Out of the swampland with multifield quintessence?
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Publication:2657726
DOI10.1007/JHEP10(2020)035zbMath1456.83120arXiv2007.11011MaRDI QIDQ2657726
Giuseppe Dibitetto, Michele Cicoli, Francisco G. Pedro
Publication date: 14 March 2021
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2007.11011
Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Astrophysical cosmology (85A40)
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Cites Work
- Explicit de Sitter flux vacua for global string models with chiral matter
- Dynamical systems applied to cosmology: dark energy and modified gravity
- A new class of de Sitter vacua in type IIB large volume compactifications
- De Sitter string vacua from Dilaton-dependent non-perturbative effects
- The type IIB string axiverse and its low-energy phenomenology
- On the de Sitter swampland criterion
- Dark energy beyond quintessence: constraints from the swampland
- Hidden sectors in string theory: kinetic mixings, fifth forces and quintessence
- General analysis of dark radiation in sequestered string models
- de Sitter vacua in string theory
- Consistent de Sitter string vacua from Kähler stabilization and D‐term uplifting
- Cosmological parameters from SDSS and WMAP
- What if string theory has no de Sitter vacua?
- Scaling attractors in multi-field inflation
- Late-time cosmic acceleration from compactification
- The string swampland constraints require multi-field inflation
- The Landscape, the Swampland and the Era of Precision Cosmology
- De Sitter vs Quintessence in String Theory
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