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相关论文: Classical Dark Matter

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It is shown that the theory of dark matter can be derived from the first principles. Particles representing a new form of matter gravitate but do not interact electromagnetically, strongly and weakly with the known elementary particles.…

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

Production of massive stable relics in $R^2$-modified gravity is considered. It is shown that the cosmological evolution and kinetics of massive species differs significantly from those in the conventional cosmology. The results are applied…

宇宙学与河外天体物理 · 物理学 2019-04-17 E. V. Arbuzova , A. D. Dolgov , R. S. Singh

[A brief review intended for a general physics colloquium audience.] Astrophysicists now know that 80% of the matter in the universe is `dark matter', composed of neutral and weakly interacting elementary particles that are not part of the…

高能物理 - 唯象学 · 物理学 2008-11-26 Michael E. Peskin

It is now, generally, believed that the presence of some form of dark matter is essential to explain the flat rotation curves of galaxies, and anomalous large velocities of galaxies in the clusters and superclusters. This dark matter turns…

天体物理学 · 物理学 2007-05-23 Mofazzal Azam

The origin of dark matter in the universe may be weakly interacting scalar particles produced by amplification of quantum fluctuations during a period of dilaton-driven inflation. We present two interesting cases, the case of small…

高能物理 - 唯象学 · 物理学 2009-10-31 Ram Brustein , Merav Hadad

The nature of dark matter is one of the open problems of the Standard Model of particle physics. Despite the great experimental efforts, we have not yet found a positive signal of its interactions with ordinary matter. One possible…

高能物理 - 唯象学 · 物理学 2019-04-09 M. Blennow , E. Fernández-Martínez , A. Olivares-Del Campo , S. Pascoli , S. Rosauro-Alcaraz , A. V. Titov

The nonbaryonic dark matter of the Universe is assumed to consist of new stable particles. A specific case is possible, when new stable particles bear ordinary electric charge and bind in heavy "atoms" by ordinary Coulomb interaction. Such…

宇宙学与河外天体物理 · 物理学 2015-03-17 Maxim Yu. Khlopov , Andrey G. Mayorov , Evgeny Yu. Soldatov

Small-scale clumps of dark matter are gravitationally bounded structures that have masses comparable to or lower than stellar masses and consist of noninteracting or weakly interacting dark matter particles. In this paper, the current…

高能天体物理现象 · 物理学 2014-05-12 V. S. Berezinsky , V. I. Dokuchaev , Yu. N. Eroshenko

The idea that dark matter could be made of stable relics of microscopic black holes is not new. In this article, we revisit this hypothesis, focusing on the creation of black holes by the scattering of trans-Planckian particles in the early…

高能物理 - 唯象学 · 物理学 2019-12-11 Aurélien Barrau , Killian Martineau , Flora Moulin , Jean-Frédéric Ngono

Astrophysics gives evidence for the existence of Dark Matter and puts constraints on its nature. The Cold Dark Matter model has become "standard" cosmology combined with a cosmological constant. There are indications that "Cold" Dark Matter…

宇宙学与河外天体物理 · 物理学 2015-05-30 Charling Tao

It is a well-known truism, inspired on the general theory of relativity, that gravity gravitates. Here we suggest the possibility that dark matter may be caused by the gravitation of the metric. At first sight this seems impossible since…

星系天体物理 · 物理学 2011-07-05 Max Chaves

Dark matter is a fundamental constituent of the universe, which is needed to explain a wide variety of astrophysical and cosmological observations. Although the existence of dark matter was first postulated nearly a century ago and its…

宇宙学与河外天体物理 · 物理学 2025-09-23 Csaba Balazs , Torsten Bringmann , Felix Kahlhoefer , Martin White

In this article we address the mystery of dark matter. We expound the various evidences, astrophysical and cosmological, leading to hypothesize the existence of an invisible form of matter, whose attempts at detecting it have so far all…

广义相对论与量子宇宙学 · 物理学 2024-10-15 Sergio Luigi Cacciatori , Vittorio Gorini , Federico Re

Introduction to the meaning of dark matter and a few historical gestures. What it is? By what the dark matter is formed? Experimental phenomenon evidences and relative explanation under the point of view of the physics of the elementary…

天体物理学 · 物理学 2007-05-23 Azzurra Auteri

It is now believed that the universe is composed of a small amount of the normal luminous matter, a substantial amount of matter (Cold Dark Matter: CDM) which is non-luminous and a large amount of smooth energy (Dark Energy: DE). Both CDM…

Observational evidence for the existence of Dark Matter is limited to its gravitational effects. The extensive program for dedicated searches has yielded null results so far, challenging the most popular models. Here we propose that this is…

Well known scaling laws among the structural properties of the dark and the luminous matter in disc systems are too complex to be arisen by two inert components that just share the same gravitational field. This brings us to critically…

星系天体物理 · 物理学 2020-03-10 Paolo Salucci , Nicola Turini

The existence of extremely dark and compact astronomical bodies is by now a well established observational fact. On the other hand, classical General Relativity predicts the existence of black holes which fit very well with the…

广义相对论与量子宇宙学 · 物理学 2015-05-14 C. Barcelo , S. Liberati , S. Sonego , M. Visser

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 identification of a solution to the dark matter problem has many arrows to its bow: if dark matter is a new elementary particle, both laboratory experiments and astrophysics can bring relevant and complementary pieces of information,…

高能天体物理现象 · 物理学 2017-01-17 N. Fornengo