Massive scalar field evolution in de Sitter
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Publication:1678944
DOI10.1007/JHEP01(2017)133zbMath1373.83019arXiv1607.00334WikidataQ63353996 ScholiaQ63353996MaRDI QIDQ1678944
Tommi Markkanen, Arttu K. Rajantie
Publication date: 7 November 2017
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1607.00334
Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Kaluza-Klein and other higher-dimensional theories (83E15) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Analogues of general relativity in lower dimensions (83C80)
Related Items (9)
Markovian dynamics in de Sitter ⋮ Light scalars on cosmological backgrounds ⋮ Gravitational production of superheavy dark matter and associated cosmological signatures ⋮ Gravitational particle creation in a stiff matter dominated universe ⋮ Decoherence can relax cosmic acceleration: an example ⋮ Renormalization of the inflationary perturbations revisited ⋮ Cosmological constant problem and renormalized vacuum energy density in curved background ⋮ Primordial black holes from thermal inflation ⋮ A manifestly covariant theory of multifield stochastic inflation in phase space: solving the discretisation ambiguity in stochastic inflation
Cites Work
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- Particle creation by black holes
- Decay of vacuum energy
- De Sitter space and eternity
- The quantum gravitational back-reaction on inflation
- Attractor states and quantum instabilities in de Sitter space
- Quantum gravity slows inflation
- The four laws of black hole mechanics
- Asymptotic behavior of homogeneous cosmological models in the presence of a positive cosmological constant
- Quantum Field Theory in Curved Spacetime
- Inflation and de Sitter thermodynamics
- Thermodynamics of Spacetime: The Einstein Equation of State
- Classical and quantum thermodynamics of horizons in spherically symmetric spacetimes
- Super-acceleration from massless, minimally coupled $\phi$4
- Black Holes and Entropy
- Black hole explosions?
- Quantized Fields and Particle Creation in Expanding Universes. I
- On Gauge Invariance and Vacuum Polarization
- Quantum Fields in Curved Space
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