Details
| Original language | English |
|---|---|
| Article number | 084046 |
| Journal | Physical Review D |
| Volume | 106 |
| Issue number | 8 |
| Publication status | Published - 26 Oct 2022 |
| Externally published | Yes |
Abstract
The main goal of this paper is to investigate one of the important astrophysical systems, namely Thick accretion disks, in the background of the spherically symmetric solution in Born-Infeld teleparallel gravity to examine observable predictions of the theory in the vicinity of black holes. Thus, the properties of the non-self-gravitating equilibrium surfaces characterizing the Thick accretion disks model are studied. In addition, we find an observational bound on the parameter of the model as λ≳140. We show this analytical accretion disk model for different values of λ and compare the result with the corresponding Schwarzschild solution in the general theory of relativity.
ASJC Scopus subject areas
- Physics and Astronomy(all)
- Nuclear and High Energy Physics
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In: Physical Review D, Vol. 106, No. 8, 084046, 26.10.2022.
Research output: Contribution to journal › Article › Research › peer review
}
TY - JOUR
T1 - Thick accretion disk configurations in the Born-Infeld teleparallel gravity
AU - Bahamonde, Sebastian
AU - Faraji, Shokoufe
AU - Hackmann, Eva
AU - Pfeifer, Christian
N1 - Publisher Copyright: © 2022 American Physical Society.
PY - 2022/10/26
Y1 - 2022/10/26
N2 - The main goal of this paper is to investigate one of the important astrophysical systems, namely Thick accretion disks, in the background of the spherically symmetric solution in Born-Infeld teleparallel gravity to examine observable predictions of the theory in the vicinity of black holes. Thus, the properties of the non-self-gravitating equilibrium surfaces characterizing the Thick accretion disks model are studied. In addition, we find an observational bound on the parameter of the model as λ≳140. We show this analytical accretion disk model for different values of λ and compare the result with the corresponding Schwarzschild solution in the general theory of relativity.
AB - The main goal of this paper is to investigate one of the important astrophysical systems, namely Thick accretion disks, in the background of the spherically symmetric solution in Born-Infeld teleparallel gravity to examine observable predictions of the theory in the vicinity of black holes. Thus, the properties of the non-self-gravitating equilibrium surfaces characterizing the Thick accretion disks model are studied. In addition, we find an observational bound on the parameter of the model as λ≳140. We show this analytical accretion disk model for different values of λ and compare the result with the corresponding Schwarzschild solution in the general theory of relativity.
UR - http://www.scopus.com/inward/record.url?scp=85141578424&partnerID=8YFLogxK
U2 - 10.1103/physrevd.106.084046
DO - 10.1103/physrevd.106.084046
M3 - Article
VL - 106
JO - Physical Review D
JF - Physical Review D
SN - 2470-0029
IS - 8
M1 - 084046
ER -