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The astronomical dark matter is an essential component of the Universe and yet its nature is still unresolved. It could be made of neutral and massive elementary particles which are their own antimatter partners. These dark matter species…

高能天体物理现象 · 物理学 2015-06-19 Pierre Salati

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

One of the major challenges of modern physics is to decipher the nature of dark matter. Astrophysical observations provide ample evidence for the existence of an invisible and dominant mass component in the observable universe, from the…

宇宙学与河外天体物理 · 物理学 2015-09-04 Laura Baudis

The nonbaryonic dark matter of the Universe is assumed to consist of new stable forms of matter. Their stability reflects symmetry of micro world and particle candidates for cosmological dark matter are the lightest particles that bear new…

高能物理 - 唯象学 · 物理学 2015-06-18 M. Yu. Khlopov

Dark matter in the universe seems to be one of the most important puzzles science has to face in this moment. In this essay we point out that dark matter could be a spin-0 fundamental interaction of Nature rather than a simple particle.…

天体物理学 · 物理学 2010-12-09 T. Matos , L. A. Urena-Lopez

We consider the possibility that the massive graviton is a viable candidate of dark matter in the context of bimetric gravity. We first derive the energy-momentum tensor of the massive graviton and show that it indeed behaves as that of…

高能物理 - 理论 · 物理学 2016-07-19 Katsuki Aoki , Shinji Mukohyama

One of the great mysteries of contemporary science is dark matter, an exotic substance of unknown nature that, in theory, makes up about 27\% of the total mass-energy density of the universe, and which does not appear to emit, absorb, or…

物理教育 · 物理学 2024-06-25 Jorge Pinochet

Dark matter in galaxies, its abundance, and its distribution remain a subject of long-standing discussion, especially in view of the fact that neither dark matter particles nor dark matter bodies have yet been found. Experts' opinions range…

星系天体物理 · 物理学 2017-10-31 A. V. Zasov , A. S. Saburova , A. V. Khoperskov , S. A. Khoperskov

More than 90% of matter in the Universe could be composed of heavy particles, which were non-relativistic, or 'cold', when they froze-out from the primordial soup. I will review current searches for these hypothetical particles, both via…

天体物理学 · 物理学 2009-11-11 Laura Baudis

We point out that current constraints on dark matter imply only that the majority of dark matter is cold and collisionless. A subdominant fraction of dark matter could have much stronger interactions. In particular, it could interact in a…

高能物理 - 唯象学 · 物理学 2013-08-06 JiJi Fan , Andrey Katz , Lisa Randall , Matthew Reece

A sizable fraction of the total energy density of the universe may be in heavy particles with a net dark $U(1)'$ charge comparable to its mass. When the charges have the same sign the cancellation between their gravitational and gauge…

宇宙学与河外天体物理 · 物理学 2010-04-23 Nemanja Kaloper , Antonio Padilla

[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

We propose that dark matter is composed of particles that naturally have the correct thermal relic density, but have neither weak-scale masses nor weak interactions. These WIMPless models emerge naturally from gauge-mediated supersymmetry…

高能物理 - 唯象学 · 物理学 2009-01-10 Jonathan L. Feng , Jason Kumar

The instability of dark matter may produce visible signals in the spectrum of cosmic gamma-rays. We consider this possibility in frameworks with additional spatial dimensions and supersymmetry. Examples of particles include…

天体物理学 · 物理学 2011-11-10 Jose A. R. Cembranos , Jonathan L. Feng , Louis E. Strigari

Dark matter is one of the pillars of the current standard model of structure formation: it is assumed to constitute most of the matter in the Universe. However, it can so far only be probed indirectly through its gravitational effects, and…

The existence of dark matter was suggested, using simple gravitational arguments, seventy years ago. Although we are now convinced that most of the mass in the Universe is indeed some non-luminous matter, we still do not know its…

高能物理 - 唯象学 · 物理学 2009-11-10 Carlos Munoz

The dynamics of the universe may be dominated by novel weakly interacting elementary particles, by baryons in an invisible form, by black holes, and globally by vacuum energy. The main arguments for and against such hypotheses are reviewed.

天体物理学 · 物理学 2007-05-23 Georg G. Raffelt

Dark matter, proposed decades ago as a speculative component of the universe, is now known to be the vital ingredient in the cosmos, eight times more abundant than ordinary matter, one quarter of the total energy density and the component…

天体物理学 · 物理学 2009-09-15 Jeremiah P. Ostriker , Paul J. Steinhardt

In the brane-world scenario with low tension, brane fluctuations (branons) together with the Standard Model particles are the only relevant degrees of freedom at low energies. Branons are stable, weakly interacting, massive particles and…

高能物理 - 唯象学 · 物理学 2016-11-09 J. A. R. Cembranos , A. Dobado , A. L. Maroto

Observing the Universe, astronomers have concluded that the motion of stars can not be accounted for unless one assumes that most of the mass in the Universe is carried on by a ``dark matter", so far impervious to all attempts at being…

可精确求解与可积系统 · 物理学 2015-06-26 Boris A. Kupershmidt