Resonance Spectra of Caged Stringy Black Hole and Its Spectroscopy

Maggiore’s method (MM), which evaluates the transition frequency that appears in the adiabatic invariant from the highly damped quasinormal mode (QNM) frequencies, is used to investigate the entropy/area spectra of the Garfinkle–Horowitz–Strominger black hole (GHSBH). Instead of the ordinary QNMs, w...

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Main Authors: I. Sakalli, G. Tokgoz
Format: Article
Language:English
Published: Wiley 2015-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2015/739153
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author I. Sakalli
G. Tokgoz
author_facet I. Sakalli
G. Tokgoz
author_sort I. Sakalli
collection DOAJ
description Maggiore’s method (MM), which evaluates the transition frequency that appears in the adiabatic invariant from the highly damped quasinormal mode (QNM) frequencies, is used to investigate the entropy/area spectra of the Garfinkle–Horowitz–Strominger black hole (GHSBH). Instead of the ordinary QNMs, we compute the boxed QNMs (BQNMs) that are the characteristic resonance spectra of the confined scalar fields in the GHSBH geometry. For this purpose, we assume that the GHSBH has a confining cavity (mirror) placed in the vicinity of the event horizon. We then show how the complex resonant frequencies of the caged GHSBH are computed using the Bessel differential equation that arises when the scalar perturbations around the event horizon are considered. Although the entropy/area is characterized by the GHSBH parameters, their quantization is shown to be independent of those parameters. However, both spectra are equally spaced.
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spelling doaj-art-570c3f8004864dd3849cfc6bce57a14f2025-02-03T06:44:21ZengWileyAdvances in High Energy Physics1687-73571687-73652015-01-01201510.1155/2015/739153739153Resonance Spectra of Caged Stringy Black Hole and Its SpectroscopyI. Sakalli0G. Tokgoz1Department of Physics, Eastern Mediterranean University, Gazimagosa, Northern Cyprus, Mersin 10, TurkeyDepartment of Physics, Eastern Mediterranean University, Gazimagosa, Northern Cyprus, Mersin 10, TurkeyMaggiore’s method (MM), which evaluates the transition frequency that appears in the adiabatic invariant from the highly damped quasinormal mode (QNM) frequencies, is used to investigate the entropy/area spectra of the Garfinkle–Horowitz–Strominger black hole (GHSBH). Instead of the ordinary QNMs, we compute the boxed QNMs (BQNMs) that are the characteristic resonance spectra of the confined scalar fields in the GHSBH geometry. For this purpose, we assume that the GHSBH has a confining cavity (mirror) placed in the vicinity of the event horizon. We then show how the complex resonant frequencies of the caged GHSBH are computed using the Bessel differential equation that arises when the scalar perturbations around the event horizon are considered. Although the entropy/area is characterized by the GHSBH parameters, their quantization is shown to be independent of those parameters. However, both spectra are equally spaced.http://dx.doi.org/10.1155/2015/739153
spellingShingle I. Sakalli
G. Tokgoz
Resonance Spectra of Caged Stringy Black Hole and Its Spectroscopy
Advances in High Energy Physics
title Resonance Spectra of Caged Stringy Black Hole and Its Spectroscopy
title_full Resonance Spectra of Caged Stringy Black Hole and Its Spectroscopy
title_fullStr Resonance Spectra of Caged Stringy Black Hole and Its Spectroscopy
title_full_unstemmed Resonance Spectra of Caged Stringy Black Hole and Its Spectroscopy
title_short Resonance Spectra of Caged Stringy Black Hole and Its Spectroscopy
title_sort resonance spectra of caged stringy black hole and its spectroscopy
url http://dx.doi.org/10.1155/2015/739153
work_keys_str_mv AT isakalli resonancespectraofcagedstringyblackholeanditsspectroscopy
AT gtokgoz resonancespectraofcagedstringyblackholeanditsspectroscopy