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2022

Periapsis shifts in dark matter distribution around a black hole

Igata, Takahisa, Harada, Tomohiro, Saida, Hiromi et al.

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We consider the periapsis shifts of bound orbits of stars on static clouds around a black hole.

The background spacetime is constructed from a Schwarzschild black hole surrounded by a static and spherically symmetric self-gravitating system of massive particles, which satisfies all the standard energy conditions and physically models the gravitational effect of dark matter distribution around a nonrotating black hole.
Using nearly circular bound orbits of stars, we obtain a simple formula for the precession rate.
This formula explicitly shows that the precession rate is determined by a positive contribution (i.e., a prograde shift) from the conventional general-relativistic effect and a negative contribution (i.e., a retrograde shift) from the local matter density.

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N. Bar, K. Blum, T. Lacroix, and P. Panci, Looking for ultralight dark matter near supermassive black holes, JCAP 07
Original
1905
Earlier work this paper cites.
T. Do et al
Original
1907
Earlier work this paper cites.
H. Saida et al
Original
1910
Earlier work this paper cites.
A. Einstein, On a stationary system with spherical symmetry consisting of many gravitating masses, Ann. Math. 40
1939
Earlier work this paper cites.
C. W. Misner and D. H. Sharp, Relativistic equations for adiabatic, spherically symmetric gravitational collapse, Phys. Rev. 136
1964
Earlier work this paper cites.
S. Weinberg, Gravitation and Cosmology
1972
Earlier work this paper cites.
J. M. Bardeen, Timelike and null geodesics in the Kerr metric, in Black Holes (Les Astres Occlus)
1973
Earlier work this paper cites.
R. M. Wald, General Relavity
1984
Earlier work this paper cites.
L. Hernquist, An analytical model for spherical galaxies and bulges, Astrophys. J. 356
1990
Earlier work this paper cites.
G. L. Comer and J. Katz, Thick Einstein shells and their mechanical stability, Classical Quantum Gravity 10
1993
Earlier work this paper cites.
S. A. Hayward, Gravitational energy in spherical symmetry, Phys. Rev. D 53
1996
Earlier work this paper cites.
J. F. Navarro, C. S. Frenk, and S. D. M. White, The structure of cold dark matter halos, Astrophys. J. 462
1996
Earlier work this paper cites.
P. Gondolo and J. Silk, Dark matter annihilation at the galactic center, Phys. Rev. Lett. 83
1999
Earlier work this paper cites.

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Original
2004
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D. Bini, F. De Paolis, A. Geralico, G. Ingrosso, and A. Nucita, Periastron shift in Weyl class spacetimes, Gen. Rel. Grav. 37
2005
Cited alongside, same era.
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Then

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Original
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Later among the works it cites.
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Original
2018
Later among the works it cites.
P. Bambhaniya, D. Dey, A. B. Joshi, P. S. Joshi, D. N. Solanki, and A. Mehta, Shadows and negative precession in non-Kerr spacetime, Phys. Rev. D 103
Original
2021
Later among the works it cites.
R. A. Konoplya, Black holes in galactic centers: Quasinormal ringing, grey-body factors and Unruh temperature, Phys. Lett. B 823
Original
2021
Later among the works it cites.
Z. Stuchlík and J. Vrba, Supermassive black holes surrounded by dark matter modeled as anisotropic fluid: epicyclic oscillations and their fitting to observed QPOs, JCAP 11

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