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相关论文: QED Vacuum Loops and Dark Energy

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The evolution of a scalar field is explored taking into account the presence of a background fluid in a positively curved Universe in the framework of loop quantum cosmology. Though the mechanism that provides the initial conditions for…

天体物理学 · 物理学 2009-11-13 N. J. Nunes

We propose a model in which there exists a real scalar field $q$ satisfying a condition $\dot{q} =MH$ and its energy density is given by $(1/2)\dot{q}^2+V(q)$, where $H$ is the Hubble parameter ($H=\dot{a}/a$) and $M$ is a mass scale…

宇宙学与河外天体物理 · 物理学 2012-07-03 Aiichi Iwazaki

We show that quantum fluctuations of electromagnetic fields induce an additional zero-point energy in solids, which scales with the volume. For insulators, the zero-point energy density is proportional to quantum fluctuation of electric…

介观与纳米尺度物理 · 物理学 2026-02-10 Yugo Onishi , Liang Fu

The origin of the observed dark energy could be explained entirely within the standard model, with no new fields required. We show how the low-energy sector of the chiral QCD Lagrangian, once embedded in a non-trivial spacetime, gives rise…

宇宙学与河外天体物理 · 物理学 2015-03-13 Federico R. Urban , Ariel R. Zhitnitsky

We study the influence of a vacuum instability on the effective energy-momentum tensor (EMT) of QED, in the presence of a quasiconstant external electric field, by means of the relevant Green functions. In the case when the initial vacuum,…

高能物理 - 理论 · 物理学 2009-11-11 S. P. Gavrilov

Quantum gravity, as a fundamental theory of space-time, is expected to reveal how the universe may have started, perhaps during or before an inflationary epoch. It may then leave a potentially observable (but probably minuscule) trace in…

广义相对论与量子宇宙学 · 物理学 2015-12-17 Martin Bojowald

We suppose that vacuum is filled with a kind of continuously distributed matter which may be called the $\Omega(1)$ substratum, or the electromagnetic aether. Suppose that the time scale of a macroscopic observer is very large compares to…

综合物理 · 物理学 2021-01-25 Xiao-Song Wang

We give a well-motivated explanation for the origin of dark energy, claiming that it arises from a small residual negative scalar-curvature present even in empty spacetime. The vacuum has this residual curvature because spacetime is…

数学物理 · 物理学 2012-08-16 Aaron D. Trout

In this talk, I will present highlights of a recent model of dark energy and dark matter in which the present universe is ``trapped'' in a {\em false vacuum} described by the potential of an axion-like scalar field (the acceleron) which is…

天体物理学 · 物理学 2008-11-26 P. Q. Hung

Physics invites the idea that space contains energy whose gravitational effect approximates that of Einstein's cosmological constant, Lambda; nowadays the concept is termed dark energy or quintessence. Physics also suggests the dark energy…

天体物理学 · 物理学 2008-11-26 P. J. E. Peebles , Bharat Ratra

In a recent model of dark energy (with several phenomenological consequences), the universe is assumed to be trapped in a false vacuum with an energy density of the order of (10^{-3} eV)^4, mimicking the presently successful $\Lambda CDM$…

高能物理 - 唯象学 · 物理学 2007-11-29 P. Q. Hung

Quarks play an active role in shaping the QCD vacuum structure. Being dual carriers of both `color' and `electric' charges they also respond to externally applied electromagnetic fields. Thus, in principle, the vacuum of strong interactions…

高能物理 - 唯象学 · 物理学 2007-05-23 Johann Rafelski , H. -Thomas Elze

A new approach to generalised Casimir type of problems is derived within the context of renormalisable quantum field theory (QFT). We study the simplest case of a massive fluctuating boson field coupled to a time-independent background…

高能物理 - 理论 · 物理学 2007-05-23 Markus Quandt

We obtain a magnetically charged regular black hole in general relativity. The source to the Einstein field equations is nonlinear electrodynamic field in a physically reasonable model of nonlinear electrodynamics (NED). "Physically" here…

广义相对论与量子宇宙学 · 物理学 2015-09-21 Meng-Sen Ma

Various TeVeS-inspired and f(R)-inspired theories of gravity have added an interesting twist to the search for dark matter and vacuum energy, modifying the landscape of astrophysics day by day. These theories can be together called a {\bf…

天体物理学 · 物理学 2009-06-23 HongSheng Zhao

The Veneziano ghost field has been proposed as an alternative source of dark energy whose energy density is consistent with the cosmological observations. In this model, the energy density of QCD ghost field is expressed in terms of QCD…

高能物理 - 唯象学 · 物理学 2016-05-18 K. Azizi , N. Katirci

In the cosmological context an effective quantum field theory describing the behavior of visible matter in the universe is characterized with its inherent UV cutoff and also with an IR scale that is set by the cosmological (particle)…

高能物理 - 唯象学 · 物理学 2008-11-26 Michael Maziashvili

We present a mechanism for the emergence of cosmic acceleration within the mean-field approximation of Group Field Theory models of quantum gravity. Depending on the interaction type, the resulting cosmological dynamics can either feature a…

广义相对论与量子宇宙学 · 物理学 2025-12-15 Luca Marchetti , Tom R. Ladstätter , Daniele Oriti

Empirical theories of Dark Matter like MOND gravity and of Dark Energy like f(R) gravity were motivated by astronomical data. But could these theories be branches rooted from a more general hence natural framework? Here we propose the…

天体物理学 · 物理学 2015-05-13 HongSheng Zhao , Baojiu Li

We propose the pure natural quintessential inflation model which is motivated by Witten's conjecture, where the axion couples to pure Yang-Mills $SU(N)$ gauge field at large N limit. This modifies the standard cosine potential which is…

高能物理 - 唯象学 · 物理学 2020-08-05 Selvaganapathy J
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