Thermalization after inflation and production of massive stable particles
arXiv:hep-ph/0205246 · doi:10.1103/PhysRevD.66.063513
Abstract
We discuss thermalization through perturbative inflaton decay at the end of inflation. We find that a thermal plasma should form well before all inflatons have decayed, unless all gauge symmetries are badly broken during that epoch. However, before they thermalize, the very energetic inflaton decay products can contribute to the production of massive stable particles, either through collisions with the thermal plasma, or through collisions with each other. If such reactions exist, the same massive particles can also be produced directly in inflaton decay, once higher--order processes are included. We show that these new, non--thermal production mechanisms often significantly strengthen constraints on the parameters of models containing massive stable particles; for example, stable charged particles with mass below the inflaton mass seem to be essentially excluded.
Revtex, 18 pages, 3 figures, uses axodraw. References added. Final version to appear in Phys. Rev. D
References in corpus (7)
- The MSSM Parameter Space with Non-Universal Higgs Masses
- Higgsino and Wino Dark Matter from Q-ball Decay in Affleck-Dine Baryogenesis
- Constraining Supersymmetry
- Production of massive stable particles in inflaton decay
- Relic Neutralino Density in Scenarios with Intermediate Unification Scale
- Possible astrophysical signatures of heavy stable neutral relics in supergravity models
- From (p)reheating to nucleosynthesis
Cited by in corpus (81)
- Reheating in Inflationary Cosmology: Theory and Applications
- Neutralino with the Right Cold Dark Matter Abundance in (Almost) Any Supersymmetric Model
- Equation of state and Beginning of Thermalization After Preheating
- The effect of a late decaying scalar on the neutralino relic density
- Reheating Effects in the Matter Power Spectrum and Implications for Substructure
- Freeze-In Dark Matter with Displaced Signatures at Colliders
- Dark Matter Production in Late Time Reheating
- When the Universe Expands Too Fast: Relentless Dark Matter
- Relic Abundance of Asymmetric Dark Matter
- Ultraviolet Freeze-in and Non-Standard Cosmologies
- Chilly Dark Sectors and Asymmetric Reheating
- Observing Invisible Axions with Gravitational Waves
- Massive Particle Decay and Cold Dark Matter Abundance
- Supersymmetric Dark Matter and the Reheating Temperature of the Universe
- Multiple dark matter scenarios from ubiquitous stringy throats
- Dark Matter Production in an Early Matter Dominated Era
- Resonant decay of flat directions
- Supersymmetric Thermalization and Quasi-Thermal Universe: Consequences for Gravitinos and Leptogenesis
- Ultra-cold WIMPs: relics of non-standard pre-BBN cosmologies
- Abundance of Cosmological Relics in Low-Temperature Scenarios
- Constraining Non-thermal and Thermal properties of Dark Matter
- Right-Handed Sneutrinos as Curvatons
- Connecting CMB anisotropy and cold dark matter phenomenology via reheating
- UV Freeze-in in Starobinsky Inflation
- A simple nonsingular inflationary quintessential model
- Reheating in supersymmetric high scale inflation
- Identifying the curvaton within MSSM
- Constraints on the Very Early Universe from Thermal WIMP Dark Matter
- Neutralino Dark Matter in Scenarios with Early Matter Domination
- TeV Scale Leptogenesis with Dark Matter in Non-standard Cosmology
- Quantifying the reheating temperature of the universe
- Boosted Dark Matter and its implications for the features in IceCube HESE data
- Boosting Ultraviolet Freeze-in in NO Models
- Energy Spectrum of Thermalizing High Energy Decay Products in the Early Universe
- Gravitational particle production in bouncing cosmologies
- On the viability of quintessential inflationary models from observational data
- Cosmological perturbations for an inflaton field coupled to radiation
- Longevity of supersymmetric flat directions
- Boosted Neutrinos and Relativistic Dark Particles as Messengers from Reheating
- Affleck-Dine Baryogenesis and Dark Matter Production after High-scale Inflation
- Leptogenesis from a sneutrino condensate revisited
- Enlarging mSUGRA parameter space by decreasing pre-BBN Hubble rate in Scalar-Tensor Cosmologies
- Non-thermal production of Dark Matter after Inflation
- Direct detection of neutralino dark mattter in non-standard cosmologies
- GUTzilla Dark Matter
- Symmetric and Asymmetric Reheating
- Non-thermal leptogenesis with almost degenerate superheavy neutrinos
- Cascades of high-energy SM particles in the primordial thermal plasma
- Post-inflationary thermalization with hadronization scenario
- Inflation and late-time acceleration from a double-well potential with cosmological constant
- keV Neutrino Dark Matter in a Fast Expanding Universe
- Dark Matter Casts Light on the Early Universe
- SUSY In The Sky: Observing Ultra-High Energy Cosmic Neutralinos
- Concealing Dirac neutrinos from cosmic microwave background
- Electroweak Vacuum Stabilized by Moduli during/after Inflation
- Freeze-in Production of Dark Matter Prior to Early Matter Domination
- Direct baryogenesis in the broken phase
- Superheavy Dark Matter from String Theory
- Muon g-2 in Anomaly Mediated SUSY Breaking
- High Energy Sphalerons for Baryogenesis at Low Temperatures
- Higgsino Dark Matter in a Non-Standard History of the Universe
- Leptogenesis and rescattering in supersymmetric models
- Leptogenesis as the source of gravitino dark matter and density perturbations
- Sleptogenesis
- Variable Inflaton Equation of State and Reheating
- WIMPy Leptogenesis in Non-Standard Cosmologies
- Constraints on Minimal SUSY models with warm dark matter neutralinos
- Heavy Particles from Inflation
- Thermal abundance of non-relativistic relics with Sommerfeld enhancement
- A map of the non-thermal WIMP
- New developments on embedding inflation in gauge theory and particle physics
- Decay of Super-Heavy particles: User guide of the SHdecay program
- Seminatural SUSY from Nonlinear Sigma Model
- Boltzmann equations for preheating
- Supermassive gravitinos, dark matter, leptogenesis and flat direction baryogenesis
- Cosmological bounds on large extra dimensions from non-thermal production of Kaluza-Klein modes
- Dark matter cooling during early matter-domination boosts sub-earth halos
- High Reheating Temperature without Axion Domain Walls
- Light Thermal Self-Interacting Dark Matter in the Shadow of Non-Standard Cosmology
- Cosmology of Single Species Hidden Dark Matter
- The Early Universe with High-Scale Supersymmetry