http://arxiv.org/abs/1402.3691
We revise Gamow’s calculation of the neutron star critical mass \cite{gamow} regarding calculational and conceptual aspects and discuss the implications on its importance for the history of astrophysics. We compare his approach to other early and modern approaches to the problem.
H. Ludwig and R. Ruffini
Tue, 18 Feb 14
45/72
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