2020
DOI: 10.1103/physrevd.102.023507
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Quantum initial conditions for inflation and canonical invariance

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Cited by 10 publications
(9 citation statements)
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“…( 7) and ( 8) in a more appropriate form. As observed by Agocs et al [20], there is considerable freedom in the form that these equations take, as one may simultaneously transform both the independent and dependent variables.…”
Section: The Mukhanov-sazaki Equationmentioning
confidence: 99%
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“…( 7) and ( 8) in a more appropriate form. As observed by Agocs et al [20], there is considerable freedom in the form that these equations take, as one may simultaneously transform both the independent and dependent variables.…”
Section: The Mukhanov-sazaki Equationmentioning
confidence: 99%
“…In the fast-roll and kinetically dominated paradigms, this condition can never be fulfilled for small k. In these cases, the situation becomes less clear-cut, although alternative initial conditions have been proposed [18][19][20].…”
Section: Introductionmentioning
confidence: 99%
“…Hence the key features in these primordial power spectra, which may allow for experimentally distinguishing between vacuum initial conditions, are the position of the low k cutoff and the size of any oscillations in the intermediate k region. Therefore qualitatively it seems RSET may be observationally distinguishable from the other three, this idea has been previously discussed in [9,10].…”
Section: E Approximating the Primordial Power Spectramentioning
confidence: 55%
“…There remains much debate as to which of the proposed vacua is the correct one to set. Detailed discussions of the theoretical merits and issues of some of these different choices can be found in [9,10].…”
Section: Initial Condition Definitionmentioning
confidence: 99%
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