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相关论文: Dark energy and particle mixing

200 篇论文

The discovery ten years ago that the expansion of the Universe is accelerating put in place the present cosmological model, in which the Universe is composed of 4% baryons, 20% dark matter, and 76% dark energy. Yet the underlying cause of…

宇宙学与河外天体物理 · 物理学 2009-04-17 Joshua A. Frieman

We study the vacuum condensate characterizing many physical phenomena. We show that such a condensate may leads to non-trivial components of the dark energy and of the dark matter and may induces the spontaneous supersymmetry breaking, in a…

高能物理 - 理论 · 物理学 2019-05-23 Antonio Capolupo

We present cosmological perturbation theory in neutrino probe interacting dark-energy models, and calculate cosmic microwave background anisotropies and matter power spectrum. In these models, the evolution of the mass of neutrinos is…

高能物理 - 唯象学 · 物理学 2008-11-26 Yong-Yeon Keum

Dark energy and dark matter are the dominant sources in the evolution of the late universe. They are currently only indirectly detected via their gravitational effects, and there could be a coupling between them without violating…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Christian G. Boehmer , Gabriela Caldera-Cabral , Ruth Lazkoz , Roy Maartens

We show that when a dark abelian gauge sector and SU$(2)_{L}$ kinetically mix it necessarily generates a relation between the kinetic mixing strength and the mass of the mediating particle. Remarkably, this correspondence maps the weak…

高能物理 - 唯象学 · 物理学 2016-09-21 G. Barello , Spencer Chang , Christopher A. Newby

I consider couplings between the dark energy and dark matter sectors. I describe how the existence of an adiabatic regime, in which the dark energy field instantaneously tracks the minimum of its effective potential, opens the door for a…

宇宙学与河外天体物理 · 物理学 2009-10-16 Mark Trodden

A dark energy component is responsible for the present stage of acceleration of our universe. If no fine tuning is assumed on the dark energy potential then it will end up dominating the universe at late times and the universe will not stop…

天体物理学 · 物理学 2008-11-26 A. de la Macorra

More than sixty years ago Zwicky made the case that the great clusters of galaxies are held together by the gravitational force of unseen (dark) matter. Today, the case is stronger and more precise: Dark, nonbaryonic matter accounts for 30%…

天体物理学 · 物理学 2016-11-23 Michael S. Turner

Progress in observational cosmology over the past five years has established that the Universe is dominated dynamically by dark matter and dark energy. Both these new and apparently independent forms of matter-energy have properties that…

天体物理学 · 物理学 2009-11-10 J. M. Overduin , P. S. Wesson

While there is evidence for the existence of dark matter, its properties have yet to be discovered. Simultaneously, the nature of high-energy astrophysical neutrinos detected by IceCube remains unresolved. If dark matter and neutrinos are…

高能天体物理现象 · 物理学 2021-07-27 Adam McMullen , Aaron Vincent , Carlos Arguelles , Austin Schneider

We consider theories in which there exists a nontrivial coupling between the dark matter sector and the sector responsible for the acceleration of the universe. Such theories can possess an adiabatic regime in which the quintessence field…

天体物理学 · 物理学 2008-11-26 Rachel Bean , Eanna E. Flanagan , Mark Trodden

We investigate a possible resolution of the dark energy problem within a pair-universe framework, in which the Universe emerges as an entangled pair of time-reversed sectors. In this setting, a global zero-energy condition allows vacuum…

广义相对论与量子宇宙学 · 物理学 2026-03-05 Merab Gogberashvili , Tinatin Tsiskaridze

Dark energy is usually parametrized as a perfect fluid with negative pressure and a certain equation of state. Besides, it is supposed to interact very weakly with the rest of the components of the universe and, as a consequence, there is…

天体物理学 · 物理学 2015-05-13 Jose Beltran Jimenez , Antonio L. Maroto

We uncover the general mechanism producing the dark energy(DE). This is only based on well known quantum physics and cosmology. We show that the observed DE originates from the cosmological quantum vacuum of light particles which provides a…

天体物理学 · 物理学 2023-04-05 Hector J. de Vega , Norma G. Sanchez

We describe how known matter effects within a well-motivated particle physics framework can explain the dark energy component of the Universe. By considering a cold gas of particles which interact via a vector mediator, we show that there…

宇宙学与河外天体物理 · 物理学 2015-06-22 Andi Hektor , Luca Marzola , Martti Raidal , Hardi Veermäe

A disk-shaped universe (encompassing the observable universe) rotating globally with an angular speed equal to the Hubble constant is postulated. It is shown that dark energy and dark matter are cosmic inertial effects resulting from such a…

综合物理 · 物理学 2016-06-03 Serkan Zorba

The recent study on the the 6-year up-going muon neutrinos by the IceCube Collaboration and the multi-messenger analyses support the hypothesis of a two-component scenario explaining the diffuse TeV-PeV neutrino flux. Depending on the…

高能物理 - 唯象学 · 物理学 2017-02-14 Marco Chianese

A degenerate fermionic vacuum population is suggested. Based on the abundance of the dark energy density in the Universe the vacuum particle mass and number density are estimated. The obtained mass is in reasonable agreement with…

综合物理 · 物理学 2017-04-27 R. A. Treumann

In this paper we present a possible origin of dark matter and dark energy from a solution of the Einstein's equation to a primordial universe, which was presented in a previous paper. We also analyze the Dirac's equation in this primordial…

广义相对论与量子宇宙学 · 物理学 2010-10-01 A. C. V. V. de Siqueira

Context. The external regions of galaxy clusters may be under strong influence of the dark energy, discovered by observations of the SN Ia at redshift z < 1. Aims. The presence of the dark energy in the gravitational equilibrium equation,…

宇宙学与河外天体物理 · 物理学 2014-09-05 Marco Merafina , Gennady S. Bisnovatyi-Kogan , Martina Donnari