Thermal stability with emission energy and Joule–Thomson expansion of regular BTZ-like black hole - INSPIRE

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Thermal stability with emission energy and Joule–Thomson expansion of regular BTZ-like black hole

Allah Ditta
(
- Shanghai U.
)
,
Xia Tiecheng
(
- Shanghai U.
)
,
G. Mustafa
(
- Zhejiang Normal U.
)
,
Muhammad Yasir
(
- Shanghai U.
)
,
Farruh Atamurotov
(
- Tashkent, CTPA and
- Silesian U., Czech Republic and
- Uzbekistan Natl. U. and
- Unlisted, UZ
)

Aug 29, 2022

12 pages

Published in:

Eur.Phys.J.C 82 (2022) 8, 756

Published: Aug 29, 2022

DOI:

10.1140/epjc/s10052-022-10708-z

reference search37 citations

Citations per year

Abstract: (Springer)

We investigate the thermodynamic properties and Joule–Thomson expansion for conical or BTZ-like black holes. To analyze the thermal stability, we discuss the temperature and thermal stability relative to the horizon radius for different values of model parameters

\beta _0

and

\alpha _2

. Moreover, we analyze thermodynamical geometries like Ruppeiner, Weinhold and Hendi Panahiyah Eslam Momennia formulation and calculate respective scalar curvatures for BTZ-like black holes. Interestingly, the black holes have no singularity in some cases, i.e., completely regular. We obtain the inversion temperatures and inversion curves and investigate the similarities and differences between van der Waals and charged fluids. To discuss this expansion, we use a BTZ-like black hole. Further, we establish the position of the inversion point versus different values of mass

\mu

, and the parameters

\beta _0

and

\alpha _2

for such a BTZ-like black hole. The Joule–Thomson coefficient

\mu

at this point disappears. A crucial trait upon which we relied to inspect the sign of quantity

\mu

to get the cooling-heating areas. We also investigate the energy emission depending upon the frequency

\omega

.

stability: thermal
energy: emission
curvature: scalar
geometry: thermodynamical
black hole: BTZ
temperature
fluid
horizon
singularity
van der Waals

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Figures(0)

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