超轻膨胀振荡和宇宙常数

IF 4.8 2区 物理与天体物理 Q2 PHYSICS, PARTICLES & FIELDS
Abdellah Touati
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引用次数: 0

摘要

在这项工作中,我们提出了一个模型,预测从超轻膨胀振荡中出现一个宇宙常数。我们首先在二维标量张量引力的背景下引入引力作用,推导了具有任意膨胀势的引力场的作用。然后建立并求解了引力场的运动方程。最后,我们提出了一个模型,其中振荡膨胀粒子的能量导致度规中出现一个宇宙学项。我们的结果表明,与类粒子膨胀子振荡相关的能量有助于在史瓦西度规中出现一个宇宙学项。这一项被解释为宇宙常数,表明膨胀子的振荡能量可以被认为是解释暗能量的潜在候选。此外,我们将膨胀质量限制在\(m_\varPhi \sim 10^{-13}\) eV/ \(c^2\)量级,与超轻暗物质模型一致。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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.

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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.
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