Radiative Plateau Inflation with Conformal Invariance: Dynamical Generation of Electroweak and Seesaw Scales
arXiv:2203.00677 · doi:10.1103/PhysRevD.106.055024
Abstract
We investigate a scale-invariant scenario where the Standard Model (SM) is supplemented with a dark scalar which has gauge \& Yukawa interactions, with the couplings and , respectively, leading to radiative plateau inflation at scale in the ultraviolet (UV), while dynamically generating the Electroweak and Seesaw scales \textit{á lá} Coleman-Weinberg in the infrared (IR). This is particularly achieved by implementing threshold corrections at an energy scale arising due to the presence of vector-like fermions. We show that implementing the inflationary observables makes the couplings solely dependent on the plateau scale , leaving us with only two independent parameters and . Within the theoretically consistent parameter space defined by , from the assumption of independent evolution of the dark sector couplings from the SM couplings and required for the realisation of inflationary \textit{plateau-like} behaviour of the potential around , where GeV is the reduced Planck mass, we identify the parameter space that is excluded by the current LHC results from the search for the heavy boson. For typical benchmark points in the viable parameter regions, we estimate the reheating temperature to be thus consistent with the standard Big Bang Nucleosynthesis (BBN) constraints. For typical benchmark points () we predict the scales of inflation to be GeV, GeV and GeV, respectively.
27 pages, 4 figures, Published in PRD
References in corpus (29)
- The Standard Model Higgs boson as the inflaton
- Gauge invariant MSSM inflaton
- Improved limits on the tensor-to-scalar ratio using BICEP and Planck
- A solution to the hierarchy problem from an almost decoupled hidden sector within a classically scale invariant theory
- A Delicate Universe
- The Minimal Scale Invariant Extension of the Standard Model
- Dark Matter from a Classically Scale-Invariant
- Dynamical generation of the weak and Dark Matter scales from strong interactions
- Embedding inflation into the Standard Model - more evidence for classical scale invariance
- Naturalness and Dimensional Transmutation in Classically Scale-Invariant Gravity
- Chaotic inflation, radiative corrections and precision cosmology
- Inflation in scale-invariant theories of gravity
- Light Dark Matter, Naturalness, and the Radiative Origin of the Electroweak Scale
- Dimensional Transmutation in Gravity and Cosmology
- Inflation and reheating in scale-invariant scalar-tensor gravity
- Small Field Polynomial Inflation: Reheating, Radiative Stability and Lower Bound
- Volume modulus inflection point inflation and the gravitino mass problem
- Warm Inflection
- Inflection-point Higgs Inflation
- Scale Invariant FIMP Miracle
- Probing the minimal model at future electron-positron colliders via the fermion pair-production channel
- Two-component scalar and fermionic dark matter candidates in a generic U model
- Non-local Non-Abelian Gauge Theory: Conformal Invariance and -function
- Inflationary Parameters in Renormalization Group Improved Theory
- Unified Emergence of Energy Scales and Cosmic Inflation
- Mass Gap in Infinite Derivative Non-local Higgs: Dyson-Schwinger Approach
- Strongly Coupled String-inspired Infinite Derivative Non-local Yang-Mills: Diluted Mass Gap
- Dynamical Inflection Point Inflation
- High Higgs excess as a signal of non-local QFT at the LHC
Cited by in corpus (6)
- Gravitational Wave Pathway to Testable Leptogenesis
- Testing scale-invariant inflation against cosmological data
- Inflation and primordial gravitational waves in scale-invariant quadratic gravity with Higgs
- eV Hubble Scale Inflation with Radiative Plateau: Very light Inflaton, Reheating & Dark Matter in B-L Extensions
- Conformal B-L and Pseudo-Goldstone Dark Matter
- Fate of the false vacuum in string-inspired nonlocal field theory