Zobrazeno 1 - 10
of 166
pro vyhledávání: '"Aref'eva, Irina"'
In the thermodynamics of black holes in asymptotically flat space, the third law of thermodynamics is violated, and entropy cannot be consistently modeled through conventional statistical mechanics. Notably, the third law of thermodynamics is violate
Externí odkaz:
http://arxiv.org/abs/2411.01778
In recent literature on holographic QCD, the consideration of the five-dimensional Einstein-dilaton-Maxwell models has played a crucial role. Typically, one Maxwell field is associated with the chemical potential, while additional Maxwell fields are
Externí odkaz:
http://arxiv.org/abs/2409.12131
We study the dependence of beta-function on running coupling constant in holographic models supported by Einstein-dilaton-Maxwell action for light and heavy quarks. Although, in the previous paper [arXiv:2402.14512], we considered different types of
Externí odkaz:
http://arxiv.org/abs/2407.14448
Publikováno v:
Phys.Rev.D 110 (2024) 8, 086021
We consider running coupling constant in holographic model with external magnetic field supported by Einstein-dilaton-three-Maxwell action. We obtain a significant dependence of the running coupling constant $\alpha$ on chemical potential, temperatur
Externí odkaz:
http://arxiv.org/abs/2407.11924
We consider running coupling constant and beta-function in holographic models supported by Einstein-dilaton-Maxwell action for heavy and light quarks. To obtain the dependence of the running coupling constant $\alpha$ on temperature and chemical pote
Externí odkaz:
http://arxiv.org/abs/2402.14512
Publikováno v:
Eur. Phys. J. C 83, no.12, 1143 (2023)
In our previous paper [arXiv:2011.07023] we have constructed a twice anisotropic five-dimensional holographic model supported by Einstein-dilaton-three-Maxwell action that reproduced some essential features of the "heavy quarks" model. However, that
Externí odkaz:
http://arxiv.org/abs/2305.06345
Autor:
Aref'eva, Irina, Volovich, Igor
Black holes violate the third law of thermodynamics in its standard formulation. Schwarzschild black hole entropy is inverse proportional to the square of the temperature $S=1/(16 \pi T^2) $ and tends to infinity rather than zero when the temperature
Externí odkaz:
http://arxiv.org/abs/2304.04695
Autor:
Ageev, Dmitry S., Aref'eva, Irina Ya.
In this paper, we study entanglement islands and the Page curve in the eternal four-dimensional Schwarzschild black hole surrounded by finite temperature conformal matter. By finite temperature conformal matter we mean the matter described by the the
Externí odkaz:
http://arxiv.org/abs/2206.04094
Publikováno v:
Eur.Phys.J.C 83 (2023) 1, 79
We present a five-dimensional twice anisotropic holographic model supported by Einstein-dilaton-three-Maxwell action describing light quarks. The first of the Maxwell fields provides finite chemical potential. The second Maxwell field serves for anis
Externí odkaz:
http://arxiv.org/abs/2203.12539
Autor:
Aref'eva, Irina, Volovich, Igor
The problem of complete evaporation of Schwarzschild black holes raised by Hawking is that one has an explosion of the temperature $T=1/8\pi M$ for vanishing black hole mass M. We consider the Reissner-Nordstrom black hole and note that if mass $M$ a
Externí odkaz:
http://arxiv.org/abs/2202.00548