Quantum Fisher Cosmology: Confronting Observations and the Trans-Planckian Problem
arXiv:2105.05251 · doi:10.1088/1475-7516/2021/09/016
Abstract
The aim of Quantum Fisher Cosmology is to use the quantum Fisher information about pure de Sitter states to derive model independent observational consequences of the existence of a primordial phase of the Universe of de Sitter accelerated expansion. These quantum features are encoded in a scale dependent quantum cosmological tilt that defines what we can call the de Sitter universality class. The experimental predictions are: i) A phase transition from red into blue tilt at a scale order Mpc that naturally solves the cosmological trans-Planckian problem, ii) A spectral index for curvature fluctuations at CMB scales Mpc equal to , iii) A tilt running at scale Mpc equal to , iv) An enhancement of the amplitude of CMB peaks for extremely high multipoles () that can provide a natural mechanism for primordial black hole formation as a source of dark matter, v) A lack of power at scales of Mpc with respect to the CMB scale that can explain the tension.
arXiv commentMatches accepted version to JCAP. Added a longer explanation on the role of the alpha-vacua and how quantum fisher is evaluated in their presence. Results unchanged
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