Salvato in:
Dettagli Bibliografici
Autori principali: Halder, Indranil, Vafa, Cumrun, Xu, Kai
Natura: Preprint
Pubblicazione: 2024
Soggetti:
Accesso online:https://arxiv.org/abs/2404.01380
Tags: Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
_version_ 1866917628703932416
author Halder, Indranil
Vafa, Cumrun
Xu, Kai
author_facet Halder, Indranil
Vafa, Cumrun
Xu, Kai
contents Microscopic black hole entropy calculations in string theory usually proceeds through identifying them as wrapped strings in one higher dimension. For M-theory on elliptic Calabi-Yau threefolds this proceeds via its relation to F-theory in one higher dimension. Here we show how this method can be extended to M-theory on non-elliptic Calabi-Yau threefolds such as the quintic via conifold transition to elliptic threefolds. This leads to the computation of the black hole entropy through elliptic genera of the strings. However the Cardy formula for the computation of the black hole entropy of these strings fails because the relevant momentum excitations on the string are much smaller than the central charge of the strings. We show how the black hole attractor entropy formula leads to predicting corrections to the Cardy formula in this regime.
format Preprint
id arxiv_https___arxiv_org_abs_2404_01380
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Black Hole Entropy for M-theory on the Quintic Threefold via F-theoretic Strings
Halder, Indranil
Vafa, Cumrun
Xu, Kai
High Energy Physics - Theory
Mathematical Physics
Microscopic black hole entropy calculations in string theory usually proceeds through identifying them as wrapped strings in one higher dimension. For M-theory on elliptic Calabi-Yau threefolds this proceeds via its relation to F-theory in one higher dimension. Here we show how this method can be extended to M-theory on non-elliptic Calabi-Yau threefolds such as the quintic via conifold transition to elliptic threefolds. This leads to the computation of the black hole entropy through elliptic genera of the strings. However the Cardy formula for the computation of the black hole entropy of these strings fails because the relevant momentum excitations on the string are much smaller than the central charge of the strings. We show how the black hole attractor entropy formula leads to predicting corrections to the Cardy formula in this regime.
title Black Hole Entropy for M-theory on the Quintic Threefold via F-theoretic Strings
topic High Energy Physics - Theory
Mathematical Physics
url https://arxiv.org/abs/2404.01380