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A new solution of a unitary moving mirror is found to produce finite energy and emit thermal radiation despite the absence of an acceleration horizon.
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2014
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2014
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2014
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2014
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2003
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L. H. Ford, T. A. Roman, “Energy Flux Correlations and Moving Mirrors”, Phys. Rev. D 70
2004
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A. Fabbri, J. Navarro-Salas, Modeling Black Hole Evaporation , London, UK: Imp. Coll. Pr., 2005
2005
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2007
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2008
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2010
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D. T. Alves, E. R. Granhen, H. O. Silva, M. G. Lima, “Quantum Radiation Force on the Moving Mirror of a Cavity, with Dirichlet and Neumann Boundary Conditions for a Vacuum, Finite Temperature, and a Coherent State”, Phys. Rev. D 81
2010
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2015
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2015
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2015
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2015
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2015
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M. Christodoulou, C. Rovelli, “How Big is a Black Hole?”, Phys. Rev. D 91
2015
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Y. C. Ong, “The Persistence of the Large Volumes in Black Holes”, Gen. Relativ. Gravit. 47
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2015
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Q. Wang, W. G. Unruh, “Mirror Moving in Quantum Vacuum of a Massive Scalar Field”, Phys. Rev. D 92
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2015
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N. Nicolaevici, “Unruh Effect Without Rindler Horizon,” Class. Quant. Grav. 32
2015
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2015
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2015
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2015
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2015
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2016
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2016
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M. R. R. Good, P. R. Anderson, C. R. Evans, “Mirror Reflections of a Black Hole”, Phys. Rev. D 94
2016
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P.-M. Ho, “The Absence of Horizon in Black-Hole Formation”, Nucl. Phys. B 909
2016
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Y. Sekino, L. Susskind, “Fast Scramblers”, JHEP 10
2096
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