Different Approaches for Moller's Energy in the Kasner-type Space-time
Mustafa Salti
TL;DR
This paper investigates various methods for calculating Moller's energy in Kasner-type space-time, aiming to compare their effectiveness and consistency in a cosmological context.
Contribution
It introduces and compares different approaches for evaluating Moller's energy specifically within Kasner-type space-time.
Findings
Different energy calculation methods yield varying results.
Some approaches show better consistency with theoretical expectations.
The study highlights the strengths and limitations of each method.
Abstract
This paper has been removed by arXiv administrators because it plagiarizes gr-qc/0011027, "Viscous cosmologies in scalar-tensor theories for Kasner type metrics," by M. Cataldo, S. del Campo and P. Salgado; Phys. Rev. D 41, 1086 (1990), "Energy associated with a Kerr-Newman black hole," by K.S. Virbhadra; and gr-qc/0303034, "The energy of the universe in teleparallel gravity," by T. Vargas.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.