Moller Energy for an Exterior Metric of Relativistic Stars
Document Type
Conference Proceeding
Publication Date
1-1-2021
Abstract
In this paper, we firstly calculate the Komar mass and energy distribution regarding a given exterior space-time of relativistic stars in scalar-Gauss-Bonnet gravity by utilizing Moller’s prescription, which is not restricted by quasi-Cartesian coordinates. The result we get by utilizing Moller’s energy-momentum complex depends on mass parameter of space-time and is equal to Komar mass when r→ ∞, i.e. lim r→∞EMoller= EKomar= M.
Publication Title
Advances in Intelligent Systems and Computing
First Page Number
103
Last Page Number
111
DOI
10.1007/978-981-15-8061-1_9
Recommended Citation
Liwei, Wang, "Moller Energy for an Exterior Metric of Relativistic Stars" (2021). Kean Publications. 1108.
https://digitalcommons.kean.edu/keanpublications/1108
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