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相关论文: Dark matter superfluid and DBI dark energy

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Asymmetric dark matter is a well-motivated approach to explain the apparent coincidence between the relic densities of visible and dark matter, $\Omega_D \simeq 5.4\Omega_b$. A complete explanation requires two components, a relation…

高能物理 - 唯象学 · 物理学 2026-03-04 Peter Cox , Rafael E. Pérez , Raymond R. Volkas

In this talk I present a new model of a unified dark sector, where late-time cosmic acceleration emerges from the dark matter (DM) superfluid framework. We will start by reviewing the dark matter superfluid model and show how it describes…

宇宙学与河外天体物理 · 物理学 2019-11-19 Elisa G. M. Ferreira

The expansion of the Universe is accelerated as testified by observations of SNeIa at varying redshifts. Explanations of this acceleration are of two kinds: modifications of Einstein gravity or new forms of energy. An example of modified…

天体物理学 · 物理学 2011-11-10 M. Roos

We construct a Dirac-Born-Infeld (DBI) action coupled to a two-form field in four dimensional $\mathcal{N}=1$ supergravity. Our superconformal formulation of the action shows a universal way to construct it in various Poincar\'e…

高能物理 - 理论 · 物理学 2017-03-08 Shuntaro Aoki , Yusuke Yamada

Modified Newtonian Dynamics (MOND) is a possible solution for the missing mass problem in galactic dynamics; its predictions are in good agreement with observations in the limit of weak accelerations. However, MOND does not derive from a…

星系天体物理 · 物理学 2017-01-18 Sascha Trippe

The expansion history of the Universe reconstructed from a combination of recent data indicates a preference for a changing Dark Energy (DE) density. Moreover, the DE density appears to be increasing with cosmic time, with its equation of…

宇宙学与河外天体物理 · 物理学 2020-02-19 Alex Zucca , Levon Pogosian , Alessandra Silvestri , Yuting Wang , Gong-Bo Zhao

The observed dark energy in the universe might give particles inertial mass. We investigate one realization of this idea, that the dark energy field might be a decayed scalar component of a supermultiplet field in the early universe that…

天体物理学 · 物理学 2007-05-23 Robert J. Nemiroff , Bijunath Patla

We study the interaction between dark matter and dark energy, with dark energy described by a scalar field having a double exponential effective potential. We discover conditions under which such a scalar field driven solution is a late…

广义相对论与量子宇宙学 · 物理学 2015-08-06 Vartika Gupta , Rakesh Kabir , Amitabha Mukherjee , Daksh Lohiya

In any physical system, when we move from short to large scales, new spacetime symmetries emerge which help us to simplify the dynamics of the system. In this letter we demonstrate that certain variations on the symmetries of General…

广义相对论与量子宇宙学 · 物理学 2023-11-13 Ivan Arraut

Interactions between dark matter and ordinary matter will transfer momentum, and therefore give rise to a force on ordinary matter due to the dark matter `wind.' We show that this force can be maximal in a realistic model of dark matter,…

高能物理 - 唯象学 · 物理学 2024-09-04 Hannah Day , Da Liu , Markus A. Luty , Yue Zhao

In the search for an explanation for the current acceleration of the Universe, scalar fields are the most simple and useful tools to build models of dark energy. This field, however, must in principle couple with the rest of the world and…

广义相对论与量子宇宙学 · 物理学 2016-11-18 Carsten van de Bruck , Jurgen Mifsud , José P. Mimoso , Nelson J. Nunes

We construct the Dirac-Born-Infeld (DBI) action of a real linear multiplet in 4D $\mathcal{N}=1$ supergravity. Based on conformal supergravity, we derive the general condition under which the DBI action can be realized, and show that it can…

高能物理 - 理论 · 物理学 2016-07-19 Shuntaro Aoki , Yusuke Yamada

The article discusses a scenario based on the idea of induced spontaneous symmetry breaking. In this type of scenario, spontaneous symmetry breaking is assumed at some highest energy level, which leads to a chain of several subsequent…

高能物理 - 唯象学 · 物理学 2022-02-16 Eduard Boos

It seems necessary to suppress, at least partially, the formation of structure on subgalactic scales. As an alternative to warm or collisional dark matter, I postulate a condensate of massive bosons interacting via a repulsive interparticle…

天体物理学 · 物理学 2009-10-31 Jeremy Goodman

We propose a model based on a DBI action for the unification of dark matter and dark energy. This is supported by the results of the study of its background behavior at early and late times, and reinforced by the analysis of the evolution…

宇宙学与河外天体物理 · 物理学 2010-04-30 Luis P. Chimento , Ruth Lazkoz , Irene Sendra

There are many hot discussions in the literature about two competing paradigms in galactic and extra-galactic astronomy and cosmology, namely the Dark Matter and the Modified Newtonian Dynamics (MOND). It is very difficult to challenge MOND…

宇宙学与河外天体物理 · 物理学 2014-05-27 Alexey Golovnev , Natalia Masalaeva

We present models that simultaneously predict presence of dark energy and cold dark matter along with slow-roll inflation. The dark energy density is found to be of order $({\rm a \;few \;meV})^4$, and the mass of dark matter constituent is…

广义相对论与量子宇宙学 · 物理学 2022-05-04 M. Yoshimura

Although the modified dynamics (MOND) proposed by Milgrom successfully accounts for the systematics of galaxy rotation curves and cluster dynamics without invoking dark matter, the idea remains a largely ad hoc modification of Newtonian…

天体物理学 · 物理学 2009-10-28 R. H. Sanders

A scale invariant model containing dilaton $\phi$ and dust (as a model of matter) is studied where the shift symmetry $\phi\to\phi +const.$ is spontaneously broken at the classical level due to intrinsic features of the model. The dilaton…

广义相对论与量子宇宙学 · 物理学 2008-11-26 E. I. Guendelman , A. B. Kaganovich

We compare perturbations in a fluid model of dark energy with those in a scalar field. As compared to the $\Lambda$CDM model, large scale matter power spectrum is suppressed in fluid model as well as in a generic quintessence dark energy…

宇宙学与河外天体物理 · 物理学 2009-07-09 H. K. Jassal
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