Charged Gauss–Bonnet black holes supporting non-minimally coupled scalar clouds: analytic treatment in the near-critical regime

Abstract Recent numerical studies have revealed the physically intriguing fact that charged black holes whose charge-to-mass ratios are larger than the critical value $$(Q/M)_{\text {crit}}=\sqrt{2(9+\sqrt{6})}/5$$ ( Q / M ) crit = 2 ( 9 + 6 ) / 5 can support hairy matter configurations which are ma...

Full description

Bibliographic Details
Main Author: Shahar Hod
Format: Article
Language:English
Published: SpringerOpen 2023-03-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-023-11385-2
_version_ 1797836267339120640
author Shahar Hod
author_facet Shahar Hod
author_sort Shahar Hod
collection DOAJ
description Abstract Recent numerical studies have revealed the physically intriguing fact that charged black holes whose charge-to-mass ratios are larger than the critical value $$(Q/M)_{\text {crit}}=\sqrt{2(9+\sqrt{6})}/5$$ ( Q / M ) crit = 2 ( 9 + 6 ) / 5 can support hairy matter configurations which are made of scalar fields with a non-minimal negative coupling to the Gauss–Bonnet invariant of the curved spacetime. Using analytical techniques, we explore the physical and mathematical properties of the composed charged-black-hole-nonminimally-coupled-linearized-massless-scalar-field configurations in the near-critical $$Q/M\gtrsim (Q/M)_{\text {crit}}$$ Q / M ≳ ( Q / M ) crit regime. In particular, we derive an analytical resonance formula that describes the charge-dependence of the dimensionless coupling parameter $$\bar{\eta }_{\text {crit}}=\bar{\eta }_{\text {crit}}(Q/M)$$ η ¯ crit = η ¯ crit ( Q / M ) of the composed Einstein–Maxwell-nonminimally-coupled-scalar-field system along the existence-line of the theory, a critical border that separates bald Reissner–Nordström black holes from hairy charged-black-hole-scalar-field configurations. In addition, it is explicitly shown that the large-coupling $$-\bar{\eta }_{\text {crit}}(Q/M)\gg 1$$ - η ¯ crit ( Q / M ) ≫ 1 analytical results derived in the present paper for the composed Einstein–Maxwell-scalar theory agree remarkably well with direct numerical computations of the corresponding black-hole-field resonance spectrum.
first_indexed 2024-04-09T15:07:10Z
format Article
id doaj.art-2e372bc9910b4ba9a72aec15da9ae4ce
institution Directory Open Access Journal
issn 1434-6052
language English
last_indexed 2024-04-09T15:07:10Z
publishDate 2023-03-01
publisher SpringerOpen
record_format Article
series European Physical Journal C: Particles and Fields
spelling doaj.art-2e372bc9910b4ba9a72aec15da9ae4ce2023-04-30T11:25:19ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522023-03-018331710.1140/epjc/s10052-023-11385-2Charged Gauss–Bonnet black holes supporting non-minimally coupled scalar clouds: analytic treatment in the near-critical regimeShahar Hod0The Ruppin Academic CenterAbstract Recent numerical studies have revealed the physically intriguing fact that charged black holes whose charge-to-mass ratios are larger than the critical value $$(Q/M)_{\text {crit}}=\sqrt{2(9+\sqrt{6})}/5$$ ( Q / M ) crit = 2 ( 9 + 6 ) / 5 can support hairy matter configurations which are made of scalar fields with a non-minimal negative coupling to the Gauss–Bonnet invariant of the curved spacetime. Using analytical techniques, we explore the physical and mathematical properties of the composed charged-black-hole-nonminimally-coupled-linearized-massless-scalar-field configurations in the near-critical $$Q/M\gtrsim (Q/M)_{\text {crit}}$$ Q / M ≳ ( Q / M ) crit regime. In particular, we derive an analytical resonance formula that describes the charge-dependence of the dimensionless coupling parameter $$\bar{\eta }_{\text {crit}}=\bar{\eta }_{\text {crit}}(Q/M)$$ η ¯ crit = η ¯ crit ( Q / M ) of the composed Einstein–Maxwell-nonminimally-coupled-scalar-field system along the existence-line of the theory, a critical border that separates bald Reissner–Nordström black holes from hairy charged-black-hole-scalar-field configurations. In addition, it is explicitly shown that the large-coupling $$-\bar{\eta }_{\text {crit}}(Q/M)\gg 1$$ - η ¯ crit ( Q / M ) ≫ 1 analytical results derived in the present paper for the composed Einstein–Maxwell-scalar theory agree remarkably well with direct numerical computations of the corresponding black-hole-field resonance spectrum.https://doi.org/10.1140/epjc/s10052-023-11385-2
spellingShingle Shahar Hod
Charged Gauss–Bonnet black holes supporting non-minimally coupled scalar clouds: analytic treatment in the near-critical regime
European Physical Journal C: Particles and Fields
title Charged Gauss–Bonnet black holes supporting non-minimally coupled scalar clouds: analytic treatment in the near-critical regime
title_full Charged Gauss–Bonnet black holes supporting non-minimally coupled scalar clouds: analytic treatment in the near-critical regime
title_fullStr Charged Gauss–Bonnet black holes supporting non-minimally coupled scalar clouds: analytic treatment in the near-critical regime
title_full_unstemmed Charged Gauss–Bonnet black holes supporting non-minimally coupled scalar clouds: analytic treatment in the near-critical regime
title_short Charged Gauss–Bonnet black holes supporting non-minimally coupled scalar clouds: analytic treatment in the near-critical regime
title_sort charged gauss bonnet black holes supporting non minimally coupled scalar clouds analytic treatment in the near critical regime
url https://doi.org/10.1140/epjc/s10052-023-11385-2
work_keys_str_mv AT shaharhod chargedgaussbonnetblackholessupportingnonminimallycoupledscalarcloudsanalytictreatmentinthenearcriticalregime