{"title":"A mechanism to generate varying speed of light via Higgs-dilaton coupling: theory and cosmological applications","authors":"Hoang Ky Nguyen","doi":"10.1140/epjc/s10052-025-14082-4","DOIUrl":null,"url":null,"abstract":"<div><p>We probe into a class of scale-invariant actions, which allow the Higgs field <span>\\(\\Phi \\)</span> to interact with a dilaton field <span>\\(\\chi \\)</span> of the background spacetime through the term <span>\\(\\chi ^{2}\\,\\Phi ^{\\dagger }\\Phi \\)</span>. Upon spontaneous gauge symmetry breaking, the vacuum expectation value (VEV) of the Higgs field becomes proportional to <span>\\(\\chi \\)</span>. Although this linkage is traditionally employed to make the Planck mass and particle masses dependent on <span>\\(\\chi \\)</span>, we present an <i>alternative</i> mechanism: the Higgs VEV will be used to <i>construct</i> Planck’s quantum of action <span>\\(\\hbar \\)</span> and speed of light <i>c</i>. Specifically, each open set vicinity of a given point <span>\\(x^{*}\\)</span> on the spacetime manifold is equipped with a replica of the Glashow–Weinberg–Salam action operating with <i>its own effective values of </i><span>\\(\\hbar _{*}\\)</span> <i>and </i><span>\\(c_{*}\\)</span> per <span>\\(\\hbar _{*}\\propto \\chi ^{-1/2}(x^{*})\\)</span> and <span>\\(c_{*}\\propto \\chi ^{1/2}(x^{*})\\)</span>, causing these “fundamental constants” to vary alongside the dynamical field <span>\\(\\chi \\)</span>. Moreover, in each open set around <span>\\(x^{*}\\)</span>, the prevailing value <span>\\(\\chi (x^{*})\\)</span> determines the length and time scales for physical processes occurring in this region as <span>\\(l\\propto \\chi ^{-1}(x^{*})\\)</span> and <span>\\(\\tau \\propto \\chi ^{-3/2}(x^{*})\\)</span>. This leads to an <i>anisotropic</i> relation <span>\\(\\tau ^{-1}\\propto l^{-3/2}\\)</span> between the rate of clocks and the length of rods, resulting in a distinct set of novel physical phenomena. For late-time cosmology, the variation of <i>c</i> along the trajectory of light waves from distant supernovae towards the Earth-based observer necessitates modifications to the Lemaître redshift formula, the Hubble law, and the luminosity distance–redshift relation. These modifications are capable of: (1) Accounting for the Pantheon Catalog of Type Ia supernovae <i>through a declining speed of light in an expanding Einstein–de Sitter universe</i>, thus avoiding the need for dark energy; (2) Revitalizing Blanchard–Douspis–Rowan-Robinson–Sarkar’s CMB power spectrum analysis that bypassed dark energy; and (3) Resolving the <span>\\(H_{0}\\)</span> tension without requiring a dynamical dark energy component.</p></div>","PeriodicalId":788,"journal":{"name":"The European Physical Journal C","volume":"85 4","pages":""},"PeriodicalIF":4.2000,"publicationDate":"2025-04-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1140/epjc/s10052-025-14082-4.pdf","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"The European Physical Journal C","FirstCategoryId":"4","ListUrlMain":"https://link.springer.com/article/10.1140/epjc/s10052-025-14082-4","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"PHYSICS, PARTICLES & FIELDS","Score":null,"Total":0}
引用次数: 0
Abstract
We probe into a class of scale-invariant actions, which allow the Higgs field \(\Phi \) to interact with a dilaton field \(\chi \) of the background spacetime through the term \(\chi ^{2}\,\Phi ^{\dagger }\Phi \). Upon spontaneous gauge symmetry breaking, the vacuum expectation value (VEV) of the Higgs field becomes proportional to \(\chi \). Although this linkage is traditionally employed to make the Planck mass and particle masses dependent on \(\chi \), we present an alternative mechanism: the Higgs VEV will be used to construct Planck’s quantum of action \(\hbar \) and speed of light c. Specifically, each open set vicinity of a given point \(x^{*}\) on the spacetime manifold is equipped with a replica of the Glashow–Weinberg–Salam action operating with its own effective values of \(\hbar _{*}\)and \(c_{*}\) per \(\hbar _{*}\propto \chi ^{-1/2}(x^{*})\) and \(c_{*}\propto \chi ^{1/2}(x^{*})\), causing these “fundamental constants” to vary alongside the dynamical field \(\chi \). Moreover, in each open set around \(x^{*}\), the prevailing value \(\chi (x^{*})\) determines the length and time scales for physical processes occurring in this region as \(l\propto \chi ^{-1}(x^{*})\) and \(\tau \propto \chi ^{-3/2}(x^{*})\). This leads to an anisotropic relation \(\tau ^{-1}\propto l^{-3/2}\) between the rate of clocks and the length of rods, resulting in a distinct set of novel physical phenomena. For late-time cosmology, the variation of c along the trajectory of light waves from distant supernovae towards the Earth-based observer necessitates modifications to the Lemaître redshift formula, the Hubble law, and the luminosity distance–redshift relation. These modifications are capable of: (1) Accounting for the Pantheon Catalog of Type Ia supernovae through a declining speed of light in an expanding Einstein–de Sitter universe, thus avoiding the need for dark energy; (2) Revitalizing Blanchard–Douspis–Rowan-Robinson–Sarkar’s CMB power spectrum analysis that bypassed dark energy; and (3) Resolving the \(H_{0}\) tension without requiring a dynamical dark energy component.
期刊介绍:
Experimental Physics I: Accelerator Based High-Energy Physics
Hadron and lepton collider physics
Lepton-nucleon scattering
High-energy nuclear reactions
Standard model precision tests
Search for new physics beyond the standard model
Heavy flavour physics
Neutrino properties
Particle detector developments
Computational methods and analysis tools
Experimental Physics II: Astroparticle Physics
Dark matter searches
High-energy cosmic rays
Double beta decay
Long baseline neutrino experiments
Neutrino astronomy
Axions and other weakly interacting light particles
Gravitational waves and observational cosmology
Particle detector developments
Computational methods and analysis tools
Theoretical Physics I: Phenomenology of the Standard Model and Beyond
Electroweak interactions
Quantum chromo dynamics
Heavy quark physics and quark flavour mixing
Neutrino physics
Phenomenology of astro- and cosmoparticle physics
Meson spectroscopy and non-perturbative QCD
Low-energy effective field theories
Lattice field theory
High temperature QCD and heavy ion physics
Phenomenology of supersymmetric extensions of the SM
Phenomenology of non-supersymmetric extensions of the SM
Model building and alternative models of electroweak symmetry breaking
Flavour physics beyond the SM
Computational algorithms and tools...etc.