Pith. sign in

REVIEW

Astrophysical flows near f(T) gravity black holes

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1602.03523 v2 pith:WCYIIXD5 submitted 2016-02-10 gr-qc astro-ph.GA

Astrophysical flows near f(T) gravity black holes

Ayyesha K. Ahmed , Mustapha Azreg-A\"inou (C. Author) , Sebastian Bahamonde , Salvatore Capozziello , Mubasher Jamil This is my paper
classification gr-qc astro-ph.GA
keywords blackgravityholeaccretionflowsfluidsnearprocess
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

In this paper, we study the accretion process for fluids flowing near a black hole in the context of $f(T)$ teleparallel gravity. Specifically, by performing a dynamical analysis by a Hamiltonian system, we are able to find the sonic points. After that, we consider different isothermal test fluids in order to study the accretion process when they are falling onto the black hole. We found that these flows can be classified according to the equation of state and the black hole features. Results are compared in $f(T)$ and $f(R)$ gravity.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.