindler space–times. The parameters of the black hole in each region change in opposite order to the parameters of the black ...
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Close black-hole binary systems
Physical Review D, 1992When the amount of gravitational radiation is small, a binary system of two orbiting black holes evolves in a quasistationary manner. This system can be approximated by a linear combination of geometries each of which has standing waves at spatial infinity; however, the combination has purely outgoing radiation.
, Blackburn, , Detweiler
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AIP Conference Proceedings, 2010
In this study, we consider binary systems with black‐hole components whose physical parameters are determined. In these systems, angular‐momentum (AM) loss via cool stellar winds is compared to AM loss by gravitational radiation.
K. Yakut +2 more
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In this study, we consider binary systems with black‐hole components whose physical parameters are determined. In these systems, angular‐momentum (AM) loss via cool stellar winds is compared to AM loss by gravitational radiation.
K. Yakut +2 more
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Physics Today, 2011
Solving the equations of general relativity presents unique challenges. Nowadays many of those have been met, and new numerical simulations are revealing surprising astrophysical phenomena.
Thomas W. Baumgarte, Stuart L. Shapiro
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Solving the equations of general relativity presents unique challenges. Nowadays many of those have been met, and new numerical simulations are revealing surprising astrophysical phenomena.
Thomas W. Baumgarte, Stuart L. Shapiro
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2001
The black hole is the most exotic object in the universe predicted as a direct consequence of general relativity. Research of stellar mass black holes dates back to 1939, when Oppenheimer and ***Snyder (1939) predicted the possible presence of black holes.
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The black hole is the most exotic object in the universe predicted as a direct consequence of general relativity. Research of stellar mass black holes dates back to 1939, when Oppenheimer and ***Snyder (1939) predicted the possible presence of black holes.
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1996
Introduction Distinguishing neutron stars and black holes Optical companions and dynamical masses X-ray signatures of the nature of a compact object Structure and evolution of black-hole binaries High-mass black-hole binaries Low-mass black-hole binaries Low-mass black holes Formation of black holes in binaries Conclusions and future prospects.
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Introduction Distinguishing neutron stars and black holes Optical companions and dynamical masses X-ray signatures of the nature of a compact object Structure and evolution of black-hole binaries High-mass black-hole binaries Low-mass black-hole binaries Low-mass black holes Formation of black holes in binaries Conclusions and future prospects.
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