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Spherical Accretion of Matter by Charged Black Holes on f(T) Gravity

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arxiv 1606.04918 v1 pith:BODIDXI5 submitted 2016-06-13 gr-qc astro-ph.GAhep-th

Manuel E. Rodrigues , Ednaldo L. B. Junior This is my paper · ORCID
classification gr-qcastro-ph.GAhep-th
keywords accretionfluidblackholessphericalchargedgravitymatter
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abstract

We studied the spherical accretion of matter by charged black holes on $f(T)$ Gravity. Considering the accretion model of a isentropic perfect fluid we obtain the general form of the Hamiltonian and the dynamic system for the fluid. We have analysed the movements of an isothermal fluid model with $p=\omega e$ and where $p$ is the pressure and $e$ the total energy density. The analysis of the cases shows the possibility of spherical accretion of fluid by black holes, revealing new phenomena as cyclical movement inside the event horizon.

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  1. Periodical orbits and waveforms with spontaneous Lorentz symmetry-breaking in Kalb-Ramond gravity

    gr-qc 2024-12 conditional novelty 4.0 of 10

    For a Kalb-Ramond black hole, the Lorentz-violating parameter l shifts the radii and energies of the marginal and innermost stable orbits and changes the phase of gravitational waves from extreme-mass-ratio inspirals.

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