Abnormal neutron stars

Details Abnormal neutron stars Abnormal neutron stars

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975phlb...55..178k&link_type=abstract

Physics Letters B, Volume 55, Issue 2, p. 178-182.

Physics

7

Scientific paper

Quasi-classical field theory is used to predict abnormal behaviour of neutron matter in a model with neutrons, scalar mesons and vector mesons. We predict two stable families of neutron stars, a conventional one and an unconventional one with surface density in excess of 1015g cm-3, roughly.
On leave from Institutionen för Fysik, Åbo Akademi, Åbo, Finland.

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