String theory and the first half of the universe
We perform a detailed study of stringy moduli-driven cosmologies between the end of inflation and the commencement of the Hot Big Bang, including both the background and cosmological perturbations: a period that can cover half the lifetime of the universe on a logarithmic scale. Compared to the stan...
| Main Authors: | , , , , |
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| Formato: | Journal article |
| Idioma: | English |
| Publicado em: |
IOP Publishing
2024
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| _version_ | 1826317155714465792 |
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| author | Apers, F Conlon, JP Copeland, EJ Mosny, M Revello, F |
| author_facet | Apers, F Conlon, JP Copeland, EJ Mosny, M Revello, F |
| author_sort | Apers, F |
| collection | OXFORD |
| description | We perform a detailed study of stringy moduli-driven cosmologies between the end of inflation and the commencement of the Hot Big Bang, including both the background and cosmological perturbations: a period that can cover half the lifetime of the universe on a logarithmic scale. Compared to the standard cosmology, stringy cosmologies with vacua that address the hierarchy problem motivate extended kination, tracker and moduli-dominated epochs involving significantly trans-Planckian field excursions. We analyse the cosmology within the framework of the Large Volume Scenario but explain how analogous cosmological features are expected in other string theory models characterized by final vacua located in the asymptotic regions of moduli space. Conventional effective field theory is unable to control Planck-suppressed operators and so such epochs require a stringy completion for a consistent analysis. Perturbation growth in these stringy cosmologies is substantially enhanced compared to conventional cosmological histories. The transPlanckian field evolution results in radical changes to Standard Model couplings during this history and we outline potential applications to baryogenesis, dark matter and gravitational wave production. |
| first_indexed | 2024-09-25T04:32:46Z |
| format | Journal article |
| id | oxford-uuid:f79da13f-b7e1-4567-99b3-1a153cecec09 |
| institution | University of Oxford |
| language | English |
| last_indexed | 2025-02-19T04:34:02Z |
| publishDate | 2024 |
| publisher | IOP Publishing |
| record_format | dspace |
| spelling | oxford-uuid:f79da13f-b7e1-4567-99b3-1a153cecec092025-01-22T10:53:33ZString theory and the first half of the universeJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:f79da13f-b7e1-4567-99b3-1a153cecec09EnglishSymplectic ElementsIOP Publishing2024Apers, FConlon, JPCopeland, EJMosny, MRevello, FWe perform a detailed study of stringy moduli-driven cosmologies between the end of inflation and the commencement of the Hot Big Bang, including both the background and cosmological perturbations: a period that can cover half the lifetime of the universe on a logarithmic scale. Compared to the standard cosmology, stringy cosmologies with vacua that address the hierarchy problem motivate extended kination, tracker and moduli-dominated epochs involving significantly trans-Planckian field excursions. We analyse the cosmology within the framework of the Large Volume Scenario but explain how analogous cosmological features are expected in other string theory models characterized by final vacua located in the asymptotic regions of moduli space. Conventional effective field theory is unable to control Planck-suppressed operators and so such epochs require a stringy completion for a consistent analysis. Perturbation growth in these stringy cosmologies is substantially enhanced compared to conventional cosmological histories. The transPlanckian field evolution results in radical changes to Standard Model couplings during this history and we outline potential applications to baryogenesis, dark matter and gravitational wave production. |
| spellingShingle | Apers, F Conlon, JP Copeland, EJ Mosny, M Revello, F String theory and the first half of the universe |
| title | String theory and the first half of the universe |
| title_full | String theory and the first half of the universe |
| title_fullStr | String theory and the first half of the universe |
| title_full_unstemmed | String theory and the first half of the universe |
| title_short | String theory and the first half of the universe |
| title_sort | string theory and the first half of the universe |
| work_keys_str_mv | AT apersf stringtheoryandthefirsthalfoftheuniverse AT conlonjp stringtheoryandthefirsthalfoftheuniverse AT copelandej stringtheoryandthefirsthalfoftheuniverse AT mosnym stringtheoryandthefirsthalfoftheuniverse AT revellof stringtheoryandthefirsthalfoftheuniverse |