Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983acaps...2..285w&link_type=abstract
(Acta Astrophysica Sinica, vol. 2, no. 4, 1982, p. 285-290) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 7, March 1
Astronomy and Astrophysics
Astrophysics
Neutron Stars, Nucleons, Particle Theory, Stellar Models, Inhomogeneity, Neutrons, Protons
Scientific paper
An inhomogeneous model of a neutron star made of abnormal state neutrons and protons is analyzed. Compared to a homogeneous model, the maximum mass is slightly smaller. From the equation of state, values for the nucleon number density at P = O are found which are greater than the value at which normal neutron stars must consist entirely of abnormal neutrons (including abnormal protons and electrons); they cannot consist of a shell of normal neutrons with a core of abnormal neutrons. Any transformation of a normal neutron star must be global and not local, offering a possible mechanism for an explosive release of energy.
Chu Yan-Yi
Lu Tan
Qu Qin-Yue
Wang Zhen-Ru
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