https://doi.org/10.1140/epjp/s13360-024-05235-7
Regular Article
Extended phase space thermodynamics of Bardeen–Letelier black holes in 4D Einstein–Gauss–Bonnet gravity
1
Institute for Theoretical Physics and Cosmology, Zhejiang University of Technology, 310023, Hangzhou, China
2
Department of Mathematical Sciences, University of Zululand, Private Bag X1001, 3886, Kwa-Dlangezwa, South Africa
3
Centre for Theoretical Physics, Jamia Millia Islamia, 110025, New Delhi, India
4
Astrophysics and Cosmology Research Unit, School of Mathematics, Statistics and Computer Science, University of KwaZulu-Natal, Private Bag X54001, 4000, Durban, South Africa
5
Department of Mathematical Sciences, University of Zululand, Private Bag X1001, 3886, Kwa-Dlangezwa, South Africa
6
Faculty of Natural Sciences, Mangosuthu University of Technology, P.O. Box 12363, 4026, Jacobs, South Africa
Received:
8
February
2024
Accepted:
30
April
2024
Published online:
24
May
2024
We use the black hole chemistry prescription, , to investigate the thermodynamic behavior of Bardeen-AdS black holes surrounded by clouds of strings in 4D EGB gravity. The Hawking temperature shows local maxima and minima at critical horizon radii
and
, when we take
, signifying the existence of phase transition. Further, when we take the value of pressure less than critical pressure, the isobars on
–
plane exhibit a swallowtail-like structure confirming the first-order phase transition between small and large stable black holes, but because of clouds of strings, it occurs at a lower temperature and lower critical pressure. In the limit
, surrounded by a cloud of strings (
) and with nonlinear electrodynamics (NED) switched off (
), the Hawking–Page phase transition exists, but it would be disappeared, and SBH/LBH phase transition recovers as soon one switch on the NED (
). The effects of clouds of strings on P–V criticality suggest that the isotherms undergo liquid–gas-like phase transition for
at lower
and that the critical exponents identical with van der Walls fluid.
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© The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.