Inflaton vacuum fluctuations as dark matter and the potential V(phi) as dark energy
arXiv:1712.07960
Abstract
It is shown, using quantum field theory in curved spacetime, how the expansion of the universe during inflation produces an aggregate of particles and inflaton vacuum fluctuations at a temperature of 5x10^17GeV and dense enough to make reheating unnecessary. The standard calculation that predicts the Hubble parameter has to be way smaller than the Planck energy is shown to be fallacious: it applies the conservation of the perturbative curvature R to a single inflaton fluctuation when it should be applied to the energy density contrast of an aggregate. The quantum inflaton fluctuations varphi are with respect to the classical value phi_0 of the inflaton field phi=phi_0+varphi. Fluctuations varphi that have grown to the size of the horizon, or a pair of virtual particles that are separated by a distance the length of the horizon, are forced to become real and take energy from the potential V(phi_0). The slowing down of inflation is due to the eventual domination of the continuously being created radiation over the decreasing inflaton potential V(phi_0). It is not necessary at all for the potential V(phi_0) to go to zero. Since there is no need for reheating the inflaton field phi does not couple to matter (except gravitationally). After inflation, the fluctuations varphi quickly cool down and can be described as dark matter. Now the inverse process begins to occur. Inflaton fluctuations varphi that exited the horizon during inflation begin reentering it after inflation's end. Then they are again causally connected and have a probability of undergoing the inverse of the quantum process they underwent before and give their energy back to the potential V(phi_0). The varphi fluctuations are turning into V(phi_0), which acts as dark energy and accelerates again the expansion of the universe. The disintegration of a perturbation is a quantum jump of cosmological size.
16 pages. Calculation, using quantum field theory in curved space, of density of matter and its temperature produced during inflation, has been added. Section 2 and the Abstract have been rewritten for clarity
References in corpus (13)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- A direct empirical proof of the existence of dark matter
- An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi-GBM Detection of GRB 170817A
- Dark Energy after GW170817: dead ends and the road ahead
- Strong constraints on cosmological gravity from GW170817 and GRB 170817A
- Dark Energy after GW170817 and GRB170817A
- Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories
- Nonperturbative Dynamics Of Reheating After Inflation: A Review
- Review of LHC Dark Matter Searches
- Search for -ray line signals from dark matter annihilations in the inner Galactic halo from ten years of observations with H.E.S.S
- Indirect Detection of WIMP Dark Matter: a compact review
- A review of the past and present MAGIC dark matter search program and a glimpse at the future