Deformation and anisotropic magnetic field effects on neutron star

A. Yanis, Anto Sulaksono

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

We have investigated the deformation and anisotropic magnetic field effects on neutron star by means of the TOV equation. The deformation effect is obtained by modifying the metric tensor and adding a deformation parameter on z-axis star [1], while the effect of magnetic field is obtained by adjusting the energy-momentum tensor for the anisotropic magnetic field [2]. Both modifications are implemented in the TOV equation. The final result of this equation can explain the effect of deformation and the magnetic field on the neutron star's profile.

Original languageEnglish
Title of host publicationProceedings of the 3rd International Symposium on Current Progress in Mathematics and Sciences 2017, ISCPMS 2017
EditorsRatna Yuniati, Terry Mart, Ivandini T. Anggraningrum, Djoko Triyono, Kiki A. Sugeng
PublisherAmerican Institute of Physics Inc.
ISBN (Electronic)9780735417410
DOIs
Publication statusPublished - 22 Oct 2018
Event3rd International Symposium on Current Progress in Mathematics and Sciences 2017, ISCPMS 2017 - Bali, Indonesia
Duration: 26 Jul 201727 Jul 2017

Publication series

NameAIP Conference Proceedings
Volume2023
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Conference

Conference3rd International Symposium on Current Progress in Mathematics and Sciences 2017, ISCPMS 2017
CountryIndonesia
CityBali
Period26/07/1727/07/17

Keywords

  • Neutron stars
  • deformation
  • magnetic field

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    Yanis, A., & Sulaksono, A. (2018). Deformation and anisotropic magnetic field effects on neutron star. In R. Yuniati, T. Mart, I. T. Anggraningrum, D. Triyono, & K. A. Sugeng (Eds.), Proceedings of the 3rd International Symposium on Current Progress in Mathematics and Sciences 2017, ISCPMS 2017 [020009] (AIP Conference Proceedings; Vol. 2023). American Institute of Physics Inc.. https://doi.org/10.1063/1.5064006