Results 31 to 40 of about 28,835 (313)

Silence of Binary Kerr Black Holes [PDF]

open access: yesPhysical Review Letters, 2020
A nontrivial S matrix generally implies a production of entanglement: starting with an incoming pure state, the scattering generally returns an outgoing state with nonvanishing entanglement entropy. It is then interesting to ask if there exists a nontrivial S matrix that generates no entanglement.
Rafael Aoude   +4 more
openaire   +2 more sources

Close supermassive binary black holes [PDF]

open access: yesNature, 2010
Nature in press. 4 pages, 1 figure [Title, abstract, text, and references shortened to conform to journal requirements]
openaire   +3 more sources

BLACK HOLE–NEUTRON STAR COALESCING BINARIES

open access: yesInternational Journal of Modern Physics D, 2010
Coalescing black hole–neutron star binaries have been invoked as possible progenitors of short gamma-ray bursts and are also among the most promising gravitational wave sources to be detected by ground-based laser interferometers. When the star is disrupted by tidal interactions before reaching the innermost stable circular orbit, the gravitational ...
FERRARI, Valeria   +2 more
openaire   +4 more sources

Binary black hole spectroscopy [PDF]

open access: yesClassical and Quantum Gravity, 2007
We study parameter estimation with post-Newtonian (PN) gravitational waveforms for the quasi-circular, adiabatic inspiral of spinning binary compact objects. The performance of amplitude-corrected waveforms is compared with that of the more commonly used restricted waveforms, in Advanced LIGO and EGO.
Broeck, Chris Van Den   +1 more
openaire   +2 more sources

Asymmetric Light Curves of Black Hole Binaries and the Doppler Beaming Effect [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2002
Black hole binary candidates are known to be composed of a black hole with 10Msolar and a K or M type companion. Because the companion is believed to fill the Roche lobe that is very aspherical, the light curves of black hole binaries are characterized ...
Hee-Won Lee   +2 more
doaj   +1 more source

Approximate binary-black-hole metric [PDF]

open access: yesPhysical Review D, 2000
20 pages, 1 figure; some changes in Sec.
openaire   +2 more sources

Physics-inspired deep learning to characterize the signal manifold of quasi-circular, spinning, non-precessing binary black hole mergers

open access: yesPhysics Letters B, 2020
The spin distribution of binary black hole mergers contains key information concerning the formation channels of these objects, and the astrophysical environments where they form, evolve and coalesce.
Asad Khan, E.A. Huerta, Arnav Das
doaj   +1 more source

OJ 287 binary black hole system

open access: yesMemorie della Societa Astronomica Italiana, 2011
To appear in "Multifrequency Behaviour of High Energy Cosmic Sources", F. Giovannelli & L. Sabau-Graziati (eds.), Mem. SAIt., Vol. 81 N. 1 (2012)
Mauri Valtonen, Stefano Ciprini
openaire   +3 more sources

Enhanced black hole mergers in binary–binary interactions [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2018
We study the orbital evolution of black hole (BH) binaries in quadruple systems, where the tertiary binary excites large eccentricity in the BH binary through Lidov-Kozai (LK) oscillations, causing the binary BHs to merge via gravitational radiation. For typical BH binaries with masses $m_{1,2}\simeq 20M_\odot-30M_\odot$ and initial semimajor axis $a_0\
Liu, Bin, Lai, Dong
openaire   +2 more sources

Spectrally Tunable 2D Material‐Based Infrared Photodetectors for Intelligent Optoelectronics

open access: yesAdvanced Functional Materials, EarlyView.
Intelligent optoelectronics through spectral engineering of 2D material‐based infrared photodetectors. Abstract The evolution of intelligent optoelectronic systems is driven by artificial intelligence (AI). However, their practical realization hinges on the ability to dynamically capture and process optical signals across a broad infrared (IR) spectrum.
Junheon Ha   +18 more
wiley   +1 more source

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