Compact objects and the swampland
From MaRDI portal
Publication:667321
DOI10.1007/JHEP01(2019)215zbMath1409.83098arXiv1811.10844OpenAlexW2902441536WikidataQ128471209 ScholiaQ128471209MaRDI QIDQ667321
Carlos A. R. Herdeiro, Eugen Radu, Kunihito Uzawa
Publication date: 12 March 2019
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1811.10844
Relativistic cosmology (83F05) Black holes (83C57) String and superstring theories in gravitational theory (83E30) Perturbative methods of renormalization applied to problems in quantum field theory (81T15) Quantization of the gravitational field (83C45) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
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Cites Work
- Unnamed Item
- Inflationary constraints on type IIA string theory
- Comments on the four-dimensional effective theory for warped compactification
- Quantum corrections and the de Sitter swampland conjecture
- On the geometry of the string landscape and the swampland
- A no-go theorem for string warped compactifications
- Spinning Kerr black holes with stationary massive scalar clouds: the large-coupling regime
- The swampland conjecture and F-term axion monodromy inflation
- Non-supersymmetric AdS and the swampland
- Do we live in the swampland?
- Infinite distances in field space and massless towers of states
- Dark energy beyond quintessence: constraints from the swampland
- The quantum swampland
- Fencing in the swampland: quantum gravity constraints on large field inflation
- SUPERGRAVITY DESCRIPTION OF FIELD THEORIES ON CURVED MANIFOLDS AND A NO GO THEOREM
- Asymptotically flat black holes with scalar hair: A review
- Spinning boson stars and Kerr black holes with scalar hair: The effect of self-interactions
- Shadows of Kerr black holes with and without scalar hair
- de Sitter vacua in string theory
- Flux compactification
- Construction and physical properties of Kerr black holes with scalar hair
- Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
- General relativistic boson stars
- What if string theory has no de Sitter vacua?
- The string swampland constraints require multi-field inflation
- Dynamical boson stars
- CFT's from Calabi-Yau four-folds
- A Note on Inflation and the Swampland