首页|Thermodynamics of Barrow Einstein-power-Yang-Mills AdS black hole in the
restricted phase space
Thermodynamics of Barrow Einstein-power-Yang-Mills AdS black hole in the
restricted phase space
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Arxiv
As we know that due to the quantum gravitational effects black hole horizons
are ``fractalized'' into a sphereflake by Barrow. Based on this issue, in this
work we investigate the phase structure and stability of the
Einstein-Power-Yang-Mills AdS black holes with the fractal structure on the
black hole horizon in the restricted phase space. Through the thermodynamics
first law and the Smarr relation in the restricted phase space, we observe that
the mass parameter is understood as the inter energy and the Smarr relation is
not a homogeneous function of order one for all quantities due to the fractal
structure. And the fractal structure can be regarded as a phase transition
probe. When this system with the fixed central charge there exists a novel
phenomena: the supercritical phase transition. Furthermore the effects of the
fractal parameter and non-linear Yang-Mills parameter on the thermodynamics
stability of this system are also investigated.
Arxiv
