Core-envelope compact-star models with envelope anisotropy accumulate up to 10^50 erg of stress energy that may trigger starquakes comparable in scale to GRBs.
K Bisht and N Pant
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Relativistic stellar modeling with perfect fluid core and anisotropic envelope fluid
Core-envelope compact-star models with envelope anisotropy accumulate up to 10^50 erg of stress energy that may trigger starquakes comparable in scale to GRBs.