Tomographic analysis of quantum and classical de Sitter cosmological models
2019 ◽
Vol 28
(16)
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pp. 2040009
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Keyword(s):
In this work, we show the importance of introducing the quantum tomography formalism to analyze the properties of wave functions in quantum cosmology. In particular, we examine the initial conditions of the universe proposed by various authors in the context of de Sitter’s cosmology studying their classical limit and comparing it with the classical tomogram obtained from the Hamiltonian constraint in General Relativity. This comparison gives us the opportunity to find under which conditions there is a transition from the quantum universe to the classical one. A relevant result is that in these models the decay of the cosmological constant is a sufficient condition for this transition.
2019 ◽
Vol 16
(01)
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pp. 1950012
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2017 ◽
Vol 32
(30)
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pp. 1750164
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Keyword(s):
2001 ◽
Vol 10
(06)
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pp. 943-956
2017 ◽
Vol 26
(10)
◽
pp. 1750116
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Keyword(s):
2016 ◽
Vol 25
(08)
◽
pp. 1642003
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Keyword(s):
2005 ◽
Vol 14
(02)
◽
pp. 291-307
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2002 ◽
Vol 2
(4)
◽
pp. 173-182
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Keyword(s):