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For almost a century, the cosmological constant has been a mysterious object, in relation to both its origin and its very small value. By using a Bose-Einstein condensate analogue model for gravitational dynamics, we address here the…

广义相对论与量子宇宙学 · 物理学 2012-07-25 Stefano Finazzi , Stefano Liberati , Lorenzo Sindoni

The cosmological constant presents one of the most fascinating and confounding problems in physics. A straightforward, seemingly robust prediction of quantum mechanics and general relativity is that the vacuum energy gravitates. Therefore,…

高能物理 - 理论 · 物理学 2023-08-16 Suman Kumar Kundu , Arnab Pradhan , Carl Rosenzweig

Following fresh attempts to resolve the problem of the energy density of the vacuum, we reconsider the case where the cosmological constant is derived from a higher-dimensional version of general relativity, and interpret the…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Paul S. Wesson

The formalism to treat quantization and evolution of cosmological perturbations of multiple fluids is described. We first construct the Lagrangian for both the gravitational and matter parts, providing the necessary relevant variables and…

广义相对论与量子宇宙学 · 物理学 2016-02-01 Patrick Peter , Nelson Pinto-Neto , Sandro Dias Pinto Vitenti

There are now two cosmological constant problems: (i) why the vacuum energy is so small and (ii) why it comes to dominate at about the epoch of galaxy formation. Anthropic selection appears to be the only approach that can naturally resolve…

高能物理 - 理论 · 物理学 2007-06-20 Alexander Vilenkin

We explore the idea that quantum vacuum energy $\rho_{\rm vac} $ is at the origin of Gravity. We formulate a gravitational version of the electromagnetic Casimir effect, and provide an argument for how gravity can arise from $\rho_{\rm vac}…

高能物理 - 理论 · 物理学 2026-01-01 André LeClair

If quantum fields exist in extra compact dimensions, they will give rise to a quantum vacuum or Casimir energy. That vacuum energy will manifest itself as a cosmological constant. The fact that supernova and cosmic microwave background data…

高能物理 - 理论 · 物理学 2014-12-10 Kimball A. Milton

A static non-singular 10-dimensional closed Friedmann universe of Planck size, filled with a perfect fluid with an equation of state with w = -2/3, can arise spontaneously by a quantum fluctuation from nothing in 11-dimensional spacetime. A…

广义相对论与量子宇宙学 · 物理学 2009-11-11 T. R. Mongan

When the vacuum fluctuation pressure is calculated directly from fundamental principles of quantum field theory, in the same manner as vacuum fluctuation energy density is commonly calculated, one finds it is not equal to the negative of…

综合物理 · 物理学 2007-11-05 Robert D. Klauber

Wheeler's conjectured "spacetime foam" -- large quantum fluctuations of spacetime at the Planck scale -- could have important implications for quantum gravity, perhaps even explaining why the cosmological constant seems so small. Here I…

广义相对论与量子宇宙学 · 物理学 2022-01-05 S. Carlip

The macroscopic behavior of many physical systems can be approximately described by classical quantities. However, quantum theory demands the existence of omnipresent quantum fluctuations on top of this classical background -- which, albeit…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Ralf Schützhold

In quantum theory the vacuum is defined as a state of minimum energy that is devoid of particles but still not completely empty. It is perhaps more surprising that its definition depends on the geometry of the system and on the trajectory…

量子物理 · 物理学 2016-05-04 F. Intravaia

A class of $k$-Essence cosmological models, with a power law kinetic term, is quantised in the mini-superspace. It is shown that for a specific configuration, corresponding to a pressureless fluid, a Schr\"odinger-type equation is obtained…

广义相对论与量子宇宙学 · 物理学 2016-12-28 C. R. Almeida , J. C. Fabris , F. Sbisá , Y. Tavakoli

Increasing improvements in the independent determinations of the Hubble constant and the age of the universe now seem to indicate that we need a small non-vanishing cosmological constant to make the two independent observations consistent…

高能物理 - 唯象学 · 物理学 2009-10-28 Anupam Singh

Dynamical vacuum energy or quintessence, a slowly varying and spatially inhomogeneous component of the energy density with negative pressure, is currently consistent with the observational data. One potential difficulty with the idea of…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Takeshi Chiba

The standard model of the universe is further completed back in time before inflation in agreement with observations, classical-quantum gravity duality and quantum space-time. Quantum vacuum energy bends the space-time and produces a…

综合物理 · 物理学 2022-04-25 Norma G. Sanchez

Some form of missing energy may account for the difference between the observed cosmic matter density and the critical density. Two leading candidates are a cosmological constant and quintessence (a time-varying, inhomogenous component with…

天体物理学 · 物理学 2009-09-15 Greg Huey , Limin Wang , R. Dave , R. R. Caldwell , Paul J. Steinhardt

Arguments are gived for the plausibility that quantum mechanics is a stochastic theory and that many quantum phenomena derive from the existence of a real noise consisting of vacuum fluctuations of all fundamental fields existing in nature.…

量子物理 · 物理学 2016-09-26 Emilio Santos

Rising to Mach, the problem of establishing the unity of the physical essence of the Universe on all space-time scales of its evolution is, apparently, one of the main problems in contemporary epistemology. The issues are primarily related…

综合物理 · 物理学 2019-02-13 Serge F. Timashev

Motivated by some recent speculative attempts to model the dark energy, scalar fields with negative kinetic energy coupled to gravity without a cosmological constant are considered. It is shown that in the presence of an ordinary fluid, any…

高能物理 - 理论 · 物理学 2007-05-23 G. W. Gibbons