Towards a formal description of the collapse approach to the inflationary origin of the seeds of cosmic structure
Alberto Diez-Tejedor, Daniel Sudarsky

TL;DR
This paper explores a formal quantum field theory approach to the collapse hypothesis for the origin of cosmic structure, questioning the compatibility of this process with a purely geometric space-time description.
Contribution
It develops a detailed formalism for the collapse process in inflationary cosmology, linking quantum field theory with the emergence of inhomogeneities, and challenges purely geometric models.
Findings
Collapse mechanism can produce primordial inhomogeneities
Results suggest incompatibility with purely geometric space-time
Provides a transparent quantum field theoretical framework
Abstract
Inflation plays a central role in our current understanding of the universe. According to the standard viewpoint, the homogeneous and isotropic mode of the inflaton field drove an early phase of nearly exponential expansion of the universe, while the quantum fluctuations (uncertainties) of the other modes gave rise to the seeds of cosmic structure. However, if we accept that the accelerated expansion led the universe into an essentially homogeneous and isotropic space-time, with the state of all the matter fields in their vacuum (except for the zero mode of the inflaton field), we can not escape the conclusion that the state of the universe as a whole would remain always homogeneous and isotropic. It was recently proposed in [A. Perez, H. Sahlmann and D. Sudarsky, "On the quantum origin of the seeds of cosmic structure," Class. Quant. Grav. 23, 2317-2354 (2006)] that a collapse…
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