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The Standard Model of particle physics and the theory of General Relativity (GR) currently provide a good description of almost all phenomena of particle physics and gravitation that have received controlled experimental tests. However, the…

原子物理 · 物理学 2009-01-23 Thomas Dent

The effect of fractal space time of the quantum particles on the variation of the fine structure constant $\alpha$ has been studied. The variation of fine structure constant has been investigated around De Broglie length $\lambda$ and…

宇宙学与河外天体物理 · 物理学 2013-09-05 A. Bhattacharya , A. Chandra , B. Chakrabarti

Since the public release of Planck data, several attempts have been made to explain the observed small tensions with other data-sets, most of them involving an extension of the {\Lambda}CDM Model. We try here an alternative approach to the…

宇宙学与河外天体物理 · 物理学 2015-06-18 Benjamin Audren

The standard cosmological model determined from the accurate cosmic microwave background measurements made by the Planck satellite implies a value of the Hubble constant $H_0$ that is $4.2$ standard deviations lower than the one determined…

宇宙学与河外天体物理 · 物理学 2020-11-04 Karsten Jedamzik , Levon Pogosian

Any time variation in the fine-structure constant alters the ionization history of the universe and therefore changes the pattern of cosmic microwave background fluctuations. We calculate the changes in the spectrum of these fluctuations as…

天体物理学 · 物理学 2009-10-31 Manoj Kaplinghat , Robert J. Scherrer , Michael S. Turner

We study the role of fundamental constants in an updated recombination scenario. We focus on the time variation of the fine structure constant, and the electron mass in the early Universe, and put bounds on these quantities by using data…

天体物理学 · 物理学 2008-10-31 Claudia G. Scóccola , Susana. J. Landau , Hector Vucetich

The idea that the vacuum energy density $\rho_{\Lambda}$ could be time dependent is a most reasonable one in the expanding Universe; in fact, much more reasonable than just a rigid cosmological constant for the entire cosmic history. Being…

广义相对论与量子宇宙学 · 物理学 2015-07-08 Harald Fritzsch , Joan Sola

Astrophysical indications that the fine structure constant has undergone a small time variation during the cosmological evolution are discussed within the framework of the standard model of the electroweak and strong interactions and of…

高能物理 - 唯象学 · 物理学 2009-11-07 H. Fritzsch

We study the $\Lambda(\alpha)$CDM models with $\Lambda(\alpha)$ being a function of the time-varying fine structure constant $\alpha$. We give a close look at the constraints on two specific $\Lambda(\alpha)$CDM models with one and two…

宇宙学与河外天体物理 · 物理学 2018-09-13 Jin-Jun Zhang , Lu Yin , Chao-Qiang Geng

A phenomenological model is proposed to explain the recent observed cosmological variation of the fine structure constant as an effect of the quantum vacuum, assuming a flat universe with cosmological constant $\Lambda$ in the cases…

天体物理学 · 物理学 2010-12-17 Antonio F. Rañada

The simplest cosmological model ($\Lambda$CDM) is well-known to suffer from the Hubble tension, namely an almost $5 \sigma$ discrepancy between the (model-based) early-time determination of the Hubble constant $H_0$ and its late-time (and…

宇宙学与河外天体物理 · 物理学 2023-10-06 Darshan Kumar , Debajyoti Choudhury , Debottam Nandi

We report on constraints to the cosmological jerk parameter ($j$) and to possible variability of the fine-structure constant ($\Delta \alpha/\alpha$) based on stochastic quintessence models of dark energy, discussed by Chongchitnan and…

宇宙学与河外天体物理 · 物理学 2016-03-23 Christine C. Dantas , Andre L. B. Ribeiro

The idea of possible time or space variations of the `fundamental' constants of nature, although not new, is only now beginning to be actively considered by large numbers of researchers in the particle physics, cosmology and astrophysics…

天体物理学 · 物理学 2009-11-07 C. J. A. P. Martins

The values of the fundamental constants such as $\mu = m_P/m_e$, the proton to electron mass ratio and $\alpha$, the fine structure constant, are sensitive to the product $\sqrt{\zeta_x^2(w+1)}$ where $\zeta_x$ is a coupling constant…

宇宙学与河外天体物理 · 物理学 2013-12-19 Rodger I. Thompson

The constraints on the time variation of the fine structure constant at recombination epoch relative to its present value, $\Delta\alpha/\alpha \equiv (\alpha_{\mathrm{rec}} - \alpha_{\mathrm{now}})/\alpha_{\mathrm{now}}$, are obtained from…

天体物理学 · 物理学 2014-11-18 Masahiro Nakashima , Ryo Nagata , Jun'ichi Yokoyama

Using a gauge-invariant formalism we derive and solve the perturbed cosmological equations for the BSBM theory of varying fine structure 'constant'. We calculate the time evolution of inhomogeneous perturbations of the fine structure…

广义相对论与量子宇宙学 · 物理学 2009-11-07 John D. Barrow , D. F. Mota

We study the spontaneous baryogenesis scenario in the early universe for three different frameworks of varying constants theories. We replace the constants by dynamical scalar fields playing the role of thermions. We first obtain the…

高能物理 - 理论 · 物理学 2019-03-27 Katarzyna Leszczynska , Mariusz P. Dabrowski , Tomasz Denkiewicz

The principal component analysis (PCA), a mathematical tool commonly used in statistics, has recently been employed to interpret the $p_T$-dependent fluctuations of harmonic flow $v_n$ in terms of leading and subleading flow modes in heavy…

核实验 · 物理学 2020-08-26 Ziming Liu , Arabinda Behera , Huichao Song , Jiangyong Jia

Searching for variations of nature's fundamental constants is a crucial step in our quest to go beyond our current standard model of fundamental physics. If they exist, such variations will be very likely driven by the existence of a new…

We compute the time variation of the fundamental constants (such as the ratio of the proton mass to the electron mass, the strong coupling constant, the fine structure constant and Newton's constant) within the context of the so-called…

高能物理 - 唯象学 · 物理学 2017-04-03 Harald Fritzsch , Joan Sola , Rafael C. Nunes