Continued Gravitational Collapse for Newtonian Stars

Yan Guo, Mahir Hadzic, Juhi Jang

The classical model of an isolated selfrgavitating gaseous star is given by the Euler-Poisson system with a polytropic pressure law $P(\rho )={\rho }^{\gamma }$, $\gamma >1$. For any $1<\gamma <\frac{4}{3}$, we con…