Thin-shell wormholes from the regular Hayward black hole

Abstract We revisit the regular black hole found by Hayward in %$4%$-dimensional static, spherically symmetric spacetime. To find a possible source for such a spacetime we resort to the nonlinear electrodynamics in general relativity. It is found that a magnetic field within this context gives rise...
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Autor*in:	Halilsoy, M. [verfasserIn] Ovgun, A. [verfasserIn] Mazharimousavi, S. Habib [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2014

Schlagwörter:	Black Hole Black Hole Solution Extremal Black Hole Exotic Matter Regular Black Hole

Übergeordnetes Werk:	Enthalten in: The European physical journal - Berlin : Springer, 1998, 74(2014), 3 vom: 13. März
Übergeordnetes Werk:	volume:74 ; year:2014 ; number:3 ; day:13 ; month:03

Links:	Volltext

DOI / URN:	10.1140/epjc/s10052-014-2796-4

Katalog-ID:	SPR008337608

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520			\|a Abstract We revisit the regular black hole found by Hayward in %$4%$-dimensional static, spherically symmetric spacetime. To find a possible source for such a spacetime we resort to the nonlinear electrodynamics in general relativity. It is found that a magnetic field within this context gives rise to the regular Hayward black hole. By employing such a regular black hole we construct a thin-shell wormhole for the case of various equations of state on the shell. We abbreviate a general equation of state by %$p=\psi (\sigma )%$ where %$p%$ is the surface pressure which is a function of the mass density %$(\sigma )%$. In particular, linear, logarithmic, Chaplygin, etc. forms of equations of state are considered. In each case we study the stability of the thin shell against linear perturbations. We plot the stability regions by tuning the parameters of the theory. It is observed that the role of the Hayward parameter is to make the TSW more stable. Perturbations of the throat with small velocity condition are also studied. The matter of our TSWs, however, remains exotic.
650		4	\|a Black Hole \|7 (dpeaa)DE-He213
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650		4	\|a Extremal Black Hole \|7 (dpeaa)DE-He213
650		4	\|a Exotic Matter \|7 (dpeaa)DE-He213
650		4	\|a Regular Black Hole \|7 (dpeaa)DE-He213
700	1		\|a Ovgun, A. \|e verfasserin \|4 aut
700	1		\|a Mazharimousavi, S. Habib \|e verfasserin \|4 aut
773	0	8	\|i Enthalten in \|t The European physical journal \|d Berlin : Springer, 1998 \|g 74(2014), 3 vom: 13. März \|w (DE-627)253722934 \|w (DE-600)1459069-4 \|x 1434-6052 \|7 nnns
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912			\|a GBV_ILN_22
912			\|a GBV_ILN_23
912			\|a GBV_ILN_24
912			\|a GBV_ILN_31
912			\|a GBV_ILN_39
912			\|a GBV_ILN_40
912			\|a GBV_ILN_60
912			\|a GBV_ILN_62
912			\|a GBV_ILN_63
912			\|a GBV_ILN_69
912			\|a GBV_ILN_70
912			\|a GBV_ILN_73
912			\|a GBV_ILN_95
912			\|a GBV_ILN_105
912			\|a GBV_ILN_110
912			\|a GBV_ILN_150
912			\|a GBV_ILN_151
912			\|a GBV_ILN_161
912			\|a GBV_ILN_170
912			\|a GBV_ILN_206
912			\|a GBV_ILN_213
912			\|a GBV_ILN_230
912			\|a GBV_ILN_267
912			\|a GBV_ILN_285
912			\|a GBV_ILN_293
912			\|a GBV_ILN_370
912			\|a GBV_ILN_602
912			\|a GBV_ILN_702
912			\|a GBV_ILN_2001
912			\|a GBV_ILN_2003
912			\|a GBV_ILN_2005
912			\|a GBV_ILN_2006
912			\|a GBV_ILN_2007
912			\|a GBV_ILN_2008
912			\|a GBV_ILN_2009
912			\|a GBV_ILN_2010
912			\|a GBV_ILN_2011
912			\|a GBV_ILN_2014
912			\|a GBV_ILN_2015
912			\|a GBV_ILN_2018
912			\|a GBV_ILN_2020
912			\|a GBV_ILN_2021
912			\|a GBV_ILN_2025
912			\|a GBV_ILN_2026
912			\|a GBV_ILN_2031
912			\|a GBV_ILN_2034
912			\|a GBV_ILN_2037
912			\|a GBV_ILN_2038
912			\|a GBV_ILN_2039
912			\|a GBV_ILN_2044
912			\|a GBV_ILN_2048
912			\|a GBV_ILN_2050
912			\|a GBV_ILN_2055
912			\|a GBV_ILN_2056
912			\|a GBV_ILN_2057
912			\|a GBV_ILN_2059
912			\|a GBV_ILN_2061
912			\|a GBV_ILN_2064
912			\|a GBV_ILN_2068
912			\|a GBV_ILN_2106
912			\|a GBV_ILN_2108
912			\|a GBV_ILN_2111
912			\|a GBV_ILN_2112
912			\|a GBV_ILN_2113
912			\|a GBV_ILN_2116
912			\|a GBV_ILN_2118
912			\|a GBV_ILN_2119
912			\|a GBV_ILN_2122
912			\|a GBV_ILN_2129
912			\|a GBV_ILN_2143
912			\|a GBV_ILN_2144
912			\|a GBV_ILN_2147
912			\|a GBV_ILN_2148
912			\|a GBV_ILN_2153
912			\|a GBV_ILN_2190
912			\|a GBV_ILN_2232
912			\|a GBV_ILN_4012
912			\|a GBV_ILN_4037
912			\|a GBV_ILN_4112
912			\|a GBV_ILN_4125
912			\|a GBV_ILN_4126
912			\|a GBV_ILN_4246
912			\|a GBV_ILN_4249
912			\|a GBV_ILN_4305
912			\|a GBV_ILN_4306
912			\|a GBV_ILN_4307
912			\|a GBV_ILN_4313
912			\|a GBV_ILN_4322
912			\|a GBV_ILN_4323
912			\|a GBV_ILN_4324
912			\|a GBV_ILN_4325
912			\|a GBV_ILN_4335
912			\|a GBV_ILN_4338
912			\|a GBV_ILN_4367
912			\|a GBV_ILN_4700
936	b	k	\|a 33.50 \|q ASE
951			\|a AR
952			\|d 74 \|j 2014 \|e 3 \|b 13 \|c 03

Indexfelder

author_variant	m h mh a o ao s h m sh shm
matchkey_str	article:14346052:2014----::hnhlwrhlsrmhrglraw
hierarchy_sort_str	2014
bklnumber	33.50
publishDate	2014
allfields	10.1140/epjc/s10052-014-2796-4 doi (DE-627)SPR008337608 (SPR)s10052-014-2796-4-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Halilsoy, M. verfasserin aut Thin-shell wormholes from the regular Hayward black hole 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We revisit the regular black hole found by Hayward in %$4%$-dimensional static, spherically symmetric spacetime. To find a possible source for such a spacetime we resort to the nonlinear electrodynamics in general relativity. It is found that a magnetic field within this context gives rise to the regular Hayward black hole. By employing such a regular black hole we construct a thin-shell wormhole for the case of various equations of state on the shell. We abbreviate a general equation of state by %$p=\psi (\sigma )%$ where %$p%$ is the surface pressure which is a function of the mass density %$(\sigma )%$. In particular, linear, logarithmic, Chaplygin, etc. forms of equations of state are considered. In each case we study the stability of the thin shell against linear perturbations. We plot the stability regions by tuning the parameters of the theory. It is observed that the role of the Hayward parameter is to make the TSW more stable. Perturbations of the throat with small velocity condition are also studied. The matter of our TSWs, however, remains exotic. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Extremal Black Hole (dpeaa)DE-He213 Exotic Matter (dpeaa)DE-He213 Regular Black Hole (dpeaa)DE-He213 Ovgun, A. verfasserin aut Mazharimousavi, S. Habib verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 74(2014), 3 vom: 13. März (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:74 year:2014 number:3 day:13 month:03 https://dx.doi.org/10.1140/epjc/s10052-014-2796-4 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_2007 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_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 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 74 2014 3 13 03
spelling	10.1140/epjc/s10052-014-2796-4 doi (DE-627)SPR008337608 (SPR)s10052-014-2796-4-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Halilsoy, M. verfasserin aut Thin-shell wormholes from the regular Hayward black hole 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We revisit the regular black hole found by Hayward in %$4%$-dimensional static, spherically symmetric spacetime. To find a possible source for such a spacetime we resort to the nonlinear electrodynamics in general relativity. It is found that a magnetic field within this context gives rise to the regular Hayward black hole. By employing such a regular black hole we construct a thin-shell wormhole for the case of various equations of state on the shell. We abbreviate a general equation of state by %$p=\psi (\sigma )%$ where %$p%$ is the surface pressure which is a function of the mass density %$(\sigma )%$. In particular, linear, logarithmic, Chaplygin, etc. forms of equations of state are considered. In each case we study the stability of the thin shell against linear perturbations. We plot the stability regions by tuning the parameters of the theory. It is observed that the role of the Hayward parameter is to make the TSW more stable. Perturbations of the throat with small velocity condition are also studied. The matter of our TSWs, however, remains exotic. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Extremal Black Hole (dpeaa)DE-He213 Exotic Matter (dpeaa)DE-He213 Regular Black Hole (dpeaa)DE-He213 Ovgun, A. verfasserin aut Mazharimousavi, S. Habib verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 74(2014), 3 vom: 13. März (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:74 year:2014 number:3 day:13 month:03 https://dx.doi.org/10.1140/epjc/s10052-014-2796-4 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_2007 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_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 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 74 2014 3 13 03
allfields_unstemmed	10.1140/epjc/s10052-014-2796-4 doi (DE-627)SPR008337608 (SPR)s10052-014-2796-4-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Halilsoy, M. verfasserin aut Thin-shell wormholes from the regular Hayward black hole 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We revisit the regular black hole found by Hayward in %$4%$-dimensional static, spherically symmetric spacetime. To find a possible source for such a spacetime we resort to the nonlinear electrodynamics in general relativity. It is found that a magnetic field within this context gives rise to the regular Hayward black hole. By employing such a regular black hole we construct a thin-shell wormhole for the case of various equations of state on the shell. We abbreviate a general equation of state by %$p=\psi (\sigma )%$ where %$p%$ is the surface pressure which is a function of the mass density %$(\sigma )%$. In particular, linear, logarithmic, Chaplygin, etc. forms of equations of state are considered. In each case we study the stability of the thin shell against linear perturbations. We plot the stability regions by tuning the parameters of the theory. It is observed that the role of the Hayward parameter is to make the TSW more stable. Perturbations of the throat with small velocity condition are also studied. The matter of our TSWs, however, remains exotic. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Extremal Black Hole (dpeaa)DE-He213 Exotic Matter (dpeaa)DE-He213 Regular Black Hole (dpeaa)DE-He213 Ovgun, A. verfasserin aut Mazharimousavi, S. Habib verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 74(2014), 3 vom: 13. März (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:74 year:2014 number:3 day:13 month:03 https://dx.doi.org/10.1140/epjc/s10052-014-2796-4 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_2007 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_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 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 74 2014 3 13 03
allfieldsGer	10.1140/epjc/s10052-014-2796-4 doi (DE-627)SPR008337608 (SPR)s10052-014-2796-4-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Halilsoy, M. verfasserin aut Thin-shell wormholes from the regular Hayward black hole 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We revisit the regular black hole found by Hayward in %$4%$-dimensional static, spherically symmetric spacetime. To find a possible source for such a spacetime we resort to the nonlinear electrodynamics in general relativity. It is found that a magnetic field within this context gives rise to the regular Hayward black hole. By employing such a regular black hole we construct a thin-shell wormhole for the case of various equations of state on the shell. We abbreviate a general equation of state by %$p=\psi (\sigma )%$ where %$p%$ is the surface pressure which is a function of the mass density %$(\sigma )%$. In particular, linear, logarithmic, Chaplygin, etc. forms of equations of state are considered. In each case we study the stability of the thin shell against linear perturbations. We plot the stability regions by tuning the parameters of the theory. It is observed that the role of the Hayward parameter is to make the TSW more stable. Perturbations of the throat with small velocity condition are also studied. The matter of our TSWs, however, remains exotic. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Extremal Black Hole (dpeaa)DE-He213 Exotic Matter (dpeaa)DE-He213 Regular Black Hole (dpeaa)DE-He213 Ovgun, A. verfasserin aut Mazharimousavi, S. Habib verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 74(2014), 3 vom: 13. März (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:74 year:2014 number:3 day:13 month:03 https://dx.doi.org/10.1140/epjc/s10052-014-2796-4 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_2007 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_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 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 74 2014 3 13 03
allfieldsSound	10.1140/epjc/s10052-014-2796-4 doi (DE-627)SPR008337608 (SPR)s10052-014-2796-4-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Halilsoy, M. verfasserin aut Thin-shell wormholes from the regular Hayward black hole 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We revisit the regular black hole found by Hayward in %$4%$-dimensional static, spherically symmetric spacetime. To find a possible source for such a spacetime we resort to the nonlinear electrodynamics in general relativity. It is found that a magnetic field within this context gives rise to the regular Hayward black hole. By employing such a regular black hole we construct a thin-shell wormhole for the case of various equations of state on the shell. We abbreviate a general equation of state by %$p=\psi (\sigma )%$ where %$p%$ is the surface pressure which is a function of the mass density %$(\sigma )%$. In particular, linear, logarithmic, Chaplygin, etc. forms of equations of state are considered. In each case we study the stability of the thin shell against linear perturbations. We plot the stability regions by tuning the parameters of the theory. It is observed that the role of the Hayward parameter is to make the TSW more stable. Perturbations of the throat with small velocity condition are also studied. The matter of our TSWs, however, remains exotic. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Extremal Black Hole (dpeaa)DE-He213 Exotic Matter (dpeaa)DE-He213 Regular Black Hole (dpeaa)DE-He213 Ovgun, A. verfasserin aut Mazharimousavi, S. Habib verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 74(2014), 3 vom: 13. März (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:74 year:2014 number:3 day:13 month:03 https://dx.doi.org/10.1140/epjc/s10052-014-2796-4 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_2007 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_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 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 74 2014 3 13 03
language	English
source	Enthalten in The European physical journal 74(2014), 3 vom: 13. März volume:74 year:2014 number:3 day:13 month:03
sourceStr	Enthalten in The European physical journal 74(2014), 3 vom: 13. März volume:74 year:2014 number:3 day:13 month:03
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Black Hole Black Hole Solution Extremal Black Hole Exotic Matter Regular Black Hole
dewey-raw	530
isfreeaccess_bool	true
container_title	The European physical journal
authorswithroles_txt_mv	Halilsoy, M. @@aut@@ Ovgun, A. @@aut@@ Mazharimousavi, S. Habib @@aut@@
publishDateDaySort_date	2014-03-13T00:00:00Z
hierarchy_top_id	253722934
dewey-sort	3530
id	SPR008337608
language_de	englisch
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author	Halilsoy, M.
spellingShingle	Halilsoy, M. ddc 530 bkl 33.50 misc Black Hole misc Black Hole Solution misc Extremal Black Hole misc Exotic Matter misc Regular Black Hole Thin-shell wormholes from the regular Hayward black hole
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topic_title	530 ASE 33.50 bkl Thin-shell wormholes from the regular Hayward black hole Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Extremal Black Hole (dpeaa)DE-He213 Exotic Matter (dpeaa)DE-He213 Regular Black Hole (dpeaa)DE-He213
topic	ddc 530 bkl 33.50 misc Black Hole misc Black Hole Solution misc Extremal Black Hole misc Exotic Matter misc Regular Black Hole
topic_unstemmed	ddc 530 bkl 33.50 misc Black Hole misc Black Hole Solution misc Extremal Black Hole misc Exotic Matter misc Regular Black Hole
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title	Thin-shell wormholes from the regular Hayward black hole
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title_full	Thin-shell wormholes from the regular Hayward black hole
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title_sort	thin-shell wormholes from the regular hayward black hole
title_auth	Thin-shell wormholes from the regular Hayward black hole
abstract	Abstract We revisit the regular black hole found by Hayward in %$4%$-dimensional static, spherically symmetric spacetime. To find a possible source for such a spacetime we resort to the nonlinear electrodynamics in general relativity. It is found that a magnetic field within this context gives rise to the regular Hayward black hole. By employing such a regular black hole we construct a thin-shell wormhole for the case of various equations of state on the shell. We abbreviate a general equation of state by %$p=\psi (\sigma )%$ where %$p%$ is the surface pressure which is a function of the mass density %$(\sigma )%$. In particular, linear, logarithmic, Chaplygin, etc. forms of equations of state are considered. In each case we study the stability of the thin shell against linear perturbations. We plot the stability regions by tuning the parameters of the theory. It is observed that the role of the Hayward parameter is to make the TSW more stable. Perturbations of the throat with small velocity condition are also studied. The matter of our TSWs, however, remains exotic.
abstractGer	Abstract We revisit the regular black hole found by Hayward in %$4%$-dimensional static, spherically symmetric spacetime. To find a possible source for such a spacetime we resort to the nonlinear electrodynamics in general relativity. It is found that a magnetic field within this context gives rise to the regular Hayward black hole. By employing such a regular black hole we construct a thin-shell wormhole for the case of various equations of state on the shell. We abbreviate a general equation of state by %$p=\psi (\sigma )%$ where %$p%$ is the surface pressure which is a function of the mass density %$(\sigma )%$. In particular, linear, logarithmic, Chaplygin, etc. forms of equations of state are considered. In each case we study the stability of the thin shell against linear perturbations. We plot the stability regions by tuning the parameters of the theory. It is observed that the role of the Hayward parameter is to make the TSW more stable. Perturbations of the throat with small velocity condition are also studied. The matter of our TSWs, however, remains exotic.
abstract_unstemmed	Abstract We revisit the regular black hole found by Hayward in %$4%$-dimensional static, spherically symmetric spacetime. To find a possible source for such a spacetime we resort to the nonlinear electrodynamics in general relativity. It is found that a magnetic field within this context gives rise to the regular Hayward black hole. By employing such a regular black hole we construct a thin-shell wormhole for the case of various equations of state on the shell. We abbreviate a general equation of state by %$p=\psi (\sigma )%$ where %$p%$ is the surface pressure which is a function of the mass density %$(\sigma )%$. In particular, linear, logarithmic, Chaplygin, etc. forms of equations of state are considered. In each case we study the stability of the thin shell against linear perturbations. We plot the stability regions by tuning the parameters of the theory. It is observed that the role of the Hayward parameter is to make the TSW more stable. Perturbations of the throat with small velocity condition are also studied. The matter of our TSWs, however, remains exotic.
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title_short	Thin-shell wormholes from the regular Hayward black hole
url	https://dx.doi.org/10.1140/epjc/s10052-014-2796-4
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up_date	2024-07-03T19:12:33.314Z
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score	7.397217

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Thin-shell wormholes from the regular Hayward black hole

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