Graviton spectrum in simplified Dark Matter models with graviton mediators in the de Sitter space
arXiv:1812.10297 · doi:10.3390/universe5010039
Abstract
This is the second in a series of papers investigating the formulation of the simplified Dark Matter models with graviton mediators in cosmological backgrounds. We address here the crucial problem of the fundamental observable of interest, namely the graviton spectrum in a FRW cosmological background with an arbitrary Dark Matter background component. We calculate the correction to the free graviton two-point function up to the second order in the coupling constant between the Dark Matter and the graviton in the simplified Dark Matter model with graviton mediators approach in the de Sitter space. Our result is model independent in the sense that it does not depend on the particular form of the Dark Matter fields. Also, due to the universality of the interaction between the Dark Matter and the graviton, the result obtained here apply to the interaction between the baryonic matter and the gravitons. As an application, we discuss in detail the massive scalar Dark Matter model and calculate the first order correction to the two-point function due to two Dark Matter modes in the adiabatic regime.
Typos corrected. A new section on the scalar Dark Matter model added
References in corpus (11)
- A direct empirical proof of the existence of dark matter
- Observations of extended radio emission in clusters
- Strong and weak lensing united III: Measuring the mass distribution of the merging galaxy cluster 1E0657-56
- Revealing the properties of dark matter in the merging cluster MACSJ0025.4-1222
- A filament of dark matter between two clusters of galaxies
- Recommendations of the LHC Dark Matter Working Group: Comparing LHC searches for heavy mediators of dark matter production in visible and invisible decay channels
- Path Integral for Inflationary Perturbations
- Sensitivity of the Cherenkov Telescope Array to the detection of a dark matter signal in comparison to direct detection and collider experiments
- Planet-bound dark matter and the internal heat of Uranus, Neptune, and hot-Jupiter exoplanets
- How to Wick rotate generic curved spacetime
- Direct evidence of hierarchical assembly at low masses from isolated dwarf galaxy groups