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We investigate the possible occurrence of a Bose-Einstein condensed phase ofmatter within neutron stars due to the formation of Cooper pairs among thesuperfluid neutrons. To this end we study the condensation of bosonic particlesunder the influence of both a short-range contact and a long-rangegravitational interaction in the framework of a Hartree-Fock theory. Weconsider a finite-temperature scenario, generalizing existing approaches, andderive macroscopic and astrophysically relevant quantities like a mass limitfor neutron stars.

the european physical journal. d, atomic, molecular and optical physics/the european physical journal. d, atomic, molecular, optical and plasma physics

A theory of finite-temperature Bose-Einstein condensates in neutron stars