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Find link is a tool written by Edward Betts.searching for Spin parameter 13 found (14 total)
alternate case: spin parameter
Black hole
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J\leq {\frac {GM^{2}}{c}},} allowing definition of a dimensionless spin parameter such that 0 ≤ c J G M 2 ≤ 1. {\displaystyle 0\leq {\frac {cJ}{GM^{2}}}\leqNaked singularity (2,900 words) [view diff] exact match in snippet view article find links to article
threshold to produce a naked singularity (spin parameter 1). GRS 1915+105 comes closest to the limit, with a spin parameter of 0.82-1.00. It is hinted that GROGRS 1915+105 (804 words) [view diff] exact match in snippet view article find links to article
The black hole rotates at least 950 times per second, giving it a spin parameter >0.82 (1.0 is the theoretical maximum). In 1994, GRS 1915+105 becameRotating black hole (1,305 words) [view diff] exact match in snippet view article find links to article
key element in the 2014 film Interstellar. Black hole bomb Black hole spin parameter Black hole spin-flip BKL singularity – solution representing interiorList of gravitational wave observations (6,717 words) [view diff] exact match in snippet view article find links to article
differ by an order of magnitude. The dimensionless effective inspiral spin parameter is: m 1 a 1 c o s θ L S 1 + m 2 a 2 c o s θ L S 2 m 1 + m 2 , {\displaystyleSupermassive black hole (11,103 words) [view diff] exact match in snippet view article find links to article
prograde spin with a dimensionless spin parameter of a = 1, although the maximum limit for a black hole's spin parameter is very slightly lower at a = 0Dark matter halo (2,827 words) [view diff] exact match in snippet view article find links to article
significant angular momentum. Numerical simulations have shown that the spin parameter distribution for halos formed by dissipation-less hierarchical clusteringLense–Thirring precession (2,856 words) [view diff] exact match in snippet view article find links to article
the orbit, M is the mass of the black hole, χ is the dimensionless spin parameter (0 < χ < 1). The precessing stars also exert a torque back on the blackSagittarius A* (7,851 words) [view diff] exact match in snippet view article find links to article
interacting with Sagittarius A*. Several values have been given for its spin parameter a ∗ = c J G M 2 {\displaystyle a_{*}={\frac {cJ}{GM^{2}}}} ; some examplesKerr metric (6,963 words) [view diff] exact match in snippet view article find links to article
shadow (black) and the important surfaces (white) of a black hole. The spin parameter a {\displaystyle a} is animated from 0 {\displaystyle 0} toFirst observation of gravitational waves (7,592 words) [view diff] exact match in snippet view article find links to article
post-merger object is found to be a rotating Kerr black hole with a spin parameter of 0.68+0.05 −0.06, i.e. one with 2/3 of the maximum possible angularCarter constant (2,666 words) [view diff] exact match in snippet view article find links to article
}|}}} is the rest mass of the particle, and a {\displaystyle a} is the spin parameter of the black hole which satisfies 0 ≤ a ≤ M {\displaystyle 0\leq a\leqKerr–Newman–de–Sitter metric (3,080 words) [view diff] exact match in snippet view article find links to article
g_{\mu \nu }=0} , where a {\displaystyle {\rm {a}}} is the black hole's spin parameter, ℧ {\displaystyle {\rm {\mho }}} its electric charge, and Λ = 3 H 2