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相关论文: A Model of Dark Energy and Dark Matter

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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

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

A toy model giving rise to long lived super heavy particles and an small vacuum density energy, of the order of the one measured in the present universe, is constructed. This model consists in hidden sector invariant under an $SU(2)_L$…

高能物理 - 理论 · 物理学 2012-08-29 O. P. Santillan

We consider a model where both dark energy and dark matter originate from the coupling of a scalar field with a non-conventional kinetic term to, both, a metric measure and a non-metric measure. An interacting dark energy/dark matter…

广义相对论与量子宇宙学 · 物理学 2015-06-11 Stefano Ansoldi , Eduardo I. Guendelman

A new strong interaction sector is proposed as a possible origin for the Dark Energy and Dark matter. It is described by an unbroken gauge group $SU(2)_Z$ which grows strong at a scale $\Lambda_Z \sim 10^{-3} eV$ provided its coupling is of…

高能物理 - 唯象学 · 物理学 2007-05-23 P. Q. Hung

A model of dark energy and dark matter was proposed earlier by one of us (PQH) which involved an unbroken gauge group $SU(2)_Z$ whose coupling $\alpha_Z \equiv g_Z^2/4 \pi\sim O(1)$ at a scale $\Lambda_Z \sim 3 \times 10^{-3} eV$ starting…

高能物理 - 唯象学 · 物理学 2007-05-23 P. Q. Hung , Paola Mosconi

We introduce and study a model designed to simultaneously shed light on the mysteries connected with Baryogenesis, Dark Matter and Dark Energy. The model describes a self-interacting complex axion field whose imaginary part, a pseudo-scalar…

高能物理 - 理论 · 物理学 2021-04-21 Robert Brandenberger , Jürg Fröhlich

We present a unified model of dark matter and dark energy. The dark matter field is a modulus corresponding to a flat direction of supersymmetry, which couples, in a hybrid type potential, with the dark energy field. The latter is a light…

高能物理 - 唯象学 · 物理学 2009-11-10 Minos Axenides , Konstantinos Dimopoulos

A supersymmetric hybrid potential model with low energy supersymmetry breaking scale ($ M_{S}\sim 1-10 Tev$) is presented for both dark matter and dark energy. Cold dark matter is associated with a light modulus field ($\sim 10-100 Mev$)…

高能物理 - 唯象学 · 物理学 2007-05-23 Minos Axenides

A unified dynamical model of dark energy and inflation is presented, in which both phenomena are driven by axion-like fields-quintessences-of spontaneously broken global $U(1)_A$'s symmetries whose potentials are induced by instantons of…

高能物理 - 唯象学 · 物理学 2023-07-12 P. Q. Hung

A recent model of dark energy and dark matter was proposed, involving a new gauge group $SU(2)_Z$ whose coupling grows strong at a scale $\Lambda_Z \sim 10^{-3} eV$, a result which is obtained from a simple assumption that its initial value…

高能物理 - 唯象学 · 物理学 2008-03-27 P. Q. Hung

Dark energy is frequently modelled as an additional dynamical scalar field component in the Universe, referred to as "quintessence", which drives the late-time acceleration. Furthermore, the quintessence field may be coupled to dark matter…

宇宙学与河外天体物理 · 物理学 2023-09-12 Daniela Palma , Graeme N. Candlish

We outline a dynamical dark energy scenario whose signatures may be simultaneously tested by astronomical observations and laboratory experiments. The dark energy is a field with slightly sub-gravitational couplings to matter, a logarithmic…

天体物理学 · 物理学 2009-06-23 Nemanja Kaloper

We investigate a class of models for dark matter and/or negative-pressure, dynamical dark energy consisting of ``spintessence,'' a complex scalar field $\phi$ spinning in a U(1)-symmetric potential $V(\phi)=V(|\phi|)$. As the Universe…

天体物理学 · 物理学 2009-11-06 Latham A. Boyle , Robert R. Caldwell , Marc Kamionkowski

In this work we explore a model of the universe in which dark energy is modelled explicitely with both a dynamical quintessence field (with a double exponential self-interaction potential) and a cosmological constant. For a given region of…

天体物理学 · 物理学 2007-05-23 Rolando Cardenas , Tame Gonzalez , Osmel Martin , Israel Quiros

An analysis is given of interacting dark energy and dark matter where the dark energy is assumed to be an ultralight axionic field with a pseudo-Nambu-Goldstone Boson potential which is in general a superposition of $N$ number of cosine…

宇宙学与河外天体物理 · 物理学 2025-12-01 Amin Aboubrahim , Andrew H. Giman , Pran Nath

We derive two field theory models of interacting dark energy, one in which dark energy is associated with the quintessence and another in which it is associated with the tachyon. In both, instead of choosing arbitrarily the potential of…

广义相对论与量子宇宙学 · 物理学 2020-07-10 Sandro M. R. Micheletti

We study a cosmological model in which phantom dark energy is coupled to dark matter by phenomenologically introducing a coupled term to the equations of motion of dark energy and dark matter. This term is parameterized by a dimensionless…

高能物理 - 理论 · 物理学 2009-11-10 Rong-Gen Cai , Anzhong Wang

After recalling some puzzles in cosmology and briefly reviewing the Friedmann-Lema\^itre cosmos a simple unified model of the ``Dark Sector'' is described. This model involves a scalar field and a pseudo-scalar axion field that give rise to…

宇宙学与河外天体物理 · 物理学 2022-11-23 Jürg Fröhlich

Dark Energy is some of the weirdest and most mysterious stuff in the universe that tends to increase the rate of expansion of the universe. Two commonly known forms of dark energy are the cosmological constant, a constant energy density…

广义相对论与量子宇宙学 · 物理学 2010-04-28 Ishwaree P. Neupane , Holly Trowland
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