Electromagnetic field around the magnetized and idealized neutron star

被引：0

作者：

Turimov, Bobur ^{[1
,2
,3
]}

Atamurotov, Farruh ^{[4
,5
,6
]}

机构：

[1] New Uzbekistan Univ, Mustaqillik Ave 54, Tashkent 100007, Uzbekistan

[2] Cent Asian Univ, Milliy Bog St 264, Tashkent 111221, Uzbekistan

[3] Ulugh Beg Astron Inst, Astron St 33, Tashkent 100052, Uzbekistan

[4] Inha Univ Tashkent, Ziyolilar 9, Tashkent 100170, Uzbekistan

[5] Natl Univ Uzbekistan, Tashkent 100174, Uzbekistan

[6] Tashkent State Tech Univ, Tashkent 100095, Uzbekistan

来源：

INTERNATIONAL JOURNAL OF GEOMETRIC METHODS IN MODERN PHYSICS | 2023年

关键词：

Magnetized neutron star; electromagnetic fields; radiation power; TELEPARALLEL THEORY EQUIVALENT; RELATIVISTIC STAR; ENERGY; EVOLUTION; EXTERIOR; MOMENTUM; DILATON;

D O I：

10.1142/S0219887823502328

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The electrodynamics of the highly magnetized and spherical symmetric neutron star within the framework of special relativity has been investigated. It is assumed that the neutron star is isolated and consists of highly conducting matter. Explicit demonstrations were made regarding the multipole solutions for both axially symmetric and non-axially symmetric electromagnetic fields surrounding the neutron star. It was observed that the axially symmetric solutions are independent of time, whereas the non-axially symmetric solutions are time-dependent. Additionally, wave-like solutions for the electromagnetic field in TE and TM modes were derived.

引用

页数：12