Stringy Spacetime Uncertainty Principle and a Modified Trans-Planckian Censorship Criterion
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| Main Authors: | , , , |
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| Format: | Preprint |
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2024
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| _version_ | 1866909065271050240 |
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| author | Brandenberger, Robert Ho, Pei-Ming Kawai, Hikaru Shao, Wei-Hsiang |
| author_facet | Brandenberger, Robert Ho, Pei-Ming Kawai, Hikaru Shao, Wei-Hsiang |
| contents | We study the implications of the stringy space-time uncertainty relation (STUR) for inflationary cosmology. By demanding that no fluctuation modes that exit the Hubble radius are affected by the nonlocality resulting from the STUR, we find an upper bound on the number of e-foldings of inflation. The bound is a factor of 2 weaker than what results from the Trans-Planckian Censorship Criterion (TCC). By demanding that the inflationary phase is simultaneously consistent with STUR and sufficiently long for inflation to provide a causal explanation of structure on the scale of the current Hubble radius, we find an upper bound on the energy scale of inflation. The bound is less restrictive than what follows from the TCC, but it remains in conflict with canonical single-field inflation models. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2401_04097 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Stringy Spacetime Uncertainty Principle and a Modified Trans-Planckian Censorship Criterion Brandenberger, Robert Ho, Pei-Ming Kawai, Hikaru Shao, Wei-Hsiang High Energy Physics - Theory Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Phenomenology We study the implications of the stringy space-time uncertainty relation (STUR) for inflationary cosmology. By demanding that no fluctuation modes that exit the Hubble radius are affected by the nonlocality resulting from the STUR, we find an upper bound on the number of e-foldings of inflation. The bound is a factor of 2 weaker than what results from the Trans-Planckian Censorship Criterion (TCC). By demanding that the inflationary phase is simultaneously consistent with STUR and sufficiently long for inflation to provide a causal explanation of structure on the scale of the current Hubble radius, we find an upper bound on the energy scale of inflation. The bound is less restrictive than what follows from the TCC, but it remains in conflict with canonical single-field inflation models. |
| title | Stringy Spacetime Uncertainty Principle and a Modified Trans-Planckian Censorship Criterion |
| topic | High Energy Physics - Theory Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2401.04097 |