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Relativistic Correction To Black Hole Entropy

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This paper finds an exact singular black hole solution in the presence of nonlinear electrodynamics as the source of matter field surrounded by a cloud of strings in spacetime. a GUP On the other hand, we have approximate approaches, such as the interpretation of black hole entropy as entanglement entropy [11,12] or, relatedly, the associ-ation of black

Bekenstein-Hawking entropy versus entanglement entropy of black hole ...

In 1969, Roger Penrose proposed a mechanism to extract rotational energy from a Kerr black hole. With this, he inspired two lines of investigation in the years after. On the one

We compute logarithmic correction to the entropy of BPS black holes in asymptotically flat five dimensional space-time using finite temperature black hole geometry Since black hole entropy encodes the number of microstates, this loss leads to a reduction in the information-storing static spherically capacity of the system. However, if evaporation of PBHs is unitary, as In this paper, we study the relativistic correction to Bekenstein-Hawking entropy in the canonical ensemble and isothermal-isobaric ensemble and apply it to the cases of non-rotating BTZ and

Bekenstein bound on black hole entropy in non-Gaussian statistics

The Bekenstein bound, inspired by the physics of black holes, is introduced to constrain the entropy growth of a physical system down to the quantum level in the context of a Finally, in section “ Generalized Thermodynamics of Quantum Black Holes ”, we consider generalized thermodynamics of quantum black holes and, in particular, generalized black hole

In recent decades, the intersection between black hole thermodynamics and quantum physics has provided significant insights into the nature of gravity. The relationship 1 WenotehoweverthattheCardy(hightemperature)limitisnotalways reliable for extracting the black hole entropy [24]. On the other hand, in two dimensional CFTs the logarithmic corrections are Abstract The remarkable connection between black holes and thermodynamics provides the most significant clues that we currently possess to the nature of black holes in a quantum theory of

  • Black Hole Entropy: Certain Quantum Features
  • Introductory Lectures on Black Hole Thermodynamics
  • Black hole information paradox
  • Smart Holes: Analogue black holes with the right temperature and entropy

Article „Relativistic Correction to Black Hole Entropy“ Detailed information of the J-GLOBAL is an information service managed by the Japan Science and Technology Agency (hereinafter Many extracting the black hole recent attempts to calculate black hole entropy from first principles rely on conformal field theory techniques. By examining the logarithmic corrections to the Cardy formula, I compute

Abstract The black hole information paradox has persisted as one of theoretical physics‘ most fundamental challenges, arising from the apparent incompatibility between Abstract Starting from an effective action for quantum gravity, we calculate the quantum gravitational corrections to the Wald entropy of a four dimensional non-extremal Abstract Kaniadakis ( $$\\kappa $$ κ -deformed) statistics is being widely used for describing relativistic systems with non-extensive behavior and/or interactions. It is built upon a

Relativistic accretion and burdened primordial black holes

Quantizing the system via bosonization of relativistic fermions, we obtain a microscopic description of black hole states in terms of Young diagrams, whose degeneracies

The remarkable connection between black holes and thermodynamics provides the most significant clues that we currently possess Abstract Starting from an e ective action for quantum gravity, we calculate the quantum grav-itational corrections to the Wald entropy of a four dimensional non-extremal Reissner In this study, we investigate the thermodynamic properties and phase transitions in rotating anti-de Sitter (AdS) black holes by applying the Kaniadakis (KD) entropy framework.

PPT - Gravity as Entropic Force PowerPoint Presentation, free download ...

We analyze the properties of the black hole, such as temperature and entropy, under the influence of quantum gravity and also observe that the first-order correction is

In the presence of a GUP, black hole thermodynamics undergoes significant modifications: the black hole temperature and entropy receive quantum corrections, potentially Next, we calculate the HBAR entropy in this thought experiment and show that this entropy has a leading order Bekenstein-Hawking entropy term along with some higher order correction terms

Entropy An important black hole observable is the Bekenstein-Hawking (BH) entropy, which is proportional to the area of the event horizon, SBH = Ah / (4 G). For the 3-brane solution (3.1),

e or relativistic properties [1–4]. This framework has been applied in vari-ous fields, including cosmology, black hole thermody amics, and quantum mechanics [5–8]. Entanglement entropy, by applying the Kaniadakis KD TH 1 , 8 M (1) where M is the black hole mass [5]. While, in classical thermodynamics, entropy is universal and defined uniquely, quantum effects correct the Bekenstein-Hawking entropy

Space Calc – CalculatorsBlack Hole Parameters Introduction This calculator will calculate the properties of a black hole described by given parameters (mass, charge, angular momentum), These notes aim to provide an introduction to the basics of black hole thermodynamics. After explaining Bekenstein’s original proposal that black holes have entropy,

We study the thermodinamic features of static, spherically-symmetric Schwarzschild black holes adopting different types of Barrow entropy. Specifically, in addition ture of Thermal Relativity, Gravity and Black Hole Thermody-namics, unifying inertial and accelerated observers. We will derive the exact Thermal Relativistic corrections to the

In this paper, employing the path integral method in the framework of a canonical description of a Schwarzschild black hole, we obtain the corrected inverse temperature and His pioneering work laid the foundation for what is now known as Kaniadakis entropy or ? κ -entropy. This concept emerged as a relativistic generalization of the classical Further, we examine the improved entropy to study the influences of quantum gravity and black hole geometry on entropy. We explore the graphical behavior of entropy

Majumdar, Parthasarathi. “Black Hole Entropy: Certain Quantum Features.” On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic