J 2021

General relativistic effects in neutron star electrodynamics

TURIMOV, Bobur, Zdeněk STUCHLÍK, Javlon RAYIMBAYEV and Ahmadjon ABDUJABBAROV

Basic information

Original name

General relativistic effects in neutron star electrodynamics

Authors

TURIMOV, Bobur (860 Uzbekistan, belonging to the institution), Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution), Javlon RAYIMBAYEV and Ahmadjon ABDUJABBAROV

Edition

Physical Review D, College Park (USA), American Physical Society, 2021, 2470-0010

Other information

Language

English

Type of outcome

Článek v odborném periodiku

Field of Study

10308 Astronomy

Country of publisher

United States of America

Confidentiality degree

není předmětem státního či obchodního tajemství

References:

RIV identification code

RIV/47813059:19630/21:A0000137

Organization unit

Institute of physics in Opava

UT WoS

000661821000007

Keywords in English

MAGNETIC-FIELD EVOLUTION;SOFT GAMMA-REPEATERS;ELECTROMAGNETIC-FIELDS;SPIN-DOWN;EQUATIONS;EXTERIOR;EMISSION;PULSARS;MODEL

Tags

International impact, Reviewed
Změněno: 7/2/2022 13:03, Mgr. Pavlína Jalůvková

Abstract

V originále

The paper explores general relativistic (GR) effects in electromagnetic fields of the rotating neutron star. The star has been assumed as a perfect conductor with infinity electric conductivity, i.e., sigma -> infinity. The analytical form of general relativistic Maxwell's equations for the electromagnetic fields has been derived in the presence of gravity. It is shown that six components of the electromagnetic fields can be expressed in terms of two profile functions. It has been shown that the Lense-Thirring term plays an important role in the generation of the multipole electromagnetic fields. We obtain that the rotation of the quadrupole magnetic field can create the dipole electric field. Moreover, we have also shown that GR effects are reasonably large for the highest order of electromagnetic multipole. Finally, as a test of our results, we investigate the effect of the Lense-Thirring term on the luminosity of magnetodipolar radiations.