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Energy extracted from Hartle-Thorne strange stars

2024/03/01 by Alpha O. Djalo, Djalo, Alpha O., Felipe A. Asenjo +1
Physics and Astronomy · #Astronomy and Astrophysical Research #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #History and Developments in Astronomy #Stellar, planetary, and galactic studies

paper · pdf · doi:10.48550/arxiv.2403.00618

openalex publication_date 2024/03/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

It is discussed how Penrose process can be used in a strange star, described by the Hartle-Thorne metric, to extract its rotational energy. This metric has an ergosphere region that depends only on its angular momentum. It is shown that massive particles with negative energy can exist in this ergosphere, exploring the conditions on the radial distance and on angular momentum for this to occur. It is also calculated the total amount of rotational energy that can be extracted from the strange star, and how these conditions cannot be fulfilled by a star with regular matter.

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