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相关论文: Scalar-field theory of dark matter

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The vacuum is filled with complex scalar fields, such as the Higgs field. These fields serve as order parameters for superfluidity (quantum phase coherence over macroscopic distances), making the entire universe a superfluid. We review a…

广义相对论与量子宇宙学 · 物理学 2013-11-18 Kerson Huang

We consider the hypothesis that dark matter and dark energy consists of ultra-light self-interacting scalar particles. It is found that the Klein-Gordon equation with only two free parameters (mass and self-coupling) on a Schwarzschild…

宇宙学与河外天体物理 · 物理学 2018-05-31 Merab Gogberashvili , Alexander S. Sakharov

The properties of nearby galaxies that can be observed in great detail suggest that a better theory rather than cold dark matter (CDM) would describe in a better way a mechanism by which matter is more rapidly gathered into large-scale…

广义相对论与量子宇宙学 · 物理学 2015-03-17 Abril Suárez , Tonatiuh Matos

This article introduces Kerson Huang's theory on superfluid universe in these aspects: I. choose the asymptotically free Halpern-Huang scalar field(s) to drive inflation; II. use quantum turbulence to create matter; III. consider dark…

宇宙学与河外天体物理 · 物理学 2025-04-29 Hwee-Boon Low , Chi Xiong

In this article, we examine a model which proposes a common explanation for the presence of additional attractive gravitational effects -- generally considered to be due to dark matter -- in galaxies and in clusters, and for the presence of…

天体物理学 · 物理学 2007-05-23 Alexandre Arbey

We study spherically symmetric solutions with a scalar field in the shift-symmetric subclass of the Horndeski theory. Constructing an effective energy-momentum tensor of the scalar field based on the two-fluid model, we decompose the scalar…

广义相对论与量子宇宙学 · 物理学 2020-10-13 Jiaming Shi , Taishi Katsuragawa , Taotao Qiu

We build a spherical halo model for galaxies using a general scalar-tensor theory of gravity in its Newtonian limit. The scalar field is described by a time-independent Klein-Gordon equation with a source that is coupled to the standard…

星系天体物理 · 物理学 2009-03-24 Jorge L. Cervantes-Cota , Mario A. Rodriguez-Meza , Dario Nunez

We study the formation of structure in the Universe assuming that dark matter can be described by a scalar field $\tilde{\Phi}$ with a potential $V(\Phi)=-\mathfrak{m}^{2}\tilde{\Phi}^{2}/2+\lambda\tilde{\Phi}^4/4$. We derive the evolution…

宇宙学与河外天体物理 · 物理学 2021-02-09 Juan Magaña , Tonatiuh Matos , Abril Suárez , F. J. Sánchez-Salcedo

In this work we present a model of dark matter based on scalar-tensor theory of gravity. With this scalar field dark matter model we study the non-linear evolution of the large scale structures in the universe. The equations that govern the…

宇宙学与河外天体物理 · 物理学 2015-06-03 Mario A. Rodriguez-Meza

Diverse cosmological and astrophysical observations strongly hint at the presence of dark matter and dark energy in the Universe. One of the main goals of Cosmology is to explain the nature of these two components. It may well be that both…

高能物理 - 理论 · 物理学 2023-07-10 Carsten van de Bruck , Gaspard Poulot , Elsa M. Teixeira

The superfluid dark matter model offers an elegant solution to reconcile discrepancies between the predictions of the cold dark matter paradigm and observations on galactic scales. In this scenario, dark matter is composed of ultralight…

宇宙学与河外天体物理 · 物理学 2026-02-17 Lasha Berezhiani , Giordano Cintia , Valerio De Luca , Justin Khoury

We present a model for the dark matter in spiral galaxies, which is a result of a static and axial symmetric exact solution of the Einstein-Dilaton theory. We suposse that dark matter is a scalar field endowed with a scalar potential. We…

广义相对论与量子宇宙学 · 物理学 2010-04-06 F. Siddhartha Guzman , Tonatiuh Matos

We consider superfluidity and quantum vorticity in rotating spacetimes. The system is described by a complex scalar satisfying a nonlinear Klein-Gordon equation. Rotation terms are identified and found to lead to the transfer of angular…

广义相对论与量子宇宙学 · 物理学 2016-11-11 Michael R. R. Good , Chi Xiong , Alvin J. K. Chua , Kerson Huang

In the present work, we adopt a nonlinear scalar field theory coupled to the gravity sector to model galactic dark matter. We found analytical solutions for the scalar field coupled to gravity in the Newtonian limit, assuming an isotropic…

广义相对论与量子宇宙学 · 物理学 2021-05-19 R. A. C. Correa , P. H. R. S. Moraes , A. de Souza Dutra , O. L. Dors , W. de Paula , T. Frederico

We investigate scalar-tensor theories, motivated by dark energy models, in the strong gravity regime around the black hole at the centre of our galaxy. In such theories general relativity is modified since the scalar field couples to…

宇宙学与河外天体物理 · 物理学 2022-01-24 David Benisty , Anne-Christine Davis

An exact, axially symmetric solution to the Einstein-Klein-Gordon field equations is employed to model the dark matter in spiral galaxies. The extended rotation curves from a previous analysis are used to fit the model and a very good…

天体物理学 · 物理学 2007-05-23 F. S. Guzman , T. Matos , H. Villegas-Brena

We propose a unified framework that reconciles the stunning success of MOND on galactic scales with the triumph of the LambdaCDM model on cosmological scales. This is achieved through the physics of superfluidity. Dark matter consists of…

宇宙学与河外天体物理 · 物理学 2016-02-17 Lasha Berezhiani , Justin Khoury

We present a scenario for galaxy formation based on the hypothesis of scalar field dark matter. We interpret galaxy formation through the collapse of a scalar field fluctuation. We find that a cosh potential for the self-interaction of the…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Miguel Alcubierre , F. Siddhartha Guzman , Tonatiuh Matos , Dario Nunez , L. Arturo Urena-Lopez , Petra Wiederhold

We derive an effective gravitational potential, induced by the quantum wavefunction of a physical vacuum of a self-gravitating configuration, while the vacuum itself is viewed as the superfluid described by the logarithmic quantum wave…

广义相对论与量子宇宙学 · 物理学 2020-12-01 Konstantin G. Zloshchastiev

In this work we perform some studies related to dark energy. Firstly, we propose a dynamical approach to explain the dark energy content of the universe. We assume that a massless scalar field couples to the Hubble parameter with some…

高能物理 - 唯象学 · 物理学 2009-01-07 Fei Wang , Jin Min Yang
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