<p>We study one-loop logarithmic corrections to the entropy of static hyperbolic BPS black holes in asymptotically AdS<sub>4</sub> spacetime. Our analysis is carried out in a consistent real-scalar truncation of <InlineEquation ID="IEq1"> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">N</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{N} \)</EquationSource> </InlineEquation> = 2 Fayet-Iliopoulos gauged supergravity specified by the prepotential <i>F</i> = –<i>iX</i><sup>0</sup><i>X</i><sup>1</sup>, which corresponds to an Einstein-Dilaton-Maxwell theory with a nontrivial scalar potential. In this model, the classical BPS attractor mechanism exhibits flat directions, leaving scalar moduli on the black hole horizon unfixed, while the Bekenstein-Hawking entropy depends only on the charges. We show that the resulting one-loop correction to the black hole entropy acquires a nontrivial dependence on the horizon moduli and induces an effective quantum potential that dynamically stabilizes them at a preferred value. Our results provide an explicit and concrete realization of quantum lifting of classical attractor flat directions in gauged supergravity.</p>

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Moduli-dependent one-loop entropy of hyperbolic BPS black hole in AdS4

  • Imtak Jeon,
  • Alokananda Kar,
  • Binata Panda,
  • Anowar Shaikh

摘要

We study one-loop logarithmic corrections to the entropy of static hyperbolic BPS black holes in asymptotically AdS4 spacetime. Our analysis is carried out in a consistent real-scalar truncation of N \( \mathcal{N} \) = 2 Fayet-Iliopoulos gauged supergravity specified by the prepotential F = –iX0X1, which corresponds to an Einstein-Dilaton-Maxwell theory with a nontrivial scalar potential. In this model, the classical BPS attractor mechanism exhibits flat directions, leaving scalar moduli on the black hole horizon unfixed, while the Bekenstein-Hawking entropy depends only on the charges. We show that the resulting one-loop correction to the black hole entropy acquires a nontrivial dependence on the horizon moduli and induces an effective quantum potential that dynamically stabilizes them at a preferred value. Our results provide an explicit and concrete realization of quantum lifting of classical attractor flat directions in gauged supergravity.