Can Primordial Black Holes Be Seeds for Early Galaxies in Models Satisfying the Covariant Entropy Bound?

arXiv:2607.01292 · hep-ph, astro-ph.CO, gr-qc, hep-th · Submitted 2026-07-01 · Read on arXiv

Sidan A, Tom Banks, Willy Fischler

hep-ph, astro-ph.CO, gr-qc, hep-th

Submitted: 2026-07-01

Comments: 22 pages, 6 figures, v2: revision to Appendix B, references added, v3: references added

License: http://creativecommons.org/licenses/by/4.0/

The gist: We argue that cosmological models obeying the Covariant Entropy Bound (CEB) mathematically favor states with no localized excitations or one large black hole containing all the energy in a

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Abstract

We argue that cosmological models obeying the Covariant Entropy Bound (CEB) mathematically favor states with no localized excitations or one large black hole containing all the energy in a constrained initial state. In order to get a long radiation-dominated era, one must postulate that at a very early time, most horizon volumes of the universe contained tiny black holes that decayed into radiation. A previous work by two of the authors showed that such a scenario could fit the data on the Cosmic Microwave Background (CMB). In order to account for dark matter, we also postulate some random black holes of at least horizon size at that time. A reasonable distribution of such primordial black holes can account for all of dark matter as well as the early galaxies seen by the James Webb Space Telescope. Some of the dark matter may also be in Planck-scale remnants of the decaying black holes. We describe our model both in terms of approximate solutions to General Relativity and a speculative quantum gravity model whose hydrodynamics matches the flat p = plus or minus rho FRW model that saturates the CEB.

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