Abstract
The classical model of an isolated selfgravitating gaseous star is given by the Euler–Poisson system with a polytropic pressure law P(ρ) = ργ, γ> 1. For any 1
Cite
CITATION STYLE
APA
Guo, Y., Hadžić, M., & Jang, J. (2021). Continued Gravitational Collapse for Newtonian Stars. Archive for Rational Mechanics and Analysis, 239(1), 431–552. https://doi.org/10.1007/s00205-020-01580-w
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