Landauer's principle;
Area spectrum;
Bekenstein-Hawking entropy;
Logarithmic corrections to entropy;
SPECTRUM;
ENTROPY;
KERR;
D O I:
10.1007/s10714-024-03296-8
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
This article assesses Landauer's principle from information theory in the context of area quantization of the Schwarzschild black hole. Within a quantum-mechanical perspective where Hawking evaporation can be interpreted in terms of transitions between the discrete states of the area (or mass) spectrum, we justify that Landauer's principle holds consistently in the saturated form when the number of microstates of the black hole goes as 2n\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$2<^>n$$\end{document}, where n\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$n$$\end{document} is a large positive integer labeling the levels of the area/mass spectrum in the semiclassical regime. This is equivalent to the area spacing Delta A=alpha lP2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\Delta A = \alpha l_P<^>2$$\end{document} (in natural units), where alpha=4ln2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\alpha = 4 \ln 2$$\end{document} for which the entropy spacing between consecutive levels in Boltzmann units coincides exactly with one bit of information. We also comment on the situation for other values of alpha\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\alpha $$\end{document} prevalent in the literature.
机构:
Univ Pretoria, Dept Phys, ZA-0002 Pretoria, South AfricaNatl Univ La Plata, CREG, CONICET, RA-1900 La Plata, Argentina
Zander, Claudia
Ricardo Plastino, Angel
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h-index: 0
机构:
Natl Univ La Plata, CREG, CONICET, RA-1900 La Plata, Argentina
Univ Pretoria, Dept Phys, ZA-0002 Pretoria, South Africa
Univ Granada, Fac Ciencias, Inst Fis Teor & Computac Carlos I, Granada, SpainNatl Univ La Plata, CREG, CONICET, RA-1900 La Plata, Argentina
Ricardo Plastino, Angel
Plastino, Angelo
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h-index: 0
机构:
Natl Univ La Plata, CREG, CONICET, RA-1900 La Plata, ArgentinaNatl Univ La Plata, CREG, CONICET, RA-1900 La Plata, Argentina
Plastino, Angelo
Casas, Montserrat
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h-index: 0
机构:
Univ Illes Balears, Dept Fis, Mallorca, SpainNatl Univ La Plata, CREG, CONICET, RA-1900 La Plata, Argentina
Casas, Montserrat
Curilef, Sergio
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h-index: 0
机构:
Univ Catolica Norte, Dept Fis, Antofagasta, ChileNatl Univ La Plata, CREG, CONICET, RA-1900 La Plata, Argentina
机构:
Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, I-00133 Rome, ItalyUniv Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, I-00133 Rome, Italy