# Primordial black holes from collapsing antimatter

**Authors:** Gabor Etesi

arXiv: 1704.01750 · 2024-04-15

## TL;DR

This paper proposes a new, fine-tuning free mechanism for primordial black hole formation from antimatter collapse, predicting specific black hole masses, dark matter contribution, and explaining matter-antimatter asymmetry.

## Contribution

It introduces a novel antimatter collapse mechanism for primordial black holes, with testable predictions and implications for dark matter and matter-antimatter asymmetry.

## Key findings

- Photon-baryon ratio predicted as 1.95×10^9, close to observed value.
- Black hole masses are at least 10^5-10^6 solar masses.
- Primordial black holes could constitute at least 20% of dark matter.

## Abstract

In this paper a simple (i.e. free of fine-tuning, etc.) new mechanism for primordial black hole formation based on the collapse of large antimatter systems in the early Universe is introduced. A peculiarity of this process is that, compared to their material counterparts, the collapse of large antimatter systems takes much less time due to the reversed thermodynamics of antimatter, an idea which has been proposed in our earlier paper.   This model has several testable predictions. The first is that the photon-baryon ratio is roughly computable and is equal to $1.95\times 10^9$ which is quite close to its experimentally confirmed value. The second is that the mass of black holes arising from this mechanism is at least $10^5$-$10^6M_\odot$ hence they contribute to the super- or hypermassive end of the primordial black hole mass spectrum. The third prediction is that these sort of primordial black holes constitute at least $20\%$ of dark matter. Last but not least the observed current asymmetry of matter and antimatter, even if their presence in the Universe was symmetric in the beginning, acquires a natural explanation, too.

## Full text

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## References

13 references — full list in the complete paper: https://tomesphere.com/paper/1704.01750/full.md

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Source: https://tomesphere.com/paper/1704.01750