Higgs field in cosmology
arXiv:1909.10528 · doi:10.1007/978-3-030-51197-5_11
Abstract
The accelerated expansion of the early universe is an integral part of modern cosmology and dynamically realized by the mechanism of inflation. The simplest theoretical description of the inflationary paradigm is based on the assumption of an additional propagating scalar degree of freedom which drives inflation - the inflaton. In most models of inflation the fundamental nature of the inflaton remains unexplained. In the model of Higgs inflation, the inflaton is identified with the Standard Model Higgs boson and connects cosmology with elementary particle physics. A characteristic feature of this model is a non-minimal coupling of the Higgs boson to gravity. I review and discuss several phenomenological and fundamental aspects of this model, including the impact of quantum corrections and the renormalization group, the derivation of initial conditions for Higgs inflation in a quantum cosmological framework and the classical and quantum equivalence of different field parametrizations.
36 pages, 9 figures; references added, typos corrected. Invited contribution to the Heraeus-Seminar "Hundred Years of Gauge Theory", 30 July - 3 August 2018, Physikzentrum Bad Honnef, organized by Silvia De Bianchi and Claus Kiefer. To appear in the proceedings "100 Years of Gauge Theory. Past, present and future perspectives" in the series `Fundamental Theories of Physics' (Springer)
References in corpus (31)
- Exact evolution equation for the effective potential
- The Standard Model Higgs boson as the inflaton
- Higgs inflation: consistency and generalisations
- Avoiding Dark Energy with 1/R Modifications of Gravity
- Inflation scenario via the Standard Model Higgs boson and LHC
- Power-counting and the Validity of the Classical Approximation During Inflation
- Conformal Symmetry and the Standard Model
- Quantum scale invariance, cosmological constant and hierarchy problem
- Cosmological implications of the Higgs mass measurement
- Higgs inflation at the critical point
- Higgs inflation still alive
- The lifetime of the electroweak vacuum and sensitivity to Planck scale physics
- Equivalence of the Einstein and Jordan frames
- Gravitational corrections to Standard Model vacuum decay
- Invariant quantities in the scalar-tensor theories of gravitation
- Frame-dependence of higher-order inflationary observables in scalar-tensor theories
- Probable or Improbable Universe? Correlating Electroweak Vacuum Instability with the Scale of Inflation
- One-loop divergences for gravity non-minimally coupled to a multiplet of scalar fields: calculation in the Jordan frame. I. The main results
- On the violent preheating in the mixed Higgs- inflationary model
- The Higgs Mass and the Scale of New Physics
- On gravitational and thermal corrections to vacuum decay
- (Higgs) vacuum decay during inflation
- Higgs Mass Bounds from Renormalization Flow for a Higgs-top-bottom model
- Frame Covariant Nonminimal Multifield Inflation
- Dynamical Emergence of Scalaron in Higgs Inflation
- Quantum scale symmetry
- Frame Covariance in Quantum Gravity
- Higgs- inflation -- full slow-roll study at tree-level
- Geometrized quantum Galileons
- Covariant one-loop quantum gravity and Higgs inflation
- Quantum gravitational corrections to the inflationary power spectra in scalar-tensor theories
Cited by in corpus (12)
- Reheating in Palatini inflationary models
- Scalaron-Higgs inflation reloaded: Higgs-dependent scalaron mass and primordial black hole dark matter
- The Higgs field and early universe cosmology: a (brief) review
- Discrepancy between cosmological and electroweak observables in Higgs Inflation
- Towards a unitary, renormalizable and ultraviolet-complete quantum theory of gravity
- Quantum Higgs Inflation
- Multi-field inflation from single-field models
- Testing time-delayed cosmology
- Modified Starobinsky inflation by the term
- The Effective Potential Originating from Swampland and the Non-trivial Brans-Dicke Coupling
- Fermionic wave functions and Grassmann fields as possible sources of dark energy
- Conflict between some higher-order curvature invariant terms