Abstract
The threshold for pion condensation in neutron star matter is estimated on the basis of a sufficiently realistic treatment of effective forces. It turns out that the short range repulsion of the nucleon-nucleon force raises considerably the density at which the pion condensed phase can occur.
Original language | English |
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Pages (from-to) | 297-301 |
Number of pages | 5 |
Journal | Physics Letters B |
Volume | 48 |
Issue number | 4 |
DOIs | |
State | Published - 18 Feb 1974 |
Externally published | Yes |