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相关论文: Time-Varying Fine-Structure Constant and Quantum S…

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We describe a rigorous construction, using matched asymptotic expansions, which establishes under very general conditions that local terrestrial and solar-system experiments will measure the effects of varying `constants' of Nature…

广义相对论与量子宇宙学 · 物理学 2011-07-19 Douglas J. Shaw , John D. Barrow

We present a class of models in which the coupling of the photon to an ultralight scalar field that has a time-dependent vacuum expectation value causes the fine structure constant to oscillate in time. The scalar field is assumed to…

高能物理 - 唯象学 · 物理学 2022-09-07 Dawid Brzeminski , Zackaria Chacko , Abhish Dev , Anson Hook

In this work we investigate the utility of using SNe Ia observations in constraining the cosmological parameters in BSBM theory where a scalar field is responsible for both fine structure constant variation and late time universe…

广义相对论与量子宇宙学 · 物理学 2015-06-04 H. Farajollahi , A. Salehi

It is considered that quasars evolve into normal galaxies by means of expansion of matter. The order of magnitude of the expansion velocity can be estimated. The Doppler shift caused by such expansion explains the supposed variation of the…

天体物理学 · 物理学 2007-05-23 Mario Everaldo de Souza

The structure formation in the local Universe is considered within the weak-field modification of General Relativity involving the cosmological constant. This approach enables to describe the dynamics of groups and clusters of galaxies, to…

广义相对论与量子宇宙学 · 物理学 2025-02-06 V. G. Gurzadyan

It has been widely believed that variability of the fine-structure constant alpha would imply detectable violations of the weak equivalence principle. This belief is not justified in general. It is put to rest here in the context of the…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Jacob D. Bekenstein

Cosmic strings are predicted by many field-theory models, and may have been formed at a symmetry-breaking transition early in the history of the universe, such as that associated with grand unification. They could have important…

高能物理 - 理论 · 物理学 2010-05-07 Edmund J. Copeland , T. W. B. Kibble

If the reported measurements of the time variation of the fine structure constant from observations of distant QSOs are correct, combined with the Oklo limit they would strongly constrain the class of the quintessence potential. If these…

高能物理 - 唯象学 · 物理学 2009-11-07 Takeshi Chiba , Kazunori Kohri

Many models of quintessence predict a time variation of the fundamental constants as well as a composition-dependent gravity like long-range force mediated by the cosmon. We present bounds for the cosmon coupling to matter and radiation…

高能物理 - 唯象学 · 物理学 2009-11-07 C. Wetterich

Higher-dimensional theories have the remarkable feature of predicting a time (and hence redshift) dependence of the `fundamental' four dimensional constants on cosmological timescales. In this paper we update the bounds on a possible…

Standard quantum field theory arguments predict an enormous cosmological constant. But what would this mean observationally? For a homogeneous universe the answer is clear, but if the universe is inhomogeneous at the Planck scale, the…

广义相对论与量子宇宙学 · 物理学 2025-10-30 Steven Carlip

We discuss the fundamemtal constants in the Standard Model of particle physics, in particular possible changes of these constants on the cosmological time scale. The Grand Unification of the observed strong, electromagnetic and weak…

高能物理 - 唯象学 · 物理学 2016-10-25 Harald Fritzsch

Cosmic (super)strings offer promising ways to test ideas about the early universe and physics at high energies. While in field theory constructions their tension is usually assumed to be constant (or at most slowly-varying), this is often…

高能物理 - 唯象学 · 物理学 2025-05-08 Filippo Revello , Gonzalo Villa

We argue that cosmic strings with high winding numbers generally form in first-order gauge symmetry breaking phase transitions, and we demonstrate this using computer simulations. These strings are heavier than single-winding strings and…

高能物理 - 唯象学 · 物理学 2007-05-23 M. Donaire , A. Rajantie

We investigate the cosmological consequences of a simple theory in which the electric charge $e$ is allowed to vary. The theory is locally gauge and Lorentz invariant, and satisfies general covariance. We find that in this theory the fine…

天体物理学 · 物理学 2014-10-13 H. B. Sandvik , J. D. Barrow , J. Magueijo

I briefly present some current theoretical motivations for time or space variations of the fundamental constants of nature and review current key observational results. I focus on the fine-structure constant, and particularly on…

天体物理学 · 物理学 2007-05-23 C. J. A. P. Martins

At the level of the Planck scale, the spacetime metric has to be considered a quantum variable. Conformal quantum fluctuations of the metric tensor are studied here. They lead to an extra term in the Einstein equations which can be…

天体物理学 · 物理学 2007-05-23 Alex H. Blin

We discuss experiments and observations aimed at testing the possible space-time variability of fundamental physical constants, predicted by the modern theory. Specifically, we consider two of the dimensionless physical parameters which are…

原子物理 · 物理学 2007-05-23 D. A. Varshalovich , A. Y. Potekhin , A. V. Ivanchik

A numerical coincidence relating the values of the cosmological, gravitational and electromagnetic fine structure constants is presented and discussed in relation to the apparent anthropic fine-tuning of these three fundamental constants of…

广义相对论与量子宇宙学 · 物理学 2015-10-26 Laurence Eaves

Perhaps the cosmological constant really is huge at the Planck scale, but is "hidden" by Planck scale quantum fluctuations of spacetime. I briefly review this proposal and provide some evidence, coming from a simplified midisuperspace…

广义相对论与量子宇宙学 · 物理学 2021-12-06 S. Carlip