Stringy multifield quintessence and the swampland
From MaRDI portal
Publication:2686350
DOI10.1007/JHEP11(2022)044MaRDI QIDQ2686350
Giuseppe Dibitetto, Max Brinkmann, Michele Cicoli, Francisco G. Pedro
Publication date: 27 February 2023
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2206.10649
Related Items (3)
Constraints on late time violations of the equivalence principle in the dark sector ⋮ On asymptotic dark energy in string theory ⋮ No asymptotic acceleration without higher-dimensional de Sitter vacua
Cites Work
- \(N=1\) no-scale supergravity from IIB orientifolds
- Global embedding of fibre inflation models
- \(\alpha'\) inflation: moduli stabilisation and observable tensors from higher derivatives
- A geometrical upper bound on the inflaton range
- A new class of de Sitter vacua in type IIB large volume compactifications
- Chiral global embedding of fibre inflation models
- RG-induced modulus stabilization: perturbative de Sitter vacua and improved D3-\(\overline{\mathrm{D}3}\) inflation
- Multi-field dark energy: cosmic acceleration on a steep potential
- Constructing stable De Sitter in M-theory from higher curvature corrections
- Moduli stabilisation for chiral global models
- Toric \(K3\)-fibred Calabi-Yau manifolds with del Pezzo divisors for string compactifications
- Out of the swampland with multifield quintessence?
- Quintessence: a review
- Cosmological parameters from SDSS and WMAP
- Quintessence with O ( N ) symmetry
- What if string theory has no de Sitter vacua?
- A geometrical instability for ultra-light fields during inflation?
- Late-time cosmic acceleration from compactification
- The string swampland constraints require multi-field inflation
- De Sitter vs Quintessence in String Theory
- Further Refining the de Sitter Swampland Conjecture
- UV Shadows in EFTs: Accidental Symmetries, Robustness and No‐Scale Supergravity
This page was built for publication: Stringy multifield quintessence and the swampland
