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Black Hole Mergers in Holographic Space Time Models of Cosmology
by Anish Suresh, Tom Banks
This Submission thread is now published as
Submission summary
| Authors (as registered SciPost users): | Thomas Banks |
| Submission information | |
|---|---|
| Preprint Link: | scipost_202306_00016v2 (pdf) |
| Date accepted: | July 9, 2024 |
| Date submitted: | May 24, 2024, 8:20 p.m. |
| Submitted by: | Banks, Thomas |
| Submitted to: | SciPost Physics Core |
| Ontological classification | |
|---|---|
| Academic field: | Physics |
| Specialties: |
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| Approaches: | Theoretical, Computational |
Abstract
We perform a crude computer simulation to show that no problematic black holes are formed by mergers in the early matter dominated phase of the HST models of inflation. These are black holes whose decays could have been seen as signals in the CMB. We also conclude that tiny "black hole galaxies" form. Since black hole decay products are mostly massive standard model particles, and perhaps their superpartners, the fate of these proto-galaxies is a complicated dynamical problem. It suggests the possibility of primordial structures on the order of the horizon size at the beginning of the radiation dominated era. This is about $10^9\ L_P$ in the current model.
Author comments upon resubmission
List of changes
Extensive introduction to the principles of Holographic Space Time Models of Inflation. All units changed to natural units. Numerous other changes.
Published as SciPost Phys. Core 7, 057 (2024)
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