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Implementing Markov's Limiting Curvature Hypothesis

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arxiv gr-qc/9509059 v1 pith:4LWHPDWF submitted 1995-10-01 gr-qc hep-th

classification gr-qchep-th
keywords curvatureeffectivegravitylimitingactionactionsasymptoticallyclass
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The effective action for gravity at high curvatures is likely to contain higher derivative terms. These corrections may have profound consequences for the singularity structure of space-time and for early Universe cosmology. In this contribution, recent work is reviewed which demonstrates that it is possible to construct a class of effective gravitational actions for which all solutions with sufficient symmetries have limited curvature and are nonsingular. Near the limiting curvature, the coupling between matter and gravity goes to zero and in this sense the theory is asymptotically free.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Neutron stars in 4D Einstein-Gauss-Bonnet gravity

    gr-qc 2024-12 conditional novelty 6.0 of 10

    In 4D Einstein-Gauss-Bonnet gravity, neutron stars turn unstable exactly at their maximum mass, but near the black hole limit some solutions regain stability, suggesting stable black-hole-sized objects.

  2. Regular black holes inspired by quasi-topological gravity

    gr-qc 2024-11 conditional novelty 6.0 of 10

    A new family of 2D dilaton-gravity models produces exact, regular black hole metrics whose curvature obeys a universal scaling law and a linear master equation.

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