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The quantum break-time of a system is the time-scale after which its true quantum evolution departs from the classical mean field evolution.
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1940
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G. W. Gibbons and S. W. Hawking, Cosmological event horizons, thermodynamics, and particle creation
1977
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A. H. Guth, Inflationary universe: A possible solution to the horizon and flatness problems
1981
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J. M. Maldacena, The Large N limit of superconformal field theories and supergravity
1999
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C. Deffayet, G. Dvali, and G. Gabadadze, Accelerated universe from gravity leaking to extra dimensions
2002
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G. Dvali, Predictive power of strong coupling in theories with large distance modified gravity
2006
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G. Dvali, S. Hofmann, and J. Khoury, Degravitation of the cosmological constant and graviton width
2007
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A. M. Polyakov, De Sitter space and eternity
2008
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2011
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C. de Rham, G. Gabadadze, and A. J. Tolley, Resummation of Massive Gravity
2011
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2012
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G. Dvali and C. Gomez, Quantum Compositeness of Gravity: Black Holes, AdS and Inflation
2014
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G. Dvali and C. Gomez, Black Holes as Critical Point of Quantum Phase Transition
2014
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F. Kühnel, Thoughts on the Vacuum Energy in the Quantum N-Portrait
2015
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2015
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G. Dvali and C. Gomez, Quantum Exclusion of Positive Cosmological Constant?
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2013
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G. Dvali and C. Gomez, Black Hole’s Quantum N-Portrait
2013
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G. Dvali and C. Gomez, Black Hole’s 1/N Hair
2013
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L. Berezhiani, On Corpuscular Theory of Inflation
Cited in the paper.
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Some aspects will be discussed in: G. Dvali, C. Gomez, L. Gründig, T. Rug, and D. Sarkar; and L. Gründig, T. Rug, and D. Sarkar (to appear)
Cited in the paper.
2016
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G. Dvali, C. Gomez, and D. Lüst, Classical Limit of Black Hole Quantum N-Portrait and BMS Symmetry
2016
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T. Markkanen, Decoherence Can Relax Cosmic Acceleration
2017
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