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相关论文: No-go theorem for static configurations of two cha…

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We present a no-go theorem for spherically symmetric configurations of two charged fluid species in equilibrium. The fluid species are assumed to be dusts, that is, perfect fluids without pressure, and the equilibrium can be attained for a…

广义相对论与量子宇宙学 · 物理学 2023-10-11 Andrés Aceña , Bruno Cardin Guntsche , Ivan Gentile de Austria

The qualitative behavior of charged particles in a vacuum is given by Earnshaw's Theorem which states that there is no steady configuration of charged particles in a vacuum which is asymptotically stable to perturbations. In a viscous…

流体动力学 · 物理学 2018-12-26 C. I. Trombley , M. L. Ekiel-Jezewska

The radial motion of a self-graviting charged dust and stability condition of the static charged dust spheres are considered. The stability is possible for the bound states of the weakly charged layer with abnormal charge with respect to…

广义相对论与量子宇宙学 · 物理学 2011-04-14 Valentin D. Gladush

The nonbaryonic dark matter of the Universe is assumed to consist of new stable particles. Stable particle candidates for cosmological dark matter are usually considered as neutral and weakly interacting. However stable charged leptons and…

高能物理 - 唯象学 · 物理学 2017-11-30 O. V. Bulekov , M. Yu. Khlopov , A. S. Romaniouk , Yu. S. Smirnov

We study the conditions of a possible static equilibrium between spherically symmetric, electrically charged or neutral black holes and ambient matter. The following kinds of matter are considered: (1) neutral and charged matter with a…

广义相对论与量子宇宙学 · 物理学 2013-05-29 K. A. Bronnikov , O. B. Zaslavskii

We show the existence of static, spherically symmetric spacetimes containing two stars of incompressible matter, possibly oppositely charged. The stars are held apart by the negative pressure of a positive cosmological constant but there is…

广义相对论与量子宇宙学 · 物理学 2015-05-29 Michael Fennen , Domenico Giulini

Since the electric charge in the standard model is theoretically not quantized, we may have a variant of it, called dark charge. Similar to the electric charge, the dark charge neither commutes nor closes algebraically with $SU(2)_L$. The…

高能物理 - 唯象学 · 物理学 2022-08-18 Duong Van Loi , Nguyen Manh Duc , Phung Van Dong

The concept of exotic charged dust is introduced here to represent dark matter. The term "exotic" means that the dust is not composed of normal matter, and the charge--for lack of a better term--is not an electric charge. It is also shown…

综合物理 · 物理学 2025-04-23 Gerald E. Marsh

Stable charged heavy leptons and quarks can exist and hide in elusive atoms, bound by Coulomb attraction and playing the role of dark matter. However, in the expanding Universe it is not possible to recombine all the charged particles into…

天体物理学 · 物理学 2008-11-26 K. M. Belotsky , M. Yu. Khlopov , K. I. Shibaev

We consider spherically symmetric linear perturbations of static spherically symmetric spacetimes where the matter content is ellectrically counterpoised dust. We show that the evolution equation for the fluid perturbation implies that the…

广义相对论与量子宇宙学 · 物理学 2020-10-06 Andrés Aceña , Ivan Gentile de Austria

Classical scalar fields have been considered as a possible effective description of dark matter. We show that, for any metric theory of gravity, no static, spherically symmetric, regular, spatially localized, attractive, stable spacetime…

广义相对论与量子宇宙学 · 物理学 2013-09-27 Alberto Diez-Tejedor , Alma X. Gonzalez-Morales

There is a quickly increasing wealth of experimental data on so-called dusty plasmas i. e. ionized gases or usual plasmas that contain micron sized charged particles. Interest in these structures is driven both by their importance in many…

等离子体物理 · 物理学 2009-11-13 Barbara Atamaniuk , Krzysztof Zuchowski

Conformo static charged dust distributions are investigated in the framework of General Relativity. Einstein's equations reduce to a nonlinear version of Poisson's equations and Maxwell's eqations imply the equaltiy of the charge and mass…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Metin Gurses

In this article we state and prove a dichotomy, which is satisfied by the number of non-singleton blocks in Lambda-coalescents which have a dust component. The dichotomy is of a similar type to two well known results, also dichotomies in…

概率论 · 数学 2011-11-08 Nic Freeman

It is shown that the interior solution of axially symmetric, stationary and rigidly rotating dust configurations is completely determined by the mass density along the axis of rotation. The particularly interesting case of a mass density,…

广义相对论与量子宇宙学 · 物理学 2011-05-13 Norman Gürlebeck

We consider the possibility of the existence of a stable massive charged particle by a minimal extension of the standard model particle content. Absolute stability in the case of singly charged particle is not possible if the usual doublet…

综合物理 · 物理学 2012-07-20 G. Rajasekaran

Dust aggregates are formed in a laboratory plasma as monodisperse spheres are accelerated in a self-excited dust density wave. The asymmetric charge on the aggregates causes them to rotate as they interact with the sheath electric field or…

等离子体物理 · 物理学 2013-04-09 Lorin S. Matthews , Jorge Carmona-Reyes , Victor Land , Truell W. Hyde

Particle physics candidates for cosmological dark matter are usually considered as neutral and weakly interacting. However stable charged leptons and quarks can also exist and, hidden in elusive atoms, play the role of dark matter. The…

天体物理学 · 物理学 2008-01-03 M. Yu. Khlopov

The realization of equilibrium superradiant quantum phases (photon condensates) in a spatially-uniform quantum cavity field is forbidden by a "no-go" theorem stemming from gauge invariance. We here show that the no-go theorem does not apply…

介观与纳米尺度物理 · 物理学 2020-09-25 G. M. Andolina , F. M. D. Pellegrino , V. Giovannetti , A. H. MacDonald , M. Polini

The existence of cosmological dark matter is in the bedrock of the modern cosmology. The dark matter is assumed to be nonbaryonic and to consist of new stable particles. However if composite dark matter contains stable electrically charged…

高能物理 - 唯象学 · 物理学 2018-05-02 Maxim Yu. Khlopov
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