A dynamical inflaton coupled to strongly interacting matter
- According to the inflationary theory of cosmology, most elementary particles in the current universe were created during a period of reheating after inflation. In this work we self-consistently couple the Einstein-inflaton equations to a strongly coupled quantum field theory (QFT) as described by holography. We show that this leads to an inflating universe, a reheating phase and finally a universe dominated by the QFT in thermal equilibrium.
| Author: | Christian EckerORCiD, Elias KiritsisORCiDGND, Wilke van der ScheeORCiD |
|---|---|
| URN: | urn:nbn:de:hebis:30:3-825506 |
| URL: | https://arxiv.org/abs/2302.06618v1 |
| DOI: | https://doi.org/10.48550/arXiv.2302.06618 |
| ArXiv Id: | http://arxiv.org/abs/2302.06618v1 |
| Parent Title (English): | arXiv |
| Publisher: | arXiv |
| Document Type: | Preprint |
| Language: | English |
| Date of Publication (online): | 2023/02/13 |
| Date of first Publication: | 2023/02/13 |
| Publishing Institution: | Universitätsbibliothek Johann Christian Senckenberg |
| Release Date: | 2024/04/30 |
| Issue: | 2302.06618 Version 1 |
| Edition: | Version 1 |
| Page Number: | 9 |
| HeBIS-PPN: | 518934047 |
| Institutes: | Physik / Physik |
| Dewey Decimal Classification: | 5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik |
| Sammlungen: | Universitätspublikationen |
| Licence (German): |  Creative Commons - Namensnennung 4.0 |
