Solution for the relativistic magnetic field dynamics equation of neutron stars as magnetized conductors has been formulated by assuming the magnetic field as magnetized, rapidly rotating conductor, and accreting in Zero Angular Momentum Observers (ZAMO) frame. The magnetic field in a neutron star is assumed to be bipolar. The relativistic magnetic field dynamics equation of neutron stars as magnetized is obtained by formulating the contravariant tensor, the current density of four, and the relativistic second Maxwell equation. The form of the equation is the differential equation with the solution being the radial, polar, azimuth, and time functions. The equation obtained has the same pattern as a slow-rotating neutron star. But if it is assumed that the neutron star does not perform accretion, then the star's rotation speed affects the magnetic field by showing the presence of polar, azimuthal, and time components.
Skip Nav Destination
Article navigation
18 May 2020
CONFERENCE ON THEORETICAL PHYSICS AND NONLINEAR PHENOMENA (CTPNP) 2019: Excursion from Vacuum to Condensed Matter
9–10 October 2019
Malang, Indonesia
Research Article|
May 18 2020
Solution for the relativistic magnetic field dynamics equation of neutron stars as magnetized, accreting, and rapidly rotating conductors in zero angular momentum observers (ZAMO) frame
A. Yasrina;
A. Yasrina
a)
1
Department of Physics, Faculty of Mathematics and Natural Sciences, Universitas Negeri Malang
, Jl. Semarang 5, Malang 65145, Indonesia
a)Corresponding author: [email protected]
Search for other works by this author on:
D. Andra;
D. Andra
2
Departmen of Physiscs, Faculty of Matematics and Natural Sciences, Universitas Negeri Lampung
, Jl. Prof. Soemantri Brodjonegoro No.1 Gedong Meneng Rajabasa, Bandar Lampung 35144 Indonesia
Search for other works by this author on:
N. Widianingrum;
N. Widianingrum
1
Department of Physics, Faculty of Mathematics and Natural Sciences, Universitas Negeri Malang
, Jl. Semarang 5, Malang 65145, Indonesia
Search for other works by this author on:
E. Latifah;
E. Latifah
1
Department of Physics, Faculty of Mathematics and Natural Sciences, Universitas Negeri Malang
, Jl. Semarang 5, Malang 65145, Indonesia
Search for other works by this author on:
N. A. Pramono
N. A. Pramono
1
Department of Physics, Faculty of Mathematics and Natural Sciences, Universitas Negeri Malang
, Jl. Semarang 5, Malang 65145, Indonesia
Search for other works by this author on:
a)Corresponding author: [email protected]
AIP Conf. Proc. 2234, 040029 (2020)
Citation
A. Yasrina, D. Andra, N. Widianingrum, E. Latifah, N. A. Pramono; Solution for the relativistic magnetic field dynamics equation of neutron stars as magnetized, accreting, and rapidly rotating conductors in zero angular momentum observers (ZAMO) frame. AIP Conf. Proc. 18 May 2020; 2234 (1): 040029. https://doi.org/10.1063/5.0008336
Download citation file:
Citing articles via
Inkjet- and flextrail-printing of silicon polymer-based inks for local passivating contacts
Zohreh Kiaee, Andreas Lösel, et al.
Design of a 100 MW solar power plant on wetland in Bangladesh
Apu Kowsar, Sumon Chandra Debnath, et al.
Production and characterization of corncob biochar for agricultural use
Praphatsorn Rattanaphaiboon, Nigran Homdoung, et al.
Related Content
Theoretical study of Maxwell’s solution of magnetic field dynamics around neutron star in the ZAMO (zero angular momentum observers) frame: Accreting and rapidly rotating cases
AIP Conf. Proc. (August 2020)
Relativistic mass rates of accreted matter with accretion discs in the equatorial plane of slowly rotating neutron stars
AIP Conf. Proc. (May 2023)
Formulating the equation of relativistic mass accretion rate for extreme Kerr black holes with accretion disk on the equatorial plane
AIP Conf. Proc. (May 2020)
Parametric mechanism of the rotation energy pumping by a relativistic plasma
Phys. Plasmas (June 2005)
Electron-positron outflow from black holes and the formation of winds
AIP Conference Proceedings (March 2001)