Many Aspects of Magnetic Fields in Neutron Stars

In this work, we explore different aspects in which strong magnetic fields play a role in the composition, structure and evolution of neutron stars. More specifically, we discuss (i) how strong magnetic fields change the equation of state of dense matter, alter its composition, and create anisotropi...
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Autor*in:	Rodrigo Negreiros [verfasserIn] Cristian Bernal [verfasserIn] Veronica Dexheimer [verfasserIn] Orlenys Troconis [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2018

Schlagwörter:	neutron stars stellar magnetic field stellar structure stellar evolution

Übergeordnetes Werk:	In: Universe - MDPI AG, 2015, 4(2018), 3, p 43
Übergeordnetes Werk:	volume:4 ; year:2018 ; number:3, p 43

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3390/universe4030043

Katalog-ID:	DOAJ029769752

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allfields	10.3390/universe4030043 doi (DE-627)DOAJ029769752 (DE-599)DOAJ3281c25d992f4bdcb07082661f2374af DE-627 ger DE-627 rakwb eng QC793-793.5 Rodrigo Negreiros verfasserin aut Many Aspects of Magnetic Fields in Neutron Stars 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In this work, we explore different aspects in which strong magnetic fields play a role in the composition, structure and evolution of neutron stars. More specifically, we discuss (i) how strong magnetic fields change the equation of state of dense matter, alter its composition, and create anisotropies, (ii) how they change the structure of neutron stars (such mass and radius) and the formalism necessary to calculate those changes, and (iii) how they can affect neutron stars’ evolution. In particular, we focus on how a time-dependent magnetic field modifies the cooling of a special group known as X-ray dim neutron stars. neutron stars stellar magnetic field stellar structure stellar evolution Elementary particle physics Cristian Bernal verfasserin aut Veronica Dexheimer verfasserin aut Orlenys Troconis verfasserin aut In Universe MDPI AG, 2015 4(2018), 3, p 43 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:4 year:2018 number:3, p 43 https://doi.org/10.3390/universe4030043 kostenfrei https://doaj.org/article/3281c25d992f4bdcb07082661f2374af kostenfrei http://www.mdpi.com/2218-1997/4/3/43 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 AR 4 2018 3, p 43
spelling	10.3390/universe4030043 doi (DE-627)DOAJ029769752 (DE-599)DOAJ3281c25d992f4bdcb07082661f2374af DE-627 ger DE-627 rakwb eng QC793-793.5 Rodrigo Negreiros verfasserin aut Many Aspects of Magnetic Fields in Neutron Stars 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In this work, we explore different aspects in which strong magnetic fields play a role in the composition, structure and evolution of neutron stars. More specifically, we discuss (i) how strong magnetic fields change the equation of state of dense matter, alter its composition, and create anisotropies, (ii) how they change the structure of neutron stars (such mass and radius) and the formalism necessary to calculate those changes, and (iii) how they can affect neutron stars’ evolution. In particular, we focus on how a time-dependent magnetic field modifies the cooling of a special group known as X-ray dim neutron stars. neutron stars stellar magnetic field stellar structure stellar evolution Elementary particle physics Cristian Bernal verfasserin aut Veronica Dexheimer verfasserin aut Orlenys Troconis verfasserin aut In Universe MDPI AG, 2015 4(2018), 3, p 43 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:4 year:2018 number:3, p 43 https://doi.org/10.3390/universe4030043 kostenfrei https://doaj.org/article/3281c25d992f4bdcb07082661f2374af kostenfrei http://www.mdpi.com/2218-1997/4/3/43 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 AR 4 2018 3, p 43
allfields_unstemmed	10.3390/universe4030043 doi (DE-627)DOAJ029769752 (DE-599)DOAJ3281c25d992f4bdcb07082661f2374af DE-627 ger DE-627 rakwb eng QC793-793.5 Rodrigo Negreiros verfasserin aut Many Aspects of Magnetic Fields in Neutron Stars 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In this work, we explore different aspects in which strong magnetic fields play a role in the composition, structure and evolution of neutron stars. More specifically, we discuss (i) how strong magnetic fields change the equation of state of dense matter, alter its composition, and create anisotropies, (ii) how they change the structure of neutron stars (such mass and radius) and the formalism necessary to calculate those changes, and (iii) how they can affect neutron stars’ evolution. In particular, we focus on how a time-dependent magnetic field modifies the cooling of a special group known as X-ray dim neutron stars. neutron stars stellar magnetic field stellar structure stellar evolution Elementary particle physics Cristian Bernal verfasserin aut Veronica Dexheimer verfasserin aut Orlenys Troconis verfasserin aut In Universe MDPI AG, 2015 4(2018), 3, p 43 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:4 year:2018 number:3, p 43 https://doi.org/10.3390/universe4030043 kostenfrei https://doaj.org/article/3281c25d992f4bdcb07082661f2374af kostenfrei http://www.mdpi.com/2218-1997/4/3/43 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 AR 4 2018 3, p 43
allfieldsGer	10.3390/universe4030043 doi (DE-627)DOAJ029769752 (DE-599)DOAJ3281c25d992f4bdcb07082661f2374af DE-627 ger DE-627 rakwb eng QC793-793.5 Rodrigo Negreiros verfasserin aut Many Aspects of Magnetic Fields in Neutron Stars 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In this work, we explore different aspects in which strong magnetic fields play a role in the composition, structure and evolution of neutron stars. More specifically, we discuss (i) how strong magnetic fields change the equation of state of dense matter, alter its composition, and create anisotropies, (ii) how they change the structure of neutron stars (such mass and radius) and the formalism necessary to calculate those changes, and (iii) how they can affect neutron stars’ evolution. In particular, we focus on how a time-dependent magnetic field modifies the cooling of a special group known as X-ray dim neutron stars. neutron stars stellar magnetic field stellar structure stellar evolution Elementary particle physics Cristian Bernal verfasserin aut Veronica Dexheimer verfasserin aut Orlenys Troconis verfasserin aut In Universe MDPI AG, 2015 4(2018), 3, p 43 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:4 year:2018 number:3, p 43 https://doi.org/10.3390/universe4030043 kostenfrei https://doaj.org/article/3281c25d992f4bdcb07082661f2374af kostenfrei http://www.mdpi.com/2218-1997/4/3/43 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 AR 4 2018 3, p 43
allfieldsSound	10.3390/universe4030043 doi (DE-627)DOAJ029769752 (DE-599)DOAJ3281c25d992f4bdcb07082661f2374af DE-627 ger DE-627 rakwb eng QC793-793.5 Rodrigo Negreiros verfasserin aut Many Aspects of Magnetic Fields in Neutron Stars 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In this work, we explore different aspects in which strong magnetic fields play a role in the composition, structure and evolution of neutron stars. More specifically, we discuss (i) how strong magnetic fields change the equation of state of dense matter, alter its composition, and create anisotropies, (ii) how they change the structure of neutron stars (such mass and radius) and the formalism necessary to calculate those changes, and (iii) how they can affect neutron stars’ evolution. In particular, we focus on how a time-dependent magnetic field modifies the cooling of a special group known as X-ray dim neutron stars. neutron stars stellar magnetic field stellar structure stellar evolution Elementary particle physics Cristian Bernal verfasserin aut Veronica Dexheimer verfasserin aut Orlenys Troconis verfasserin aut In Universe MDPI AG, 2015 4(2018), 3, p 43 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:4 year:2018 number:3, p 43 https://doi.org/10.3390/universe4030043 kostenfrei https://doaj.org/article/3281c25d992f4bdcb07082661f2374af kostenfrei http://www.mdpi.com/2218-1997/4/3/43 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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 AR 4 2018 3, p 43
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institution	findex.gbv.de
topic_facet	neutron stars stellar magnetic field stellar structure stellar evolution Elementary particle physics
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authorswithroles_txt_mv	Rodrigo Negreiros @@aut@@ Cristian Bernal @@aut@@ Veronica Dexheimer @@aut@@ Orlenys Troconis @@aut@@
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callnumber-first	Q - Science
author	Rodrigo Negreiros
spellingShingle	Rodrigo Negreiros misc QC793-793.5 misc neutron stars misc stellar magnetic field misc stellar structure misc stellar evolution misc Elementary particle physics Many Aspects of Magnetic Fields in Neutron Stars
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topic_title	QC793-793.5 Many Aspects of Magnetic Fields in Neutron Stars neutron stars stellar magnetic field stellar structure stellar evolution
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title	Many Aspects of Magnetic Fields in Neutron Stars
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title_full	Many Aspects of Magnetic Fields in Neutron Stars
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title_sort	many aspects of magnetic fields in neutron stars
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title_auth	Many Aspects of Magnetic Fields in Neutron Stars
abstract	In this work, we explore different aspects in which strong magnetic fields play a role in the composition, structure and evolution of neutron stars. More specifically, we discuss (i) how strong magnetic fields change the equation of state of dense matter, alter its composition, and create anisotropies, (ii) how they change the structure of neutron stars (such mass and radius) and the formalism necessary to calculate those changes, and (iii) how they can affect neutron stars’ evolution. In particular, we focus on how a time-dependent magnetic field modifies the cooling of a special group known as X-ray dim neutron stars.
abstractGer	In this work, we explore different aspects in which strong magnetic fields play a role in the composition, structure and evolution of neutron stars. More specifically, we discuss (i) how strong magnetic fields change the equation of state of dense matter, alter its composition, and create anisotropies, (ii) how they change the structure of neutron stars (such mass and radius) and the formalism necessary to calculate those changes, and (iii) how they can affect neutron stars’ evolution. In particular, we focus on how a time-dependent magnetic field modifies the cooling of a special group known as X-ray dim neutron stars.
abstract_unstemmed	In this work, we explore different aspects in which strong magnetic fields play a role in the composition, structure and evolution of neutron stars. More specifically, we discuss (i) how strong magnetic fields change the equation of state of dense matter, alter its composition, and create anisotropies, (ii) how they change the structure of neutron stars (such mass and radius) and the formalism necessary to calculate those changes, and (iii) how they can affect neutron stars’ evolution. In particular, we focus on how a time-dependent magnetic field modifies the cooling of a special group known as X-ray dim neutron stars.
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title_short	Many Aspects of Magnetic Fields in Neutron Stars
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