Key points are not available for this paper at this time.
A field-theoretic model is constructed which is asymptotically free for all temperatures and which possesses a phase transition in which masses are dynamically generated. The critical temperature above which the particle masses vanish is calculated in terms of the zero-temperature fermion mass. Our results may be of interest not only in theories of the early universe but also in the study of the formative stages of neutron stars.
Harrington et al. (Sat,) studied this question.