A Cosmological Reconstruction of the Higgs Vacuum Expectation Value
Soumya Chakrabarti, Anagha V, Selva Ganesh, Vivek Menon

TL;DR
This paper proposes a toy cosmological model where a Higgs-like scalar field causes cosmic acceleration and predicts variations in fundamental constants, linking particle physics with cosmological observations.
Contribution
It introduces a model with a self-interacting scalar field that drives cosmic acceleration and predicts observable variations in the proton-to-electron mass ratio over cosmic time.
Findings
The model predicts a variation in $mma$ consistent with observational data.
Cosmological reconstruction using jerk parameter supports the model.
Comparison with atomic clock data constrains the scalar field dynamics.
Abstract
We present a simple toy model of cosmic acceleration driven purely by a self-interacting scalar field embedded in theory of grand unification. The scalar self-interaction is Higgs-like and provokes a spontaneous symmetry breaking. The coefficient of the quadratic term in the self-interaction potential has an evolution and it leads to a cosmic variation of proton-to-electron mass ratio, . We perform a cosmological reconstruction from the kinematic parameter jerk and discuss a few cosmological consequences of the theory. We also compare the theoretically calculated variation with the observations of molecular absorption spectra from Cesium Atomic Clock data.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Particle physics theoretical and experimental studies · Relativity and Gravitational Theory
