Photon emission of extremal Kerr–Newman black holes

Abstract In this paper, we deal with the null geodesics extending from the near-horizon region out to a distant observatory in an extremal Kerr–Newman black hole background. In particular, using the matched asymptotic expansion method, we analytically solve the null geodesics near the superradiant b...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Wei, Shao-Wen [verfasserIn] Gu, Bao-Min [verfasserIn] Wang, Yong-Qiang [verfasserIn] Liu, Yu-Xiao [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2017

Schlagwörter:	Black Hole Black Hole Solution Black Hole Horizon Extremal Black Hole Null Geodesic

Übergeordnetes Werk:	Enthalten in: The European physical journal - Berlin : Springer, 1998, 77(2017), 2 vom: 24. Feb.
Übergeordnetes Werk:	volume:77 ; year:2017 ; number:2 ; day:24 ; month:02

Links:	Volltext

DOI / URN:	10.1140/epjc/s10052-017-4699-7

Katalog-ID:	SPR008358591

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allfields	10.1140/epjc/s10052-017-4699-7 doi (DE-627)SPR008358591 (SPR)s10052-017-4699-7-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Wei, Shao-Wen verfasserin aut Photon emission of extremal Kerr–Newman black holes 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper, we deal with the null geodesics extending from the near-horizon region out to a distant observatory in an extremal Kerr–Newman black hole background. In particular, using the matched asymptotic expansion method, we analytically solve the null geodesics near the superradiant bound in the form of algebraic equations. For the case that the photon trajectories are limited in the equatorial plane, the shifts in the azimuthal angle and time are obtained. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Black Hole Horizon (dpeaa)DE-He213 Extremal Black Hole (dpeaa)DE-He213 Null Geodesic (dpeaa)DE-He213 Gu, Bao-Min verfasserin aut Wang, Yong-Qiang verfasserin aut Liu, Yu-Xiao verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 77(2017), 2 vom: 24. Feb. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:77 year:2017 number:2 day:24 month:02 https://dx.doi.org/10.1140/epjc/s10052-017-4699-7 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 77 2017 2 24 02
spelling	10.1140/epjc/s10052-017-4699-7 doi (DE-627)SPR008358591 (SPR)s10052-017-4699-7-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Wei, Shao-Wen verfasserin aut Photon emission of extremal Kerr–Newman black holes 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper, we deal with the null geodesics extending from the near-horizon region out to a distant observatory in an extremal Kerr–Newman black hole background. In particular, using the matched asymptotic expansion method, we analytically solve the null geodesics near the superradiant bound in the form of algebraic equations. For the case that the photon trajectories are limited in the equatorial plane, the shifts in the azimuthal angle and time are obtained. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Black Hole Horizon (dpeaa)DE-He213 Extremal Black Hole (dpeaa)DE-He213 Null Geodesic (dpeaa)DE-He213 Gu, Bao-Min verfasserin aut Wang, Yong-Qiang verfasserin aut Liu, Yu-Xiao verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 77(2017), 2 vom: 24. Feb. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:77 year:2017 number:2 day:24 month:02 https://dx.doi.org/10.1140/epjc/s10052-017-4699-7 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 77 2017 2 24 02
allfields_unstemmed	10.1140/epjc/s10052-017-4699-7 doi (DE-627)SPR008358591 (SPR)s10052-017-4699-7-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Wei, Shao-Wen verfasserin aut Photon emission of extremal Kerr–Newman black holes 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper, we deal with the null geodesics extending from the near-horizon region out to a distant observatory in an extremal Kerr–Newman black hole background. In particular, using the matched asymptotic expansion method, we analytically solve the null geodesics near the superradiant bound in the form of algebraic equations. For the case that the photon trajectories are limited in the equatorial plane, the shifts in the azimuthal angle and time are obtained. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Black Hole Horizon (dpeaa)DE-He213 Extremal Black Hole (dpeaa)DE-He213 Null Geodesic (dpeaa)DE-He213 Gu, Bao-Min verfasserin aut Wang, Yong-Qiang verfasserin aut Liu, Yu-Xiao verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 77(2017), 2 vom: 24. Feb. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:77 year:2017 number:2 day:24 month:02 https://dx.doi.org/10.1140/epjc/s10052-017-4699-7 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 77 2017 2 24 02
allfieldsGer	10.1140/epjc/s10052-017-4699-7 doi (DE-627)SPR008358591 (SPR)s10052-017-4699-7-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Wei, Shao-Wen verfasserin aut Photon emission of extremal Kerr–Newman black holes 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper, we deal with the null geodesics extending from the near-horizon region out to a distant observatory in an extremal Kerr–Newman black hole background. In particular, using the matched asymptotic expansion method, we analytically solve the null geodesics near the superradiant bound in the form of algebraic equations. For the case that the photon trajectories are limited in the equatorial plane, the shifts in the azimuthal angle and time are obtained. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Black Hole Horizon (dpeaa)DE-He213 Extremal Black Hole (dpeaa)DE-He213 Null Geodesic (dpeaa)DE-He213 Gu, Bao-Min verfasserin aut Wang, Yong-Qiang verfasserin aut Liu, Yu-Xiao verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 77(2017), 2 vom: 24. Feb. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:77 year:2017 number:2 day:24 month:02 https://dx.doi.org/10.1140/epjc/s10052-017-4699-7 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 77 2017 2 24 02
allfieldsSound	10.1140/epjc/s10052-017-4699-7 doi (DE-627)SPR008358591 (SPR)s10052-017-4699-7-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Wei, Shao-Wen verfasserin aut Photon emission of extremal Kerr–Newman black holes 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper, we deal with the null geodesics extending from the near-horizon region out to a distant observatory in an extremal Kerr–Newman black hole background. In particular, using the matched asymptotic expansion method, we analytically solve the null geodesics near the superradiant bound in the form of algebraic equations. For the case that the photon trajectories are limited in the equatorial plane, the shifts in the azimuthal angle and time are obtained. Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Black Hole Horizon (dpeaa)DE-He213 Extremal Black Hole (dpeaa)DE-He213 Null Geodesic (dpeaa)DE-He213 Gu, Bao-Min verfasserin aut Wang, Yong-Qiang verfasserin aut Liu, Yu-Xiao verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 77(2017), 2 vom: 24. Feb. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:77 year:2017 number:2 day:24 month:02 https://dx.doi.org/10.1140/epjc/s10052-017-4699-7 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 77 2017 2 24 02
language	English
source	Enthalten in The European physical journal 77(2017), 2 vom: 24. Feb. volume:77 year:2017 number:2 day:24 month:02
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author	Wei, Shao-Wen
spellingShingle	Wei, Shao-Wen ddc 530 bkl 33.50 misc Black Hole misc Black Hole Solution misc Black Hole Horizon misc Extremal Black Hole misc Null Geodesic Photon emission of extremal Kerr–Newman black holes
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topic_title	530 ASE 33.50 bkl Photon emission of extremal Kerr–Newman black holes Black Hole (dpeaa)DE-He213 Black Hole Solution (dpeaa)DE-He213 Black Hole Horizon (dpeaa)DE-He213 Extremal Black Hole (dpeaa)DE-He213 Null Geodesic (dpeaa)DE-He213
topic	ddc 530 bkl 33.50 misc Black Hole misc Black Hole Solution misc Black Hole Horizon misc Extremal Black Hole misc Null Geodesic
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title	Photon emission of extremal Kerr–Newman black holes
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title_full	Photon emission of extremal Kerr–Newman black holes
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title_sort	photon emission of extremal kerr–newman black holes
title_auth	Photon emission of extremal Kerr–Newman black holes
abstract	Abstract In this paper, we deal with the null geodesics extending from the near-horizon region out to a distant observatory in an extremal Kerr–Newman black hole background. In particular, using the matched asymptotic expansion method, we analytically solve the null geodesics near the superradiant bound in the form of algebraic equations. For the case that the photon trajectories are limited in the equatorial plane, the shifts in the azimuthal angle and time are obtained.
abstractGer	Abstract In this paper, we deal with the null geodesics extending from the near-horizon region out to a distant observatory in an extremal Kerr–Newman black hole background. In particular, using the matched asymptotic expansion method, we analytically solve the null geodesics near the superradiant bound in the form of algebraic equations. For the case that the photon trajectories are limited in the equatorial plane, the shifts in the azimuthal angle and time are obtained.
abstract_unstemmed	Abstract In this paper, we deal with the null geodesics extending from the near-horizon region out to a distant observatory in an extremal Kerr–Newman black hole background. In particular, using the matched asymptotic expansion method, we analytically solve the null geodesics near the superradiant bound in the form of algebraic equations. For the case that the photon trajectories are limited in the equatorial plane, the shifts in the azimuthal angle and time are obtained.
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title_short	Photon emission of extremal Kerr–Newman black holes
url	https://dx.doi.org/10.1140/epjc/s10052-017-4699-7
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author2	Gu, Bao-Min Wang, Yong-Qiang Liu, Yu-Xiao
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up_date	2024-07-03T19:55:34.059Z
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In particular, using the matched asymptotic expansion method, we analytically solve the null geodesics near the superradiant bound in the form of algebraic equations. 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Photon emission of extremal Kerr–Newman black holes

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