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相关论文: Cosmology with a long-range repulsive force

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The nature of the cosmological dark matter remains elusive. Recent studies have advocated the possibility that dark matter could be composed of ultra-light, self-interacting bosons, forming a Bose-Einstein condensate in the very early…

宇宙学与河外天体物理 · 物理学 2014-04-22 Tanja Rindler-Daller , Paul R. Shapiro

We investigate dynamics of scalar field with non-minimal kinetic term. Nontrivial behavior of the field in the vicinity of singular points of kinetic term is observed. In particular, the singular points could serve as attractor for…

天体物理学 · 物理学 2016-08-16 H. Kröger , G. Melkonyan , S. G. Rubin

The existence and detection of scalar fields could provide solutions to long-standing puzzles about the nature of dark matter, the dark compact objects at the centre of most galaxies, and other phenomena. Yet, self-interacting scalar fields…

宇宙学与河外天体物理 · 物理学 2011-01-27 Pau Amaro-Seoane , Juan Barranco , Argelia Bernal , Luciano Rezzolla

In this work we extend and apply a previous proposal to study noncommutative cosmology to the FRW cosmological background coupled to a scalar field, this is done in classical and quantum scenarios. In both cases noncommutativity is…

广义相对论与量子宇宙学 · 物理学 2008-11-26 W. Guzmán , M. Sabido , J. Socorro

The consensus of opinion in cosmology is that the Universe is currently undergoing a period of accelerated expansion. With current and proposed high precision experiments it offers the hope of being able to discriminate between the two…

天体物理学 · 物理学 2011-02-09 P. S. Corasaniti , E. J. Copeland

We study evolution of cosmological models filled with the scalar field and barotropic matter. We consider the scalar field minimally and non-minimally coupled to gravity. We demonstrated the growth of degree of complexity of evolutional…

宇宙学与河外天体物理 · 物理学 2012-12-20 Orest Hrycyna , Marek Szydlowski

We have investigated the cosmological scenarios with a four dimensional effective action which is connected with multidimensional, supergravity and string theories. The solution for the scale factor is such that initially universe undergoes…

广义相对论与量子宇宙学 · 物理学 2014-11-17 A. A. Sen , S. Sen

We consider an extension of Weyl geometry with the most general connection linearly determined by a vector field. We discuss some of the geometrical properties within this framework and then we construct gravitational theories leading to an…

广义相对论与量子宇宙学 · 物理学 2016-06-15 Jose Beltran Jimenez

We consider the cosmological application of a (variant of) relatively newly proposed model \cite{1609.06915} unifying inflation, dark energy, dark matter, and the Higgs mechanism. The model was originally defined using additional…

广义相对论与量子宇宙学 · 物理学 2019-06-21 Denitsa Staicova , Michail Stoilov

Analyzing quantum cosmological scenarios containing one scalar field with exponential potential, we have obtained a universe model which realizes a classical dust contraction from very large scales, the initial repeller of the model, and…

广义相对论与量子宇宙学 · 物理学 2017-09-13 Samuel Colin , Nelson Pinto-Neto

We present a model where a non-conventional scalar field may act like dark energy leading to cosmic acceleration. The latter is driven by an appropriate field configuration, which result in an effective cosmological constant. The potential…

高能物理 - 理论 · 物理学 2009-11-11 Alex Kehagias

Using the non-canonical model of scalar field, the cosmological consequences of a pervasive, self-interacting, homogeneous and rolling scalar field are studied. In this model, the scalar field potential is nonlinear and decreases in…

广义相对论与量子宇宙学 · 物理学 2015-12-18 Z. Ossoulian , T. Golanbari , H. Sheikhahmadi , Kh. Saaidi

We investigate the dynamics of the FLRW flat cosmological models in which the vacuum energy varies with redshift. A particularly well motivated model of this type is the so-called quantum field vacuum, in which both kind of terms $H^{2}$…

宇宙学与河外天体物理 · 物理学 2015-07-15 Spyros Basilakos

Cosmology in extended theories of gravity is considered assuming the Palatini variational principle, for which the metric and connection are independent variables. The field equations are derived to linear order in perturbations about the…

天体物理学 · 物理学 2015-06-24 Tomi Koivisto , Hannu Kurki-Suonio

Cosmology with a three-form field interacting with cold dark matter is considered. In particular, the mass of the dark matter particles is assumed to depend upon the amplitude of the three-form field invariant. In comparison to coupled…

宇宙学与河外天体物理 · 物理学 2015-06-12 Tomi S. Koivisto , Nelson J. Nunes

We discuss a cosmological model where the universe shrinks rather than expands during the radiation and matter dominated periods. Instead, the Planck mass and all particle masses grow exponentially, with the size of atoms shrinking…

宇宙学与河外天体物理 · 物理学 2013-11-13 C. Wetterich

A `bouncing' cosmological model is proposed in the context of a Weyl-invariant scalar-tensor (WIST) theory of gravity. In addition to being Weyl-invariant the theory is U(1)-symmetric and has a conserved global charge. The entire cosmic…

广义相对论与量子宇宙学 · 物理学 2022-05-17 Meir Shimon

We study the dynamics of a scalar field in the brane cosmology. We assume that a scalar field is confined in our 4-dimensional world. As for the potential of the scalar field, we discuss three typical models: (1) a power-law potential, (2)…

高能物理 - 唯象学 · 物理学 2009-11-07 Shuntaro Mizuno , Kei-ichi Maeda , Kohta Yamamoto

We consider ultralight scalar dark matter that couples to right-handed neutrinos. Due to the high density of neutrinos in the early universe, the background neutrino density dominates the dynamics of the scalar field, and qualitatively…

高能物理 - 唯象学 · 物理学 2025-02-05 Ryan Plestid , Sophia Tevosyan

The inhomogeneous cosmological model with matter in the form self-acting scalar field and perfect fluid is considered. On the basis of exact solutions is considered the evolution of density distribution of a matter in space on a background…

广义相对论与量子宇宙学 · 物理学 2007-05-23 V. M. Zhuravlev , D. A. Kornilov