{"title":"超轻膨胀振荡和宇宙常数","authors":"Abdellah Touati","doi":"10.1140/epjc/s10052-025-14846-y","DOIUrl":null,"url":null,"abstract":"<div><p>In this work, we present a model predicting the emergence of a cosmological constant from ultralight dilaton oscillations. We begin by introducing the gravitational action in the context of two-dimensional scalar-tensor gravity, where the action of the gravitational field with an arbitrary dilaton potential is derived. The equations of motion for the gravitational field are then formulated and solved. Finally, we propose a model where the energy of the oscillating dilaton particle-like leads to the appearance of a cosmological term in the metric. Our results indicate that the energy associated with the oscillations of a dilaton particle-like contributes to the emergence of a cosmological term in the Schwarzschild metric. This term is interpreted as a cosmological constant, suggesting that the oscillatory energy of the dilaton could be considered a potential candidate for explaining dark energy. Furthermore, we constrain the dilaton mass to be on the order of <span>\\(m_\\varPhi \\sim 10^{-13}\\)</span> eV/<span>\\(c^2\\)</span>, consistent with ultralight dark matter models.</p></div>","PeriodicalId":788,"journal":{"name":"The European Physical Journal C","volume":"85 10","pages":""},"PeriodicalIF":4.8000,"publicationDate":"2025-10-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1140/epjc/s10052-025-14846-y.pdf","citationCount":"0","resultStr":"{\"title\":\"Ultralight dilaton oscillations and the cosmological constant\",\"authors\":\"Abdellah Touati\",\"doi\":\"10.1140/epjc/s10052-025-14846-y\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>In this work, we present a model predicting the emergence of a cosmological constant from ultralight dilaton oscillations. We begin by introducing the gravitational action in the context of two-dimensional scalar-tensor gravity, where the action of the gravitational field with an arbitrary dilaton potential is derived. The equations of motion for the gravitational field are then formulated and solved. Finally, we propose a model where the energy of the oscillating dilaton particle-like leads to the appearance of a cosmological term in the metric. Our results indicate that the energy associated with the oscillations of a dilaton particle-like contributes to the emergence of a cosmological term in the Schwarzschild metric. This term is interpreted as a cosmological constant, suggesting that the oscillatory energy of the dilaton could be considered a potential candidate for explaining dark energy. Furthermore, we constrain the dilaton mass to be on the order of <span>\\\\(m_\\\\varPhi \\\\sim 10^{-13}\\\\)</span> eV/<span>\\\\(c^2\\\\)</span>, consistent with ultralight dark matter models.</p></div>\",\"PeriodicalId\":788,\"journal\":{\"name\":\"The European Physical Journal C\",\"volume\":\"85 10\",\"pages\":\"\"},\"PeriodicalIF\":4.8000,\"publicationDate\":\"2025-10-09\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://link.springer.com/content/pdf/10.1140/epjc/s10052-025-14846-y.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/s10052-025-14846-y\",\"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/s10052-025-14846-y","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}
Ultralight dilaton oscillations and the cosmological constant
In this work, we present a model predicting the emergence of a cosmological constant from ultralight dilaton oscillations. We begin by introducing the gravitational action in the context of two-dimensional scalar-tensor gravity, where the action of the gravitational field with an arbitrary dilaton potential is derived. The equations of motion for the gravitational field are then formulated and solved. Finally, we propose a model where the energy of the oscillating dilaton particle-like leads to the appearance of a cosmological term in the metric. Our results indicate that the energy associated with the oscillations of a dilaton particle-like contributes to the emergence of a cosmological term in the Schwarzschild metric. This term is interpreted as a cosmological constant, suggesting that the oscillatory energy of the dilaton could be considered a potential candidate for explaining dark energy. Furthermore, we constrain the dilaton mass to be on the order of \(m_\varPhi \sim 10^{-13}\) eV/\(c^2\), consistent with ultralight dark matter models.
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.