Shock formation and shock structure in the cosmological radiative ERA

Details Shock formation and shock structure in the cosmological radiative ERA Shock formation and shock structure in the cosmological radiative ERA

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979nciml..26..121a&link_type=abstract

Nuovo Cimento, Lettere, Serie 2, vol. 26, Sept. 22, 1979, p. 121-124.

Mathematics

Logic

Cosmology, Radiative Transfer, Shock Wave Generators, Shock Wave Profiles, Thomson Scattering, Acoustic Propagation, Astronomical Models, Energy Transfer, Momentum Transfer

Scientific paper

The shock structure resulting from dissipative processes that could operate in the cosmological radiative era is examined. Acoustic-radiative waves, where matter and radiation are perturbed in a definite ratio, are considered. A propagation equation is obtained for these waves, and its steady-state solutions are shown to describe the shock structure of interest.

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