An effective field theory for neutron stars with many‐body forces, strong ∑– repulsion, and K– and $\bar K^0$ condensation

Publisher： John Wiley & Sons Inc

E-ISSN： 1521-3994|336|8‐9|880-884

ISSN： 0004-6337

Source： ASTRONOMISCHE NACHRICHTEN, Vol.336, Iss.8‐9, 2015-11, pp. : 880-884

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