2021
DOI: 10.1103/physrevd.103.024052
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Topological terms and the Misner string entropy

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Cited by 44 publications
(29 citation statements)
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“…We also consider the role played by the Misner string if κ = 1. This extends previous studies [19][20][21][22]; our aim here is to understand how regularity conditions of the gauge field affect the thermodynamic relations. For the dyonic RN black hole, the first law of thermodynamics is not strongly affected by the regularity condition of the gauge field, and an electric and magnetic charge are independently present in the thermodynamic relations as illustrated in appendix A.…”
Section: Jhep03(2021)039supporting
confidence: 79%
“…We also consider the role played by the Misner string if κ = 1. This extends previous studies [19][20][21][22]; our aim here is to understand how regularity conditions of the gauge field affect the thermodynamic relations. For the dyonic RN black hole, the first law of thermodynamics is not strongly affected by the regularity condition of the gauge field, and an electric and magnetic charge are independently present in the thermodynamic relations as illustrated in appendix A.…”
Section: Jhep03(2021)039supporting
confidence: 79%
“…Another illustrative example is given by the addition of both Gauss-Bonnet and Chern-Pontryagin invariants to the 4D Einstein-AdS gravity. The direct application of NW procedure leads to a charge which is identically vanishing for globally (anti-)self dual solutions, feature that is shared by the total action [34,35]. This reasoning opens the possibility of zero action/zero charges for the whole class of spaces, and not only for a particular solution.…”
Section: Jhep07(2021)156mentioning
confidence: 93%
“…In a complementary manner, in Euclidean configurations, adding topological terms to the action shows that the NUT parameter contributes to the mass [49]. Moreover, from a thermodynamic point of view Misner strings are sources of entropy [50,51]. Lastly, we mention that from an astrophysical point of view, NUT parameters have observable effects on the apparent horizon's shadow [52].…”
Section: Jhep09(2021)104mentioning
confidence: 80%