Plasma magnetosphere of slowly rotating magnetized neutron stars in modified gravity

This study explores the electromagnetic properties of slowly rotating magnetized neutron stars within Modified Gravity (MOG), focusing on their plasma magnetospheres. Building on vacuum solutions of Maxwell's equations by Deutsch and Rezzolla, it incorporates plasma effects as per Goldreich and Julian, analyzing charge-separated plasma and electric field amplification.

Publication Details

Journal: Ilmiy axborotnoma/Scientific Journal of Samarkand University
Published: 2025-06-01
DOI: https://doi.org/10.59251/2181-3973.2025.v1.138.1.3445
Primary Topic: Pulsars and Gravitational Waves Research
Type: article
Field-Weighted Citation Impact: 0.00

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article

Plasma magnetosphere of slowly rotating magnetized neutron stars in modified gravity

Jun 1, 2025

Ilmiy axborotnoma/Scientific Journal of Samarkand University

Pulsars and Gravitational Waves Research

article

Plasma magnetosphere of slowly rotating magnetized neutron stars in modified gravity

June 1, 2025article en

Abstract

Ilmiy axborotnoma/Scientific Journal of Samarkand UniversityVol. 1(3)

Openalex Percentile: Top 50%

Pulsars and Gravitational Waves Research

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Plasma magnetosphere of slowly rotating magnetized neutron stars in modified gravity · Ilmiy axborotnoma/Scientific Journal of Samarkand University (2025) | TGRS Research Map | TGRS