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Due to quantum fluctuations, spacetime is foamy on small scales. The degree of foaminess is found to be consistent with the holographic principle. One way to detect spacetime foam is to look for halos in the images of distant quasars.…

广义相对论与量子宇宙学 · 物理学 2009-05-01 Y. Jack Ng

Due to quantum fluctuations, spacetime is foamy on small scales. The degree of foaminess is found to be consistent with holography, a principle prefigured in the physics of black hole entropy. It has bearing on the ultimate accuracies of…

高能物理 - 理论 · 物理学 2015-05-13 Y. Jack Ng

Quantum fluctuations endow spacetime with a foamy texture. The degree of foaminess is dictated by blackhole physics to be of the holographic type. Applied to cosmology, the holographic foam model predicts the existence of dark energy with…

广义相对论与量子宇宙学 · 物理学 2021-02-10 Y. Jack Ng

Spacetime is foamy due to quantum fluctuations. Various gedanken experiments show that distances fluctuate by amounts consistent with the holographic principle, hence the name "holographic quantum foam" (HQF). One important prediction of…

广义相对论与量子宇宙学 · 物理学 2026-03-20 Eric Steinbring , Y. Jack Ng

Spacetime foam, also known as quantum foam, has its origin in quantum fluctuations of spacetime. Arguably it is the source of the holographic principle, which severely limits how densely information can be packed in space. Its physics is…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Y. Jack Ng , H. van Dam

Due to quantum fluctuations, spacetime is foamy on small scales. For maximum spatial resolution of the geometry of spacetime, the holographic model of spacetime foam stipulates that the uncertainty or fluctuation of distance $l$ is given,…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Michele Arzano , Thomas W. Kephart , Y. Jack Ng

Quantum foam, also known as spacetime foam, has its origin in quantum fluctuations of spacetime. Its physics is intimately linked to that of black holes and computation. Arguably it is the source of the holographic principle which severely…

广义相对论与量子宇宙学 · 物理学 2016-11-09 Y. Jack Ng

Due to quantum fluctuations, probed at small scales, spacetime is very complicated -- something akin in complexity to a turbulent froth which the late John Wheeler dubbed quantum foam, aka spacetime foam. Our recent work suggests that (1)…

广义相对论与量子宇宙学 · 物理学 2010-01-05 Y. Jack Ng

We investigate the origin of holographic dark energy models which were recently proposed to explain the dark energy-dominated universe. For this purpose, we introduce the spacetime foam uncertainty of $\delta l \ge l_{\rm…

广义相对论与量子宇宙学 · 物理学 2009-02-02 Yun Soo Myung , Min-Gyun Seo

Holographic dark energy models have been recently suggested which most clearly show that accelerating cosmology appears to be incompatible with mathematically consistent formulations of fundamental theories such as string/M theories. In…

天体物理学 · 物理学 2007-05-23 Pedro F. Gonzalez-Diaz

Spacetime foam manifests itself in a variety of ways. It has some attributes of a turbulent fluid. It is the source of the holographic principle. Cosmologically it may play a role in explaining why the energy density has the critical value,…

广义相对论与量子宇宙学 · 物理学 2011-02-24 Y. Jack Ng

The holographic dark energy model is obtained from a cosmological constant generated by generic quantum gravity effects giving a minimum length. By contrast, the usual bound for the energy density to be limited by the formation of a black…

高能物理 - 理论 · 物理学 2016-05-25 Horatiu Nastase

Spacetime is composed of a fluctuating arrangement of bubbles or loops called spacetime foam, or quantum foam. We use the holographic principle to deduce its structure, and show that the result is consistent with gedanken experiments…

广义相对论与量子宇宙学 · 物理学 2011-09-01 Y. Jack Ng

We use two simple independent gedankan experiments to show that the holographic principle can be understood intuitively as having its origin in the quantum fluctuations of spacetime. Applied to cosmology, this consideration leads to a…

广义相对论与量子宇宙学 · 物理学 2017-06-28 Y. Jack Ng

We aim at the construction of dark energy models without exotic matter but with a phantom-like equation of state (an effective phantom phase). The first model we consider is decaying vacuum cosmology where the fluctuations of the vacuum are…

高能物理 - 理论 · 物理学 2009-09-17 Emilio Elizalde , Shin'ichi Nojiri , Sergei D. Odintsov , Peng Wang

It is shown that the first law of thermodynamics and the holographic principle applied to an arbitrary large cosmic causal horizon naturally demand the zero cosmological constant and non-zero dynamical dark energy in the form of the…

高能物理 - 理论 · 物理学 2015-03-13 Jae-Weon Lee

By incorporating the holographic principle in a time-depending Lambda-term cosmology, new physical bounds on the arbitrary parameters of the model can be obtained. Considering then the dark energy as a purely geometric entity, for which no…

广义相对论与量子宇宙学 · 物理学 2009-11-11 J. P. Beltran Almeida , J. G. Pereira

Hawking's spacetime foam model predicts that due to quantum fluctuations, spacetime is filled with black hole like objects. We argue that Hawking's model implies a cosmological constant of the observed order and that it can also be used to…

广义相对论与量子宇宙学 · 物理学 2018-10-24 Benjamin Schulz

Using a new version of the holographic principle, a constant term was introduced, which conduces to the description of the standard cosmological LCDM model, and unifies under the same concept the dark matter and dark energy phenomena. The…

高能物理 - 理论 · 物理学 2011-02-03 L. N. Granda

Holographic dark energy (HDE) models, underlain by an effective quantum field theory (QFT) with a manifest UV/IR connection, have become a convincing candidate for the dark energy in the universe. On the other hand, the maximum number of…

广义相对论与量子宇宙学 · 物理学 2008-11-26 R. Horvat
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