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相关论文: Dark energy and particle mixing

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A model for a flat homogeneous and isotropic Universe composed of dark energy, dark matter, neutrinos, radiation and baryons is analyzed. The fields of dark matter and neutrinos are supposed to interact with the dark energy. The dark energy…

广义相对论与量子宇宙学 · 物理学 2008-11-26 G. M. Kremer

We have found a mechanism which regulates the dark energy in our universe. With an emergent conformal symmetry, the dark energy density is regulated to the order of a conformal anomaly parameter in the conformally coupled gravity. In the…

广义相对论与量子宇宙学 · 物理学 2013-08-30 Yongsung Yoon

In this paper, we give a conceptual explanation of dark energy as a small negative residual scalar curvature present even in empty spacetime. This curvature ultimately results from postulating a discrete spacetime geometry, very closely…

数学物理 · 物理学 2012-08-16 Aaron Trout

The traditional "explanation" for the observed acceleration of the universe is the existence of a positive cosmological constant. However, this can hardly be a truly convincing explanation, as an expanding universe is not expected to have a…

广义相对论与量子宇宙学 · 物理学 2015-06-22 Joan Sola

The Dark Sector is described by an additional barotropic fluid which evolves adiabatically during the universe's history and whose adiabatic exponent $\gamma$ is derived from the standard definitions of specific heats. Although in general…

广义相对论与量子宇宙学 · 物理学 2016-11-02 Peter K. S. Dunsby , Orlando Luongo , Lorenzo Reverberi

It has been suggested that the dark energy that explains the observed accelerating expansion of the universe may arise due to the contribution to the vacuum energy of the QCD ghost in a time-dependent background. The argument uses a…

宇宙学与河外天体物理 · 物理学 2011-01-27 Nobuyoshi Ohta

Dark energy appears to be the dominant component of the physical Universe, yet there is no persuasive theoretical explanation for its existence or magnitude. The acceleration of the Universe is, along with dark matter, the observed…

We revise the dynamics of interacting vector-like dark energy, a theoretical framework proposed to explain the accelerated expansion of the universe. By investigating the interaction between vector-like dark energy and dark matter, we…

广义相对论与量子宇宙学 · 物理学 2024-03-29 Carlos Rodriguez-Benites , Manuel Gonzalez-Espinoza , Giovanni Otalora , Manuel Alva-Morales

Constantly accumulating observational data continue to confirm that about 70% of the energy density today consists of dark energy responsible for the accelerated expansion of the Universe. We present recent observational bounds on dark…

宇宙学与河外天体物理 · 物理学 2013-11-12 Shinji Tsujikawa

It is a puzzle why the densities of dark matter and dark energy are nearly equal today when they scale so differently during the expansion of the universe. This conundrum may be solved if there is a coupling between the two dark sectors. In…

高能物理 - 唯象学 · 物理学 2009-07-09 D. Comelli , M. Pietroni , A. Riotto

The dominance of dark energy in the universe has necessitated the introduction of a repulsive gravity source to make q0 negative. The models for dark energy range from a simple lambda-term to quintessence, Chaplygin gas, etc. We look at the…

综合物理 · 物理学 2011-09-12 C. Sivaram , Kenath Arun , R. Nagaraja

A web of interlocking observations has established that the expansion of the Universe is speeding up and not slowing, revealing the presence of some form of repulsive gravity. Within the context of general relativity the cause of cosmic…

天体物理学 · 物理学 2008-11-26 Michael S. Turner , Dragan Huterer

We point out that dark matter and dark energy arise naturally in a recently proposed model of combinatorial quantum gravity. Dark energy is due to the ground-state curvature at finite coupling, dark matter arises from allotropy in the…

广义相对论与量子宇宙学 · 物理学 2024-09-17 Carlo A. Trugenberger

We have derived the quantum vacuum pressure P_vac as a primary entity, removing a trivial and a gauge terms from the cosmological constant-like part (the zeroth term) of the effective action for a free matter field. The quantum vacuum…

广义相对论与量子宇宙学 · 物理学 2014-11-20 Bogusław Broda , Michał Szanecki

The quartic-divergent vacuum energy poses an ultraviolet (UV) challenge (the cosmological constant problem) in probing the nature of dark energy. Here we try to evaluate the contribution of the vacuum energy to dark energy with a method of…

高能物理 - 唯象学 · 物理学 2025-12-25 Lian-Bao Jia

We demonstrate that a scalar field is unable to reverse its direction of motion while continuously exchanging energy with another fluid. If the rate of transfer is modulated by the scalar's acceleration, the field can undergo a rapid…

宇宙学与河外天体物理 · 物理学 2019-04-15 Fergus Simpson , Raul Jimenez , Carlos Pena-Garay , Licia Verde

Dark and baryonic matter contribute comparable energy density to the present Universe. The dark matter may also be responsible for the cosmic positron/electron excesses. We connect these phenomena with Dirac seesaw for neutrino masses. In…

高能物理 - 唯象学 · 物理学 2009-10-29 Pei-Hong Gu , Utpal Sarkar , Xinmin Zhang

A QED-based symmetry breaking/bootstrap mechanism, appearing at sufficiently small space-time distances, is suggested as an explanation for the vacuum energy that furnished the initial impulse for Inflation, and continues on, to the present…

高能物理 - 理论 · 物理学 2015-03-19 H. M. Fried , Y. Gabellini

The recent study on the the 6-year up-going muon neutrinos by the IceCube Collaboration support the hypothesis of a two-component scenario explaining the diffuse TeV-PeV neutrino flux. Once a hard astrophysical power-law is considered, an…

高能物理 - 唯象学 · 物理学 2018-11-14 Marco Chianese

Adopting the hypothesis about the exact cancellation of vacuum condensates contributions to the ground state energy in particle physics to the leading order in graviton-mediated interactions, we argue that the observable cosmological…

广义相对论与量子宇宙学 · 物理学 2013-06-26 Roman Pasechnik , Vitaly Beylin , Grigory Vereshkov