Gravitational motions of collapse and expansion of spherically symmetrical bodies in general relativity
The general theory of relativity is used to investigate the properties and behaviour of spherically symmetrical masses of perfect fluid. The stability of equilibrium models against adiabatic radial perturbations is investigated, and a new derivation is given of Chandrasekhar's well-known equati...
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Imperial College London
1967
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| Online Access: | https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.622974 |