[PDF] Top 20 A new dynamical model for the black hole binary LMC X 1
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A new dynamical model for the black hole binary LMC X 1
... an X-ray eclipse, which is not observed at a high level of ...best-fitting model in Table 5 a star rotating at ≈ 65% of the synchronous value in a moderately eccentric orbit where the X-ray source ... See full document
55
Binary black hole mergers in the first Advanced LIGO observing run
... One model is restricted to spins aligned with the orbital angular momentum [8,9], while the other allows for nonaligned orientation of the spins, which can lead to precession of the orbital plane ... See full document
36
A New Model for Black Hole Soft X-Ray Transients in Quiescence
... soft X-ray transients, A0620-00, V404 Cyg, and X-ray Nova Mus 1991, in ...the black hole as a nearly virial two-temperature ...the black hole and only a small fraction, 10 4 10 3 ... See full document
33
Accreting neutron stars and black holes
... irradiation model (described in Appendix B) for the most probable mass ratio of Sco X-1 (q ' ...pre-cataclysmic binary NN Ser (see Parsons et ...the binary orbit. Although they are not ... See full document
174
Tidal stripping of stars near supermassive black holes
... a binary system composed of a supermassive black hole and a star orbiting the hole in an equatorial, circular orbit, the stellar orbit will shrink due to the action of gravitational radiation, ... See full document
5
Black Hole Simulations: From Supercomputers to Your Laptop
... a new nu- merical grid that extends slightly inside the original excision ...This new grid is used for the evolution. On the new grid the apparent horizons lie inside the computational domain rather ... See full document
261
Astrophysical implications the binary black hole merger GW150914
... through dynamical friction ( on a timescale shorter than the overall relaxation time by a factor that is the ratio of the mass of the typical BH to the mass of an average background star ) ...Such dynamical ... See full document
15
The basic physics of the binary black hole merger GW150914
... form model, in the filtered detector strain ...two black holes. The black holes were each of approximately 35 M , still orbited each other as close as ∼350 km apart and subsequently merged to form a ... See full document
17
Properties of the binary black hole merger GW150914
... Our analysis is based on waveform models that do not include the effect of spins in their full generality. Still, the aligned-spin EOBNR and precessing IMRPhenom models produce consistent results, with an error budget ... See full document
19
Properties of the Binary Black Hole Merger GW150914
... Our analysis is based on waveform models that do not include the effect of spins in their full generality. Still, the aligned-spin EOBNR and precessing IMRPhenom models produce consistent results, with an error budget ... See full document
19
Variable O VI and N V emission from the X ray binary LMC X 3 : heating of the black hole companion
... revisit LMC X-3 with a new ephemeris and new UV ob- ...of LMC X-3 based on high-resolution optical spectroscopy recently obtained with the ...report new ultraviolet ... See full document
11
Numerical Relativity beyond General Relativity
... non-linear, dynamical, strong-field regime of gravity is one of the major goals of gravitational wave ...for binary black hole (BBH) systems in theories beyond ...in dynamical ... See full document
249
Observation of gravitational waves from a binary black hole merger
... a black hole [5,6], and in 1963 Kerr generalized the solution to rotating black holes ...of black hole quasinormal modes [8 – 10], and in the 1990s higher-order post- Newtonian ... See full document
16
Observation of Gravitational Waves from a Binary Black Hole Merger
... a black hole [5,6], and in 1963 Kerr generalized the solution to rotating black holes ...of black hole quasinormal modes [8 – 10], and in the 1990s higher-order post- Newtonian ... See full document
16
Black Hole as the Global Standard Model
... In previous sections, we have shown that the concept of velocity is replaced with the relative distance between any any two different points in the space time when we match local gravitational measurements with the local ... See full document
10
Accurate Gravitational Waveforms from Binary Black hole Systems
... of black-hole binary systems, and intro- duce a practical technique for obtaining the asymptotic form of that data from finite simulation domains in Chapter ... See full document
424
A Magnetic Model for Low/Hard States Associated with Jets in Black Hole X Ray Binaries
... MHD model for interpreting the episodic ejections from BHXBs, and GRO J1655-40, XTE J1550- 564 and GRS 1915 + 105 are ...Figure 1 of ...corona model in ... See full document
11
Spectrally accurate initial data in numerical relativity
... where we will assume the potentially nonlinear term, f (ψ), takes on a form corre- sponding to an initial puncture equation for two black holes. As in the single puncture case, the solution for ψ is known to be ... See full document
163
BHnFDIA : Energy Efficient Elimination of Black Hole and False Data Injection Attacks in Wireless Sensor Networks
... overcome black hole attack in wireless sensor networks using a new acknowledgement-based detection ...the black hole detecting node will send records to its neighbours in the new ... See full document
8
Binary Black Holes Algorithm
... In many optimization problems the searching should be performed in the binary space. Hence it is desirable for these optimization algorithms presenting Binary version. In the binary space, the ... See full document
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