Warm dark energy
DOI10.1088/1475-7516/2020/08/032zbMath1492.83034arXiv1912.09950OpenAlexW3099450211MaRDI QIDQ5070333
No author found.
Publication date: 11 April 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1912.09950
Other elementary particle theory in quantum theory (81V25) String and superstring theories in gravitational theory (83E30) Supergravity (83E50) Oscillation, zeros of solutions, mean value theorems, etc. in context of PDEs (35B05) Classical and relativistic thermodynamics (80A10) Yang-Mills and other gauge theories in mechanics of particles and systems (70S15) Dark matter and dark energy (83C56)
Related Items (3)
Cites Work
- The effective action of \(N=1\) Calabi-Yau orientifolds
- The effective action of D7-branes in \(N=1\) Calabi-Yau orientifolds
- The effective action of type IIA Calabi--Yau orientifolds
- Special geometry, cubic polynomials and homogeneous quaternionic spaces
- \(N=2\) supergravity and \(N=2\) super Yang-Mills theory on general scalar manifolds: symplectic covariance, gaugings and the momentum map
- Planckian axions and the weak gravity conjecture
- Axion monodromy and the weak gravity conjecture
- Symmetry structure of special geometries
- On the de Sitter swampland criterion
- Trans-Planckian censorship and the swampland
- Warm Little Inflaton becomes dark energy
- Relic abundance of dark photon dark matter
- Warm quintessential inflation
- Transplanckian axions!?
- Fencing in the swampland: quantum gravity constraints on large field inflation
- Planckian axions in string theory
- Weak gravity strongly constrains large-field axion inflation
- A review of axion inflation in the era of Planck
- Primordial black holes and associated gravitational waves in axion monodromy inflation
- Conditions for (no) eternal inflation
- Lattice formulation of axion inflation. Application to preheating
- The symplectic structure of \(N=2\) supergravity and its central extension
- Consistent reduction of \(N=2\rightarrow N=1\) four-dimensional supergravity coupled to matter
- The Landscape, the Swampland and the Era of Precision Cosmology
- On Exclusion of Positive Cosmological Constant
- Further Refining the de Sitter Swampland Conjecture
- The Swampland: Introduction and Review
This page was built for publication: Warm dark energy