Relativistic phase transition

Details Relativistic phase transition Relativistic phase transition

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974zhetf..67.1263k&link_type=abstract

Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki, vol. 67, Oct. 1974, p. 1263-1275. In Russian.

Astronomy and Astrophysics

Astrophysics

45

Astronomical Models, Cosmology, Electromagnetic Interactions, Nuclear Transformations, Particle Interactions, Relativistic Theory, Astrophysics, Boson Fields, Energy Transfer, Fermions, Quantum Statistics, Theoretical Physics

Scientific paper

A phase transition theory is developed on the basis of a relativistic scalar model. By considering spontaneous breakdown of symmetry (the masses of vector bosons and fermions are absent in the initial Lagrangian, and are generated by spontaneous breakdown of symmetry), the model forms an integral part of a unified theory of electromagnetic and weak interactions. It is pointed out that in processes involving temperature variations (in particular, in the evolution of a hot universe), energy balance of matter is disturbed by energy transfer from the Bose condensate.

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