Papers
Topics
Authors
Recent
Search
2000 character limit reached

Barrow black hole variable parameter model connected to information theory

Published 24 Feb 2024 in gr-qc and hep-th | (2402.15922v1)

Abstract: One of the greatest challenges of theoretical physics today is to unveil the quantum information theory concerning what happens when one bit of information enters the black hole (BH) horizon. The Landauer principle showed that a certain amount of energy is generated when one-bit of information is erased as it enters the event horizon system. In this paper we used the recently developed Barrow BH model to calculate the addition to the area of the event horizon of his toy model by using the Landauer concept. Besides we make this computation considering $\Delta$ as a constant and a variable parameter. We formulate the Barrow parameter ($\Delta$) as a function of the energy/mass, which is new in the Barrow BH literature. We will investigate the differences between the Bekenstein-Hawking entropy ($\Delta=0$) and the fractal ($\Delta=1$) cases concerning the addition in the area of the BH. The asymptotical analysis is also mentioned and we will see that it affects only the fractal case. All the results accomplished here are new concerning BHs in general and the Barrow model literature in particular.

Authors (1)
Definition Search Book Streamline Icon: https://streamlinehq.com
References (10)
  1. F. A. Bais and J. D. Farmer, “The physics of information,” arXiv: 0708.2837.
  2. R. Landauer, IBM J. Res. Dev. 5 (1961) 183; “Information is Physical,” Phys. Today 44 (1991) 23.
  3. L. Brilloin, J. Appl. Phys. 24 (1953) 1152; “Scientific uncertainty and iformation,” Academic Press, New York USA, 1964; “Science and information theory,” Academic Press, New York NY, USA, 1962; L. B. Kish, C. G. Granvist, “Energy requirement of control: comments on Szilards’s engine and Maxwell’s demon, arXiv: 1110.0197; L. B. Kish, Proc. IEEE 151 (2004) 190.
  4. R. Landauer, Phys. Lett. A 217 (1961) 1888.
  5. S. Lloyd Phys. Rev. A 56 (1997) 3374;
  6. J. D. Barrow, S. Basilakos and E. N. Saridakis, “Big Bang Nucleosynthesis constraints on Barrow entropy,” arXiv: 2010.00986 [gr-qc]; E. N. Saridakis, JCAP 07 (2020) 031, arXiv: 2006.01105; F. K. Anagnostopoulos, S. Basilakos and E. N. Saridakis, Eur. Phys. J. C 80 (2020) 826; E. N. Saridakis and S. Basilakos, “The generalized second law of thermodynamics with Barrow entropy,” arXiv: 2005.08258; E. N. Saridakis, Phys. Rev. D 102 (2020) 123525. arXiv: 2005.04115 [gr-qc].
  7. J. D. Bekenstein, Phys. Rev. D 7 (1973) 2333; Phys. Rev. D 9 (1974) 3292.
  8. S. W. Hawking, Commun. Math. Phys. 43 (1975) 199; Phys. Rev. Lett. 26 (1971) 1344.
  9. S. Basilakos, A. Lymperis, M. Petronikolou and E. N. Saridakis, “ Barrow holographic dark energy with varying exponent,” arXiv: 2312.15767 [gr-qc]
  10. G. ’t Hooft, “The Holographic Principle,” hep-th/0003004.
Citations (2)

Summary

No one has generated a summary of this paper yet.

Paper to Video (Beta)

No one has generated a video about this paper yet.

Whiteboard

No one has generated a whiteboard explanation for this paper yet.

Open Problems

We haven't generated a list of open problems mentioned in this paper yet.

Continue Learning

We haven't generated follow-up questions for this paper yet.

Collections

Sign up for free to add this paper to one or more collections.

Tweets

Sign up for free to view the 1 tweet with 3 likes about this paper.