Barrow fractal entropy and the black hole quasinormal modes

Using the Boltzmann-Gibbs statistical mechanics together with the quasinormal modes of the black holes and the Bekenstein-Hawking area entropy law, we can determine univocally the lowest possible value for the spin j, which is j...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Abreu, Everton M.C. [verfasserIn] Ananias Neto, Jorge [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2020

Schlagwörter:	Loop Quantum Gravity Barrow entropy Immirzi parameter

Übergeordnetes Werk:	Enthalten in: Physics letters - Amsterdam : North-Holland Publ, 2011, 807
Übergeordnetes Werk:	volume:807

DOI / URN:	10.1016/j.physletb.2020.135602

Katalog-ID:	ELV051085941

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520			\|a Using the Boltzmann-Gibbs statistical mechanics together with the quasinormal modes of the black holes and the Bekenstein-Hawking area entropy law, we can determine univocally the lowest possible value for the spin j, which is j m i n = 1 , in the framework of the Loop Quantum Gravity theory. Subsequently, the value of Immirzi parameter is given by γ = ln ⁡ 3 / ( 2 π 2 ) . In this paper, we have demonstrated that if we use the Barrow formulation for the black hole entropy then the minimum value of the label j depends on the value, which characterizes the fractal structure of the black hole surface called Δ parameter, and may have values other than j m i n = 1 .
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allfields	10.1016/j.physletb.2020.135602 doi (DE-627)ELV051085941 (ELSEVIER)S0370-2693(20)30406-8 DE-627 ger DE-627 rda eng 530 VZ Abreu, Everton M.C. verfasserin (orcid)0000-0002-6638-2588 aut Barrow fractal entropy and the black hole quasinormal modes 2020 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Using the Boltzmann-Gibbs statistical mechanics together with the quasinormal modes of the black holes and the Bekenstein-Hawking area entropy law, we can determine univocally the lowest possible value for the spin j, which is j m i n = 1 , in the framework of the Loop Quantum Gravity theory. Subsequently, the value of Immirzi parameter is given by γ = ln ⁡ 3 / ( 2 π 2 ) . In this paper, we have demonstrated that if we use the Barrow formulation for the black hole entropy then the minimum value of the label j depends on the value, which characterizes the fractal structure of the black hole surface called Δ parameter, and may have values other than j m i n = 1 . Loop Quantum Gravity Barrow entropy Immirzi parameter Ananias Neto, Jorge verfasserin aut Enthalten in Physics letters Amsterdam : North-Holland Publ, 2011 807 (DE-627)266015360 (DE-600)1466612-1 nnns volume:807 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 807
spelling	10.1016/j.physletb.2020.135602 doi (DE-627)ELV051085941 (ELSEVIER)S0370-2693(20)30406-8 DE-627 ger DE-627 rda eng 530 VZ Abreu, Everton M.C. verfasserin (orcid)0000-0002-6638-2588 aut Barrow fractal entropy and the black hole quasinormal modes 2020 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Using the Boltzmann-Gibbs statistical mechanics together with the quasinormal modes of the black holes and the Bekenstein-Hawking area entropy law, we can determine univocally the lowest possible value for the spin j, which is j m i n = 1 , in the framework of the Loop Quantum Gravity theory. Subsequently, the value of Immirzi parameter is given by γ = ln ⁡ 3 / ( 2 π 2 ) . In this paper, we have demonstrated that if we use the Barrow formulation for the black hole entropy then the minimum value of the label j depends on the value, which characterizes the fractal structure of the black hole surface called Δ parameter, and may have values other than j m i n = 1 . Loop Quantum Gravity Barrow entropy Immirzi parameter Ananias Neto, Jorge verfasserin aut Enthalten in Physics letters Amsterdam : North-Holland Publ, 2011 807 (DE-627)266015360 (DE-600)1466612-1 nnns volume:807 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 807
allfields_unstemmed	10.1016/j.physletb.2020.135602 doi (DE-627)ELV051085941 (ELSEVIER)S0370-2693(20)30406-8 DE-627 ger DE-627 rda eng 530 VZ Abreu, Everton M.C. verfasserin (orcid)0000-0002-6638-2588 aut Barrow fractal entropy and the black hole quasinormal modes 2020 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Using the Boltzmann-Gibbs statistical mechanics together with the quasinormal modes of the black holes and the Bekenstein-Hawking area entropy law, we can determine univocally the lowest possible value for the spin j, which is j m i n = 1 , in the framework of the Loop Quantum Gravity theory. Subsequently, the value of Immirzi parameter is given by γ = ln ⁡ 3 / ( 2 π 2 ) . In this paper, we have demonstrated that if we use the Barrow formulation for the black hole entropy then the minimum value of the label j depends on the value, which characterizes the fractal structure of the black hole surface called Δ parameter, and may have values other than j m i n = 1 . Loop Quantum Gravity Barrow entropy Immirzi parameter Ananias Neto, Jorge verfasserin aut Enthalten in Physics letters Amsterdam : North-Holland Publ, 2011 807 (DE-627)266015360 (DE-600)1466612-1 nnns volume:807 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 807
allfieldsGer	10.1016/j.physletb.2020.135602 doi (DE-627)ELV051085941 (ELSEVIER)S0370-2693(20)30406-8 DE-627 ger DE-627 rda eng 530 VZ Abreu, Everton M.C. verfasserin (orcid)0000-0002-6638-2588 aut Barrow fractal entropy and the black hole quasinormal modes 2020 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Using the Boltzmann-Gibbs statistical mechanics together with the quasinormal modes of the black holes and the Bekenstein-Hawking area entropy law, we can determine univocally the lowest possible value for the spin j, which is j m i n = 1 , in the framework of the Loop Quantum Gravity theory. Subsequently, the value of Immirzi parameter is given by γ = ln ⁡ 3 / ( 2 π 2 ) . In this paper, we have demonstrated that if we use the Barrow formulation for the black hole entropy then the minimum value of the label j depends on the value, which characterizes the fractal structure of the black hole surface called Δ parameter, and may have values other than j m i n = 1 . Loop Quantum Gravity Barrow entropy Immirzi parameter Ananias Neto, Jorge verfasserin aut Enthalten in Physics letters Amsterdam : North-Holland Publ, 2011 807 (DE-627)266015360 (DE-600)1466612-1 nnns volume:807 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 807
allfieldsSound	10.1016/j.physletb.2020.135602 doi (DE-627)ELV051085941 (ELSEVIER)S0370-2693(20)30406-8 DE-627 ger DE-627 rda eng 530 VZ Abreu, Everton M.C. verfasserin (orcid)0000-0002-6638-2588 aut Barrow fractal entropy and the black hole quasinormal modes 2020 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Using the Boltzmann-Gibbs statistical mechanics together with the quasinormal modes of the black holes and the Bekenstein-Hawking area entropy law, we can determine univocally the lowest possible value for the spin j, which is j m i n = 1 , in the framework of the Loop Quantum Gravity theory. Subsequently, the value of Immirzi parameter is given by γ = ln ⁡ 3 / ( 2 π 2 ) . In this paper, we have demonstrated that if we use the Barrow formulation for the black hole entropy then the minimum value of the label j depends on the value, which characterizes the fractal structure of the black hole surface called Δ parameter, and may have values other than j m i n = 1 . Loop Quantum Gravity Barrow entropy Immirzi parameter Ananias Neto, Jorge verfasserin aut Enthalten in Physics letters Amsterdam : North-Holland Publ, 2011 807 (DE-627)266015360 (DE-600)1466612-1 nnns volume:807 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 807
language	English
source	Enthalten in Physics letters 807 volume:807
sourceStr	Enthalten in Physics letters 807 volume:807
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topic_facet	Loop Quantum Gravity Barrow entropy Immirzi parameter
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authorswithroles_txt_mv	Abreu, Everton M.C. @@aut@@ Ananias Neto, Jorge @@aut@@
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topic_title	530 VZ Barrow fractal entropy and the black hole quasinormal modes Loop Quantum Gravity Barrow entropy Immirzi parameter
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title	Barrow fractal entropy and the black hole quasinormal modes
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title_full	Barrow fractal entropy and the black hole quasinormal modes
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title_sort	barrow fractal entropy and the black hole quasinormal modes
title_auth	Barrow fractal entropy and the black hole quasinormal modes
abstract	Using the Boltzmann-Gibbs statistical mechanics together with the quasinormal modes of the black holes and the Bekenstein-Hawking area entropy law, we can determine univocally the lowest possible value for the spin j, which is j m i n = 1 , in the framework of the Loop Quantum Gravity theory. Subsequently, the value of Immirzi parameter is given by γ = ln ⁡ 3 / ( 2 π 2 ) . In this paper, we have demonstrated that if we use the Barrow formulation for the black hole entropy then the minimum value of the label j depends on the value, which characterizes the fractal structure of the black hole surface called Δ parameter, and may have values other than j m i n = 1 .
abstractGer	Using the Boltzmann-Gibbs statistical mechanics together with the quasinormal modes of the black holes and the Bekenstein-Hawking area entropy law, we can determine univocally the lowest possible value for the spin j, which is j m i n = 1 , in the framework of the Loop Quantum Gravity theory. Subsequently, the value of Immirzi parameter is given by γ = ln ⁡ 3 / ( 2 π 2 ) . In this paper, we have demonstrated that if we use the Barrow formulation for the black hole entropy then the minimum value of the label j depends on the value, which characterizes the fractal structure of the black hole surface called Δ parameter, and may have values other than j m i n = 1 .
abstract_unstemmed	Using the Boltzmann-Gibbs statistical mechanics together with the quasinormal modes of the black holes and the Bekenstein-Hawking area entropy law, we can determine univocally the lowest possible value for the spin j, which is j m i n = 1 , in the framework of the Loop Quantum Gravity theory. Subsequently, the value of Immirzi parameter is given by γ = ln ⁡ 3 / ( 2 π 2 ) . In this paper, we have demonstrated that if we use the Barrow formulation for the black hole entropy then the minimum value of the label j depends on the value, which characterizes the fractal structure of the black hole surface called Δ parameter, and may have values other than j m i n = 1 .
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title_short	Barrow fractal entropy and the black hole quasinormal modes
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up_date	2024-07-06T19:17:35.180Z
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Barrow fractal entropy and the black hole quasinormal modes

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