Abnormal phase in dense neutron star matter

Details Abnormal phase in dense neutron star matter Abnormal phase in dense neutron star matter

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977nupha.290..493n&link_type=abstract

Nuclear Physics A, Volume 290, Issue 2, p. 493-500.

Physics

Nuclear Physics

3

Scientific paper

The possibility that neutron stars may possess an ``abnormal'' central region of the Lee-Wick type is discussed. It is found that when the abnormal equation of state includes quantum corrections and short-range repulsion as required in normal nuclear matter, the gravitational pressure in stable neutron stars is insufficient to induce a phase transition to abnormal matter.

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