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The resolution of an entropy puzzle for 4D non-BPS black holes

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dc.contributor.author BANERJEE, NABAMITA en_US
dc.contributor.author Bansal, Sukruti en_US
dc.contributor.author Lodato, Ivano en_US
dc.date.accessioned 2019-04-26T09:15:24Z
dc.date.available 2019-04-26T09:15:24Z
dc.date.issued 2016-05 en_US
dc.identifier.citation Journal of High Energy Physics, 2016(142). en_US
dc.identifier.issn 1126-6708 en_US
dc.identifier.issn 1029-8479 en_US
dc.identifier.uri http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/2546
dc.identifier.uri https://doi.org/10.1007/JHEP05(2016)142 en_US
dc.description.abstract We show the equality between macroscopic and microscopic (statistical) black hole entropy for a class of four dimensional non-supersymmetric black holes in N = 2 supergravity theory, up to the first subleading order in their charges. This solves a long standing entropy puzzle for this class of black holes. The macroscopic entropy has been computed in the presence of a newly derived higher-derivative supersymmetric invariant of [1], connected to the five dimensional supersymmetric Weyl squared Lagrangian. Microscopically, the crucial role in obtaining the equivalence is played by the anomalous gauge gravitational Chern-Simons term en_US
dc.language.iso en en_US
dc.publisher Springer Nature en_US
dc.subject Black Holes en_US
dc.subject String Theory en_US
dc.subject Chern-Simons Theories en_US
dc.subject Supergravity Models en_US
dc.subject Resolution of an entropy puzzle en_US
dc.subject 2016 en_US
dc.title The resolution of an entropy puzzle for 4D non-BPS black holes en_US
dc.type Article en_US
dc.contributor.department Dept. of Physics en_US
dc.identifier.sourcetitle Journal of High Energy Physics en_US
dc.publication.originofpublisher Foreign en_US


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