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Thin accretion disk signatures in hybrid metric-Palatini gravity by Dyadina, P. I.; Avdeev, N. A. is a scholarly article available to read on EtoBox.

What is Thin accretion disk signatures in hybrid metric-Palatini gravity about?

In the present work, accretion onto a static spherically symmetric black hole in the hybrid metric-Palatini gravity is considered. The Novikov-Thorne model for a relativistic thin accretion disk is used. The energy flux, temperature distribution, emission spectrum and energy conversion efficiency of accretion disks around such black holes are numerically calculated. A comparison with the results for a Schwarzschild black hole is made and conclusions about the viability of the model are drawn. As a result, it is obtained that the accretion disks around black holes in hybrid metric-Palatini gravity are colder and less luminous than in general relativity.

Author

Dyadina, P. I.; Avdeev, N. A.

Published

2023

Language

EN