Higgs condensation as an unwanted curvaton
arXiv:1208.2316 · doi:10.1103/PhysRevD.86.083541
Abstract
During inflation in the early universe, the Higgs field continuously acquires long-wave quantum fluctuations. They accumulate to yield a non-vanishing value with an exponentially large correlation length. We study consequences of such Higgs condensations to show that, in inflation models where the universe is reheated through gravitational particle production at the transition to the kination regime, they not only contribute to reheat the universe but also act as a curvaton. Unfortunately, however, for parameters of the Standard Model Higgs field, this curvaton produces density fluctuations too large, so the inflation models followed by a long kination regime are ruled out.
13 pages; v2, layout adjusted, references added
References in corpus (9)
- Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC
- Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC
- The Standard Model Higgs boson as the inflaton
- G-inflation: inflation driven by the Galileon field
- Inflation scenario via the Standard Model Higgs boson and LHC
- Cosmological implications of the Higgs mass measurement
- Higgs G-inflation
- Gravitational corrections to Standard Model vacuum decay
- Higgs Chaotic Inflation in Standard Model and NMSSM
Cited by in corpus (39)
- The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe
- Higgs Scalaron Mixed Inflation
- Cosmological Aspects of Higgs Vacuum Metastability
- Higgs Dynamics during Inflation
- Gravitational particle creation for dark matter and reheating
- Spectator Dark Matter
- The Standard Model Higgs as the origin of the hot Big Bang
- Gravitational reheating through conformally coupled superheavy scalar particles
- Galilean Creation of the Inflationary Universe
- Scalar correlation functions in de Sitter space from the stochastic spectral expansion
- Inconsistency of an inflationary sector coupled only to Einstein gravity
- Gravitational wave production from the decay of the Standard Model Higgs field after inflation
- Gravitational wave signals and cosmological consequences of gravitational reheating
- Bounce Inflation Cosmology with Standard Model Higgs Boson
- Minimal -inflation in light of the conformal metric-affine geometry
- Scalar correlation functions for a double-well potential in de Sitter space
- The Higgs field and early universe cosmology: a (brief) review
- Reheating through the Higgs amplified by spinodal instabilities and gravitational creation of gravitons
- Gravitational leptogenesis with kination and gravitational reheating
- Dark matter and baryon-number generation in quintessential inflation via hierarchical right-handed neutrinos
- The Secret Higgstory of the Highest Temperature during Reheating
- No quasi-stable scalaron lump forms after inflation
- Stochastic evolution of scalar fields with continuous symmetries during inflation
- Renormalization in gravitational leptogenesis with pseudo-scalar-tensor coupling
- An analytic evaluation of gravitational particle production of fermions via Stokes phenomenon
- Note on Reheating in G-inflation
- Reheating via gravitational particle production in kination epoch
- Standard model Higgs field and hidden sector cosmology
- New parameterization for unified dark matter and dark energy
- Reheating and particle creation in unimodular f(R, T) gravity
- Large Density Perturbations from Reheating to Standard Model particles due to the Dynamics of the Higgs Boson during Inflation
- Thermal and nonthermal dark matters with gravitational neutrino reheating
- Spectator dark matter in non-standard cosmologies
- Stochastic Baryogenesis
- Gauge Field Production and Schwinger Reheating in Runaway Axion Inflation
- Generation of neutrino dark matter, baryon asymmetry, and radiation after quintessential inflation
- Thermodynamics of the Primordial Universe
- Hill-climbing dark inflation
- Reheating in the kination epoch via multi-channel decay of gravitationally created massive scalars