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Fast Radio Bursts and White Hole Signals

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arxiv 1409.4031 v3 pith:2VNTQFWN submitted 2014-09-14 gr-qc astro-ph.COastro-ph.HE

Aurélien Barrau , Carlo Rovelli , Francesca Vidotto This is my paper · ORCID
classification gr-qcastro-ph.COastro-ph.HE
keywords holeburstsexplodingfastradiosignalssizewhite
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We estimate the size of a primordial black hole exploding today via a white hole transition, and the power in the resulting explosion, using a simple model. We point out that Fast Radio Bursts, strong signals with millisecond duration, probably extragalactic and having unknown source, have wavelength not far from the expected size of the exploding hole. We also discuss the possible higher energy components of the signal.

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Cited by 3 Pith papers

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

  1. Semiclassical Black Hole-White Hole transitions: an analytical treatment

    gr-qc 2026-08 conditional novelty 6.0 of 10

    The |in>-vacuum stress-energy in 2D collapse models amplifies at the inner horizon and can flip the ingoing null expansion, turning a trapped region into an anti-trapped one.

  2. Observable thin accretion disk around a self-dual black hole in loop quantum gravity

    gr-qc 2025-09 conditional novelty 3.0 of 10

    A self-dual loop quantum black hole is shown to look smaller and brighter than Schwarzschild in thin disk models, with the polymer parameter P bounded by Mercury and S2 star data.

  3. Polymer Black Hole Surrounded by Quintessence

    gr-qc 2025-07 conditional novelty 3.0 of 10

    A polymer black hole with quintessence yields a shadow that can match Sgr A* for many combinations of free parameters while cooling and dimming the black hole.

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