The Stefan-Boltzmann constant in n-dimensional space
Abstract
For theoretical discussions of black-body radiation in a curved spacetime with n spatial dimensions, as envisaged in current superstring theories, one wants to know the n-dimensional generalisation of the main standard results. These are given, but only for zero curvature, namely the Planck distribution, the Wien displacement law and the Stefan-Boltzmann law.
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The (1+1)-dimensional Stefan-Boltzmann law states that the rate of energy loss from the black hole is dM/dv = c_evap π /12 β^2.
“The (1 + 1)-dimensional Stefan-Boltzman law [55] states that the rate of energy loss from the black hole is given by dM dv = c evap π 12 β 2 ,(2.15)”
From Entanglement wedge reconstruction and the information paradox (2020) · cites this paper as [55]
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- Authors
- Landsberg, P. T., & Vos, A. D.
- Affiliations
- University of Southampton (GB)
- Venue
- Journal of Physics A: Mathematical and General
- Publisher
- IOP Publishing
- Published
- 1989-04-21
- Volume
- 22
- Issue
- 8
- Pages
- 1073-1084
- ISSN
- 0305-4470 (ISSN-L)
- 1361-6447
- OpenAlex
- W1975544955
- Cited by
- 86
- References
- 5
- Citations by year
- 2026: 3 · 2025: 9 · 2024: 10 · 2023: 6 · 2022: 4 · 2021: 4 · 2020: 7 · 2019: 13 · 2018: 4 · 2017: 1 · 2016: 4 · 2015: 3 · 2014: 6 · 2013: 3
- FWCI
- 0.00
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Journal of Physics A Mathematical and General (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Keywords
- Stefan-Boltzmann law, blackbody radiation, curved spacetime, n-dimensional spacetime, superstring theory, Planck distribution, Wien displacement law, general relativity
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