通过希格斯-膨胀子耦合产生不同光速的机制:理论和宇宙学应用

IF 4.2 2区 物理与天体物理 Q2 PHYSICS, PARTICLES & FIELDS
Hoang Ky Nguyen
{"title":"通过希格斯-膨胀子耦合产生不同光速的机制:理论和宇宙学应用","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":"{\"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}","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

摘要

我们探讨了一类尺度不变的作用,它允许希格斯场\(\Phi \)通过\(\chi ^{2}\,\Phi ^{\dagger }\Phi \)项与背景时空的膨胀场\(\chi \)相互作用。在自发规范对称破断时,希格斯场的真空期望值(VEV)与\(\chi \)成正比。虽然这种联系传统上被用来使普朗克质量和粒子质量依赖于\(\chi \),但我们提出了一种替代机制:希格斯VEV将用于构建普朗克作用量子\(\hbar \)和光速c。具体来说,在时空流形上给定点\(x^{*}\)附近的每个开放集都配备了一个格拉斯哥-温伯格-萨拉姆作用的复制品,其有效值分别为\(\hbar _{*}\propto \chi ^{-1/2}(x^{*})\)和\(c_{*}\propto \chi ^{1/2}(x^{*})\)的\(\hbar _{*}\)和\(c_{*}\),导致这些“基本常数”随着动力场\(\chi \)而变化。此外,在\(x^{*}\)周围的每个开放集中,流行值\(\chi (x^{*})\)决定了该区域内发生的物理过程的长度和时间尺度,如\(l\propto \chi ^{-1}(x^{*})\)和\(\tau \propto \chi ^{-3/2}(x^{*})\)。这导致时钟的速率和杆的长度之间的各向异性关系\(\tau ^{-1}\propto l^{-3/2}\),导致一组独特的新颖的物理现象。对于晚时间宇宙学,c沿着光波从遥远的超新星到地球上的观测者的轨迹的变化需要修改lema 3红移公式,哈勃定律和光度距离红移关系。这些修改能够:(1)通过在膨胀的爱因斯坦-德西特宇宙中光速的下降来计算Ia型超新星的万神殿目录,从而避免了对暗能量的需要;(2)复兴了Blanchard-Douspis-Rowan-Robinson-Sarkar的CMB功率谱分析方法,该方法绕过暗能量;(3)在不需要动态暗能量分量的情况下求解\(H_{0}\)张力。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A mechanism to generate varying speed of light via Higgs-dilaton coupling: theory and cosmological applications

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.

求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
The European Physical Journal C
The European Physical Journal C 物理-物理:粒子与场物理
CiteScore
8.10
自引率
15.90%
发文量
1008
审稿时长
2-4 weeks
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.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信