The second Maxwell’s relativistic equations of a rapidaly rotating neutron star, based on ZAMO framework (zero angular momentum observers)

The second Maxwell’s relativistic equations of a rapidaly rotating neutron star, based on ZAMO framework (Zero Angular Momentum Observers) has been formulated. The formulations obtained were epresented by differential equations in the radial, polar, and azimuthal components. The ZAMO basis is implem...

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Main Authors: Atsnaita Yasrina, Nugroho Adi Pramono, Eny Latifah, Hari Wisodo
Format: Article
Language:English
Published: Universitas Sebelas Maret 2017-03-01
Series:Journal of Physics: Theories and Applications
Subjects:
Online Access:https://jurnal.uns.ac.id/jphystheor-appl/article/view/4702
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author Atsnaita Yasrina
Nugroho Adi Pramono
Eny Latifah
Hari Wisodo
author_facet Atsnaita Yasrina
Nugroho Adi Pramono
Eny Latifah
Hari Wisodo
author_sort Atsnaita Yasrina
collection DOAJ
description The second Maxwell’s relativistic equations of a rapidaly rotating neutron star, based on ZAMO framework (Zero Angular Momentum Observers) has been formulated. The formulations obtained were epresented by differential equations in the radial, polar, and azimuthal components. The ZAMO basis is implemented because the neutron star reviewed as a rotating star. The second Maxwell’s equation is important to use as one of the fundamental equations to formulate relativistic magnetic fields dynamics of the neutron stars that rotate rapidly.
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spelling doaj.art-72fdc0da03c54b48ba199ad0b65353512022-12-22T00:31:11ZengUniversitas Sebelas MaretJournal of Physics: Theories and Applications2549-73162549-73242017-03-0111132010.20961/jphystheor-appl.v1i1.47023950The second Maxwell’s relativistic equations of a rapidaly rotating neutron star, based on ZAMO framework (zero angular momentum observers)Atsnaita Yasrina0Nugroho Adi Pramono1Eny Latifah2Hari Wisodo3Jurusan Fisika, FMIPA, Universitas Negeri Malang, Jl. Semarang No. 5, MalangJurusan Fisika, FMIPA, Universitas Negeri Malang, Jl. Semarang No. 5, MalangJurusan Fisika, FMIPA, Universitas Negeri Malang, Jl. Semarang No. 5, MalangJurusan Fisika, FMIPA, Universitas Negeri Malang, Jl. Semarang No. 5, MalangThe second Maxwell’s relativistic equations of a rapidaly rotating neutron star, based on ZAMO framework (Zero Angular Momentum Observers) has been formulated. The formulations obtained were epresented by differential equations in the radial, polar, and azimuthal components. The ZAMO basis is implemented because the neutron star reviewed as a rotating star. The second Maxwell’s equation is important to use as one of the fundamental equations to formulate relativistic magnetic fields dynamics of the neutron stars that rotate rapidly.https://jurnal.uns.ac.id/jphystheor-appl/article/view/4702the second maxwell’s equationneutron starfast rotationzamo
spellingShingle Atsnaita Yasrina
Nugroho Adi Pramono
Eny Latifah
Hari Wisodo
The second Maxwell’s relativistic equations of a rapidaly rotating neutron star, based on ZAMO framework (zero angular momentum observers)
Journal of Physics: Theories and Applications
the second maxwell’s equation
neutron star
fast rotation
zamo
title The second Maxwell’s relativistic equations of a rapidaly rotating neutron star, based on ZAMO framework (zero angular momentum observers)
title_full The second Maxwell’s relativistic equations of a rapidaly rotating neutron star, based on ZAMO framework (zero angular momentum observers)
title_fullStr The second Maxwell’s relativistic equations of a rapidaly rotating neutron star, based on ZAMO framework (zero angular momentum observers)
title_full_unstemmed The second Maxwell’s relativistic equations of a rapidaly rotating neutron star, based on ZAMO framework (zero angular momentum observers)
title_short The second Maxwell’s relativistic equations of a rapidaly rotating neutron star, based on ZAMO framework (zero angular momentum observers)
title_sort second maxwell s relativistic equations of a rapidaly rotating neutron star based on zamo framework zero angular momentum observers
topic the second maxwell’s equation
neutron star
fast rotation
zamo
url https://jurnal.uns.ac.id/jphystheor-appl/article/view/4702
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