2022
DOI: 10.48550/arxiv.2202.04657
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Large and Small Non-extremal Black Holes, Thermodynamic Dualities, and the Swampland

Abstract: In this paper we discuss black hole solutions parametrized by their entropy S and temperature T in gravitational effective theories. We are especially interested in the analysis of the boundary regions in the T − S diagram, i.e. large/small values of entropy and temperature, and their relation to Swampland constraints. To explore this correlation, we couple the gravitational theories to scalar fields and connect limits of thermodynamic quantities of black holes to scalar field excursions in the corresponding s… Show more

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Cited by 2 publications
(6 citation statements)
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References 57 publications
(106 reference statements)
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“…Using (4. 19) we find that the r.h.s. of (4.48) indeed coincides with the inverse of (4.46) for e = (1, −1).…”
Section: Jhep08(2022)004mentioning
confidence: 71%
See 1 more Smart Citation
“…Using (4. 19) we find that the r.h.s. of (4.48) indeed coincides with the inverse of (4.46) for e = (1, −1).…”
Section: Jhep08(2022)004mentioning
confidence: 71%
“…In general, it was found that the physics of local EFT string solutions characterises the EFT itself along infinite distance limits. It is in this sense that properties of objects with non-trivial backreaction serve to probe the EFT and uncover its structure and limitations, an idea that has been recently applied in different contexts [9][10][11][12][13][14][15][16][17][18][19].…”
Section: Jhep08(2022)004mentioning
confidence: 99%
“…to the Schwarzschild case. The physical region of the parameter space for the Hawking temperature and entropy is shown in the in figure 1, which is taken from [57].…”
Section: Extremal and Non-extremal Charged Black Holesmentioning
confidence: 99%
“…The lowest order black hole entropy, i.e. without higher curvature contributions, and the extremality parameter c are related in the following way [57,58] 6…”
Section: Jhep06(2024)127mentioning
confidence: 99%
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