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We study evolution and thermodynamics of a slow-roll transition between early and late time de Sitter phases, both in the homogeneous case and in the presence of a black hole, in a scalar field model with a generic potential having both a maximum and a positive minimum.
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K. Skenderis and P. K. Townsend, Hidden supersymmetry of domain walls and cosmologies
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K. Skenderis and P. K. Townsend, Hamilton-Jacobi method for curved domain walls and cosmologies
2006
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M. Henneaux, C. Martinez, R. Troncoso and J. Zanelli, Asymptotic behavior and Hamiltonian analysis of anti-de Sitter gravity coupled to scalar fields
2007
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P. McFadden and K. Skenderis, The Holographic Universe
2007
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K. Skenderis and P. K. Townsend, Pseudo-Supersymmetry and the Domain-Wall/Cosmology Correspondence
2007
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V. Faraoni and A. Jacques, Cosmological expansion and local physics
2007
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2013
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E. O. Babichev, V. I. Dokuchaev and Y. N. Eroshenko, Black holes in the presence of dark energy
2013
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U. Kol, On the dual flow of slow-roll Inflation
2014
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S. Chadburn and R. Gregory, Time dependent black holes and scalar hair
2014
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2014
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2014
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F. Faedo, D. Klemm and M. Nozawa, Hairy black holes in N = 2 \rm{N}=2 gauged supergravity
2015
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J. Kaplan and J. Wang, An Effective Theory for Holographic RG Flows
2015
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B. Carr, F. Kuhnel and M. Sandstad, Primordial Black Holes as Dark Matter
2016
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A. C. Davis, R. Gregory and R. Jha, Black hole accretion discs and screened scalar hair
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