The value for it is thought to be around 1.4 solar masses or 2.96x1030 [2.96 times 10 to the 30th] kilograms, and no white dwarf can be stabilized by degeneracy pressure beyond it.
In 1987, Lieb and Yau proposed an analog of this for boson-composed stars such as axion stars, using a Hartree-type equation instead of the namesake's. As a consequence of it, main sequence stars larger than eight solar masses must become neutron stars or black holes. The value for it is thought to be around 1.4 solar masses or 2.96x1030 [2.96 times 10 to the 30th] kilograms, and no white dwarf can be stabilized by degeneracy pressure beyond it. For 10 points, identify this mass limit named for an Indian astrophysicist.
In 1987, Lieb and Yau proposed an analog of this for boson-composed stars such as axion stars, using a Hartree-type equation instead of the namesake's.
Schoenberg-{Chandrasekhar} limit [accept {Chandrasekhar} after “{limit}”]