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(1) For some purposes it is useful to use an alternative set of functions: f (r) = e2Φ(r), h (r) = 1 1 − 2m(r) r , (2) where Φ(r) is the redshift function, m(r) is the Misner-Sh

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Beyond Buchdahl's limit: bilayered stars and thin-shell configurations

gr-qc · 2024-11-21 · conditional · novelty 6.0

Explicit bilayered and thin-shell GR models show that relaxing monotonic density or isotropy lets compactness approach Bondi's bound or even the black hole limit.

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Beyond Buchdahl's limit: bilayered stars and thin-shell configurations gr-qc · 2024-11-21 · conditional · none · ref 2
Explicit bilayered and thin-shell GR models show that relaxing monotonic density or isotropy lets compactness approach Bondi's bound or even the black hole limit.

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