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What prevents gravitational collapse in string theory?

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arxiv 1609.05222 v1 pith:3RR7XG3U submitted 2016-09-16 hep-th gr-qc

classification hep-thgr-qc
keywords collapsematterblackdimensionextragravitymicrostatesstring
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abstract

It is conventionally believed that if a ball of matter of mass $M$ has a radius close to $2GM$ then it must collapse to a black hole. But string theory microstates (fuzzballs) have no horizon or singularity, and they do {\it not} collapse. We consider two simple examples from classical gravity to illustrate how this violation of our intuition happens. In each case the `matter' arises from an extra compact dimension, but the topology of this extra dimension is not trivial. The pressure and density of this matter diverge at various points, but this is only an artifact of dimensional reduction; thus we bypass results like Buchadahl's theorem. Such microstates give the entropy of black holes, so these topologically nontrivial constructions dominate the state space of quantum gravity.

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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. Space cannot stretch too {\it fast}

    hep-th 2025-05 reject novelty 5.0 of 10

    The essay proposes that fast stretching of space releases energy stored in vacuum entanglements left by virtual black hole microstates, resolving the information paradox and yielding dark energy.

  2. Blackish Holes

    hep-th 2024-11 conditional novelty 5.0 of 10

    Placing a Dirichlet wall just outside the BTZ horizon produces a dense spectrum of normal modes that, in the continuum limit, yields a thermal two-point function at the Hawking temperature.

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