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In this paper we used the theory of adiabatic radial oscillations developed by Chandrasekhar to study the conditions for dynamical stability of constant energy-density stars, or Schwarzschild stars, in the… Click to show full abstract
In this paper we used the theory of adiabatic radial oscillations developed by Chandrasekhar to study the conditions for dynamical stability of constant energy-density stars, or Schwarzschild stars, in the unstudied ultra compact regime beyond the Buchdahl limit, that is, for configurations with radius $R$ in the range $R_{\rm S}
Keywords:
ultra compact;
beyond buchdahl;
buchdahl limit;
schwarzschild stars;
stability
Journal Title: Classical and Quantum Gravity
Year Published: 2019
Link to full text (if available)
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Journal Title: Classical and Quantum Gravity
Year Published: 2019
Link to full text (if available)
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recommendations!