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In this paper we calculate the energy distribution E(r) associated with a static spherically symmetric non-singular phantom black hole metric in Einstein's prescription in general relativity. As required for Einstein energy-momentum complex, we perfo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e186f3349c0fc6bf6ddb320ee83fcbdd
http://arxiv.org/abs/1409.6513
http://arxiv.org/abs/1409.6513
