Geodesic motion in the spacetime of a SU(2)-Colored (A)dS black hole in conformal gravity

Hoseini, Bahareh; Saffari, Reza; Soroushfar, Saheb

doi:10.1140/epjp/s13360-021-01511-y

Cited by 2 publications

(1 citation statement)

References 20 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…In [97] the authors examined the validity of the four black hole thermodynamic laws in massive gravity. For more details about massive gravity, its thermodynamics etc., we refer the reader to [98][99][100][101][102][103][104][106][107][108][109][110][111].…”

Section: Introductionmentioning

confidence: 99%

Thermodynamic geometry of static and rotating regular black holes in conformal massive gravity

Soroushfar,

Saffari,

Abebe

et al. 2021

Preprint

Self Cite

View full text Add to dashboard Cite

A version of massive gravity, namely conformal massive gravity, is employed to study the behavior of thermodynamic geometry for both static and rotating regular black holes. Whereas in thermodynamic geometry singularity can be interpreted as the second phase transition, seeing such phenomena as heat capacity behavior for both cases is investigated in detail. In addition, other thermodynamic quantities like the entropy and the temperature are analyzed in detail. Another important property of the black holes is the so-called stability, in which utilizing the first phase transition of the heat capacity is analyzed in detail, for both cases, say the static and the spinning black holes. It is also interestingly figured out that, the behavior of temperature of the uncharged black holes in the presence of hair parameter, λ, can mimic the charged ones. To investigate the properties of the black holes both regular thermodynamics and thermodynamic geometry approaches are considered. Then one can observe that, aiming to realize the physics of the black holes, many complicated phenomena can be analyzed dramatically easier by considering the latter approach.

show abstract