A Simple Dynamical Model for Catastrophe of Homogeneous Material of Star at High Densities

Details A Simple Dynamical Model for Catastrophe of Homogeneous Material of Star at High Densities A Simple Dynamical Model for Catastrophe of Homogeneous Material of Star at High Densities

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pthph..73..284f&link_type=abstract

Progress of Theoretical Physics, Vol. 73, No. 1, pp. 284-287

Physics

1

Scientific paper

When the heating of a star core due to the adiabatic gravitational collapse is not enough, the homogeneous material of a star must undergo a catastrophe analogous to the phase transition. The growth of the structure at the catastrophe is discussed. For low average densities, the characteristic length scale grows as t2/5, while for high densities it grows as t2/3, as a function of time t.

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