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- W4255144717 abstract "Starting with a “relativistic” Schrödinger Hamiltonian for neutral gravitating particles, we prove that as the particle number N → ∞ and the gravitation constant G → 0 we obtain the well known semiclassical theory for the ground state of stars. For fermions; the correct limit is to fix GN 2/3 and the Chandrasekhar formula is obtained. For bosons the correct limit is to fix GN and a Hartree type equation is obtained. In the fermion case we also prove that the semiclassical equation has a unique solution — a fact which had not been established previously." @default.
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- W4255144717 date "1997-01-01" @default.
- W4255144717 modified "2023-10-18" @default.
- W4255144717 title "The Chandrasekhar Theory of Stellar Collapse as the Limit of Quantum Mechanics" @default.
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- W4255144717 doi "https://doi.org/10.1007/978-3-662-03436-1_40" @default.
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