Instability of Black Holes with a Gauss–Bonnet Term

Abstract We investigate the fragmentation instability of hairy black holes in the theory with a Gauss–Bonnet (GB) term in asymptotically flat spacetime. Our approach is through the non-perturbative fragmentation instability. By this approach, we investigate whether the initial black hole can be brok...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Ahn, Wha-Keun [verfasserIn] Gwak, Bogeun [verfasserIn] Lee, Bum-Hoon [verfasserIn] Lee, Wonwoo [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2015

Schlagwörter:	Black Hole Black Hole Solution Black Hole Mass Minimum Mass Hairy Black Hole

Übergeordnetes Werk:	Enthalten in: The European physical journal - Berlin : Springer, 1998, 75(2015), 8 vom: 15. Aug.
Übergeordnetes Werk:	volume:75 ; year:2015 ; number:8 ; day:15 ; month:08

Links:	Volltext

DOI / URN:	10.1140/epjc/s10052-015-3568-5

Katalog-ID:	SPR008346097

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520			\|a Abstract We investigate the fragmentation instability of hairy black holes in the theory with a Gauss–Bonnet (GB) term in asymptotically flat spacetime. Our approach is through the non-perturbative fragmentation instability. By this approach, we investigate whether the initial black hole can be broken into two black holes by comparing the entropy of the initial black hole with the sum of those of two fragmented black holes. The relation between the black hole instability and the GB coupling with dilaton hair are presented. We describe the phase diagrams with respect to the mass of the black hole solutions and coupling constants. We find that a perturbatively stable black hole can be unstable under fragmentation.
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allfields	10.1140/epjc/s10052-015-3568-5 doi (DE-627)SPR008346097 (SPR)s10052-015-3568-5-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Ahn, Wha-Keun verfasserin aut Instability of Black Holes with a Gauss–Bonnet Term 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We investigate the fragmentation instability of hairy black holes in the theory with a Gauss–Bonnet (GB) term in asymptotically flat spacetime. Our approach is through the non-perturbative fragmentation instability. By this approach, we investigate whether the initial black hole can be broken into two black holes by comparing the entropy of the initial black hole with the sum of those of two fragmented black holes. The relation between the black hole instability and the GB coupling with dilaton hair are presented. We describe the phase diagrams with respect to the mass of the black hole solutions and coupling constants. We find that a perturbatively stable black hole can be unstable under fragmentation. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Black Hole Mass (dpeaa)DE-He213 Minimum Mass (dpeaa)DE-He213 Hairy Black Hole (dpeaa)DE-He213 Gwak, Bogeun verfasserin aut Lee, Bum-Hoon verfasserin aut Lee, Wonwoo verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 8 vom: 15. Aug. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:8 day:15 month:08 https://dx.doi.org/10.1140/epjc/s10052-015-3568-5 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 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 33.50 ASE AR 75 2015 8 15 08
spelling	10.1140/epjc/s10052-015-3568-5 doi (DE-627)SPR008346097 (SPR)s10052-015-3568-5-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Ahn, Wha-Keun verfasserin aut Instability of Black Holes with a Gauss–Bonnet Term 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We investigate the fragmentation instability of hairy black holes in the theory with a Gauss–Bonnet (GB) term in asymptotically flat spacetime. Our approach is through the non-perturbative fragmentation instability. By this approach, we investigate whether the initial black hole can be broken into two black holes by comparing the entropy of the initial black hole with the sum of those of two fragmented black holes. The relation between the black hole instability and the GB coupling with dilaton hair are presented. We describe the phase diagrams with respect to the mass of the black hole solutions and coupling constants. We find that a perturbatively stable black hole can be unstable under fragmentation. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Black Hole Mass (dpeaa)DE-He213 Minimum Mass (dpeaa)DE-He213 Hairy Black Hole (dpeaa)DE-He213 Gwak, Bogeun verfasserin aut Lee, Bum-Hoon verfasserin aut Lee, Wonwoo verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 8 vom: 15. Aug. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:8 day:15 month:08 https://dx.doi.org/10.1140/epjc/s10052-015-3568-5 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 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 33.50 ASE AR 75 2015 8 15 08
allfields_unstemmed	10.1140/epjc/s10052-015-3568-5 doi (DE-627)SPR008346097 (SPR)s10052-015-3568-5-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Ahn, Wha-Keun verfasserin aut Instability of Black Holes with a Gauss–Bonnet Term 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We investigate the fragmentation instability of hairy black holes in the theory with a Gauss–Bonnet (GB) term in asymptotically flat spacetime. Our approach is through the non-perturbative fragmentation instability. By this approach, we investigate whether the initial black hole can be broken into two black holes by comparing the entropy of the initial black hole with the sum of those of two fragmented black holes. The relation between the black hole instability and the GB coupling with dilaton hair are presented. We describe the phase diagrams with respect to the mass of the black hole solutions and coupling constants. We find that a perturbatively stable black hole can be unstable under fragmentation. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Black Hole Mass (dpeaa)DE-He213 Minimum Mass (dpeaa)DE-He213 Hairy Black Hole (dpeaa)DE-He213 Gwak, Bogeun verfasserin aut Lee, Bum-Hoon verfasserin aut Lee, Wonwoo verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 8 vom: 15. Aug. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:8 day:15 month:08 https://dx.doi.org/10.1140/epjc/s10052-015-3568-5 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 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 33.50 ASE AR 75 2015 8 15 08
allfieldsGer	10.1140/epjc/s10052-015-3568-5 doi (DE-627)SPR008346097 (SPR)s10052-015-3568-5-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Ahn, Wha-Keun verfasserin aut Instability of Black Holes with a Gauss–Bonnet Term 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We investigate the fragmentation instability of hairy black holes in the theory with a Gauss–Bonnet (GB) term in asymptotically flat spacetime. Our approach is through the non-perturbative fragmentation instability. By this approach, we investigate whether the initial black hole can be broken into two black holes by comparing the entropy of the initial black hole with the sum of those of two fragmented black holes. The relation between the black hole instability and the GB coupling with dilaton hair are presented. We describe the phase diagrams with respect to the mass of the black hole solutions and coupling constants. We find that a perturbatively stable black hole can be unstable under fragmentation. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Black Hole Mass (dpeaa)DE-He213 Minimum Mass (dpeaa)DE-He213 Hairy Black Hole (dpeaa)DE-He213 Gwak, Bogeun verfasserin aut Lee, Bum-Hoon verfasserin aut Lee, Wonwoo verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 8 vom: 15. Aug. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:8 day:15 month:08 https://dx.doi.org/10.1140/epjc/s10052-015-3568-5 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 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 33.50 ASE AR 75 2015 8 15 08
allfieldsSound	10.1140/epjc/s10052-015-3568-5 doi (DE-627)SPR008346097 (SPR)s10052-015-3568-5-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Ahn, Wha-Keun verfasserin aut Instability of Black Holes with a Gauss–Bonnet Term 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We investigate the fragmentation instability of hairy black holes in the theory with a Gauss–Bonnet (GB) term in asymptotically flat spacetime. Our approach is through the non-perturbative fragmentation instability. By this approach, we investigate whether the initial black hole can be broken into two black holes by comparing the entropy of the initial black hole with the sum of those of two fragmented black holes. The relation between the black hole instability and the GB coupling with dilaton hair are presented. We describe the phase diagrams with respect to the mass of the black hole solutions and coupling constants. We find that a perturbatively stable black hole can be unstable under fragmentation. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Black Hole Mass (dpeaa)DE-He213 Minimum Mass (dpeaa)DE-He213 Hairy Black Hole (dpeaa)DE-He213 Gwak, Bogeun verfasserin aut Lee, Bum-Hoon verfasserin aut Lee, Wonwoo verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 8 vom: 15. Aug. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:8 day:15 month:08 https://dx.doi.org/10.1140/epjc/s10052-015-3568-5 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 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 33.50 ASE AR 75 2015 8 15 08
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source	Enthalten in The European physical journal 75(2015), 8 vom: 15. Aug. volume:75 year:2015 number:8 day:15 month:08
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author	Ahn, Wha-Keun
spellingShingle	Ahn, Wha-Keun ddc 530 bkl 33.50 misc Black Hole misc Black Hole Solution misc Black Hole Mass misc Minimum Mass misc Hairy Black Hole Instability of Black Holes with a Gauss–Bonnet Term
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topic_title	530 ASE 33.50 bkl Instability of Black Holes with a Gauss–Bonnet Term Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Black Hole Mass (dpeaa)DE-He213 Minimum Mass (dpeaa)DE-He213 Hairy Black Hole (dpeaa)DE-He213
topic	ddc 530 bkl 33.50 misc Black Hole misc Black Hole Solution misc Black Hole Mass misc Minimum Mass misc Hairy Black Hole
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title	Instability of Black Holes with a Gauss–Bonnet Term
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title_full	Instability of Black Holes with a Gauss–Bonnet Term
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title_sort	instability of black holes with a gauss–bonnet term
title_auth	Instability of Black Holes with a Gauss–Bonnet Term
abstract	Abstract We investigate the fragmentation instability of hairy black holes in the theory with a Gauss–Bonnet (GB) term in asymptotically flat spacetime. Our approach is through the non-perturbative fragmentation instability. By this approach, we investigate whether the initial black hole can be broken into two black holes by comparing the entropy of the initial black hole with the sum of those of two fragmented black holes. The relation between the black hole instability and the GB coupling with dilaton hair are presented. We describe the phase diagrams with respect to the mass of the black hole solutions and coupling constants. We find that a perturbatively stable black hole can be unstable under fragmentation.
abstractGer	Abstract We investigate the fragmentation instability of hairy black holes in the theory with a Gauss–Bonnet (GB) term in asymptotically flat spacetime. Our approach is through the non-perturbative fragmentation instability. By this approach, we investigate whether the initial black hole can be broken into two black holes by comparing the entropy of the initial black hole with the sum of those of two fragmented black holes. The relation between the black hole instability and the GB coupling with dilaton hair are presented. We describe the phase diagrams with respect to the mass of the black hole solutions and coupling constants. We find that a perturbatively stable black hole can be unstable under fragmentation.
abstract_unstemmed	Abstract We investigate the fragmentation instability of hairy black holes in the theory with a Gauss–Bonnet (GB) term in asymptotically flat spacetime. Our approach is through the non-perturbative fragmentation instability. By this approach, we investigate whether the initial black hole can be broken into two black holes by comparing the entropy of the initial black hole with the sum of those of two fragmented black holes. The relation between the black hole instability and the GB coupling with dilaton hair are presented. We describe the phase diagrams with respect to the mass of the black hole solutions and coupling constants. We find that a perturbatively stable black hole can be unstable under fragmentation.
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title_short	Instability of Black Holes with a Gauss–Bonnet Term
url	https://dx.doi.org/10.1140/epjc/s10052-015-3568-5
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author2	Gwak, Bogeun Lee, Bum-Hoon Lee, Wonwoo
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doi_str	10.1140/epjc/s10052-015-3568-5
up_date	2024-07-03T19:30:04.716Z
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Our approach is through the non-perturbative fragmentation instability. By this approach, we investigate whether the initial black hole can be broken into two black holes by comparing the entropy of the initial black hole with the sum of those of two fragmented black holes. The relation between the black hole instability and the GB coupling with dilaton hair are presented. We describe the phase diagrams with respect to the mass of the black hole solutions and coupling constants. 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Instability of Black Holes with a Gauss–Bonnet Term

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