No accelerating scaling cosmologies at string tree level?
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Publication:6497815
DOI10.1088/1475-7516/2024/01/055WikidataQ129398702 ScholiaQ129398702MaRDI QIDQ6497815
Publication date: 6 May 2024
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Cites Work
- A note on obstinate tachyons in classical dS solutions
- Inflationary constraints on type IIA string theory
- Tachyons in classical de Sitter vacua
- The \(F\)-term problem and other challenges of stringy quintessence
- Time-dependent compactification to De Sitter space: a no-go theorem
- Scaling limits of ds vacua and the swampland
- Weakly coupled de Sitter vacua with fluxes and the swampland
- Eternal acceleration from M-theory
- Asymptotic scalar field cosmology in string theory
- Stringy multifield quintessence and the swampland
- Universal accelerating cosmologies from 10d supergravity
- SUPERGRAVITY DESCRIPTION OF FIELD THEORIES ON CURVED MANIFOLDS AND A NO GO THEOREM
- De Sitter hunting in a classical landscape
- Scaling cosmologies of gauged supergravity
- Scalar cosmology with multi-exponential potentials
- What if string theory has no de Sitter vacua?
- Dynamics of generalized assisted inflation
- Runaway quintessence, out of the swampland
- On asymptotic dark energy in string theory
- The Asymptotic dS Swampland Conjecture ‐ a Simplified Derivation and a Potential Loophole
- Tachyonic de Sitter Solutions of 10d Type II Supergravities
- Superstring cosmology — a complementary review
- Asymptotic accelerated expansion in string theory and the swampland
- No asymptotic acceleration without higher-dimensional de Sitter vacua
- Beginners lectures on flux compactifications and related swampland topics
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