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Abnormal phase in dense neutron star matter
Authors:Ebbe M. Nyman  
Affiliation:

a Department of Physics, State University of New York at Stony Brook, Stony Brook, New York 11794, USA

b Åbo Akademi, 20500, Åbo 50, Finland

Service de Physique Théorique, Centre d'Etudes Nucléaires de Saclay, BP no. 2, 91190, Gif-sur-Yvette, France

Abstract: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.
Keywords:
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