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pro vyhledávání: '"Xi, Yu"'
Autor:
Zhong-Xi Yu, Hao Wei
Publikováno v:
Journal of Cosmology and Astroparticle Physics. 2021:011
As is well known, there are various mass limits for compact stars. For example, the maximum mass for non-rotating white dwarfs is given by the famous Chandrasekhar limit about $1.4 M_\odot$ (solar masses). Although the mass limit for neutron stars is