Plasma Waves Around Massive Stars in (3+1)-General Relativistic Magnetohydrodynamics

被引：0

作者：

Hassan Shokrgozar Arani

Salman Abarghouei Nejad

Mahtab Talaei Faghloo

Reza Ramezani Arani

机构：

[1] University of Kashan,Department of Physics

[2] Universidade Estadual Paulista (IFT-UNESP),Instituto de Física Teórica

来源：

Brazilian Journal of Physics | 2022年 / 52卷

关键词：

Plasma waves propagation equations; Plasma waves dispersion equations; TPM (Thorne-Price-Macdonald) (3+1)-general relativistic magnetohydrodynamics; WKB approximation; One-fluid plasma equations;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

In this article, the propagation of plasma waves around rotating and non-rotating stars is studied in a TPM (Thorne-Price-Macdonald) (3+1)-general relativistic magnetohydrodynamics (GRMHD) formalism. For more simplicity, the plasma around the atmosphere of the stars is considered to be stationary. Using WKB approximation, we derive the local longitudinal and transverse dispersion relations and compare them to the special relativistic congener.

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