The signature of tidal disruption phenomena in the vicinity of a black hole

Details The signature of tidal disruption phenomena in the vicinity of a black hole The signature of tidal disruption phenomena in the vicinity of a black hole

2012-04-20

arxiv.org/abs/1204.4561v1

Proceedings of the MG12 Meeting on General Relativity, World Scientific, 2012, vol. 2, p. 928

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

3 pages, 8 figures

Scientific paper

Tidal effects on clumps of material during random non-stationary accretion onto a black hole produce phenomena with distinct temporal characteristics in observed light-curves. During such non-stationary accretion events, the shape of the accreting object evolves in time, and observable quasi-periodic phenomena with variable quasi-periods are produced. A number of characteristic light-curves, obtained with numerical simulations, will be shown. Their relevance to observed phenomena will be briefly discussed.

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