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Caustics are a generic feature of the nonlinear growth of structure in the dark matter distribution. If the dark matter were absolutely cold, its mass density would diverge at caustics, and the integrated annihilation probability would also…

天体物理学 · 物理学 2009-11-13 Simon D. M. White , Mark Vogelsberger

Matter in the universe has become ``dark'' or ``missing'' through misconceptions about the fluid mechanics of gravitational structure formation. Gravitational condensation occurs on non-acoustic density nuclei at the largest Schwarz length…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

The observed anomalous excess of high-energy cosmic ray (CR) positrons is widely discussed as possible indirect evidence for dark matter (DM). However, any source of cosmic positrons is inevitably the source of gamma radiation. The least…

高能物理 - 唯象学 · 物理学 2020-04-14 Konstantin M. Belotsky , Airat Kh. Kamaletdinov , Ekaterina S. Shlepkina , Maxim L. Solovyov

We propose a simple mechanism of light dark matter (DM) production from the decay of the oscillating inflaton condensation. If the reheating temperature after inflation is higher than the inflaton mass, which is of the same order of the…

高能物理 - 唯象学 · 物理学 2021-04-21 Takeo Moroi , Wen Yin

Quantum mechanics allows for states in macroscopic superpositions, but they ordinarily undergo rapid decoherence due to interactions with their environment. A system that only interacts gravitationally, such as an arrangement of dark matter…

广义相对论与量子宇宙学 · 物理学 2021-07-21 Itamar J. Allali , Mark P. Hertzberg

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

We present a new mechanism to deplete the energy density of the QCD axion, making decay constants as high as $f_a \simeq 10^{17}\,\rm{GeV}$ viable for generic initial conditions. In our setup, the axion couples to a massless dark photon…

高能物理 - 唯象学 · 物理学 2018-04-04 Prateek Agrawal , Gustavo Marques-Tavares , Wei Xue

Primordial black holes in the mass range from $10^{-5}$ to $10^9$ g might have existed in the early universe. Via their evaporation mechanism (completed before Big Bang Nucleosynthesis), they might have released stable particles beyond the…

高能物理 - 唯象学 · 物理学 2020-12-18 Isabella Masina

A simple and well-motivated explanation for the origin of dark matter is that it consists of thermal relic particles that get their mass entirely through electroweak symmetry breaking. The simplest models implementing this possibility…

高能物理 - 唯象学 · 物理学 2007-05-23 Philip C. Schuster , Natalia Toro

We propose a new mechanism by which dark matter (DM) can affect the early universe. The hot interior of a macroscopic DM, or macro, can behave as a heat reservoir so that energetic photons are emitted from its surface. This results in…

宇宙学与河外天体物理 · 物理学 2019-07-02 Saurabh Kumar , Emanuela Dimastrogiovanni , Glenn D. Starkman , Craig Copi , Bryan Lynn

There is plenty of evidence that most matter in the Universe is dark (non-luminous). Particle physics offers several possible explanations. In this talk I focus on cold dark matter; the most promising candidates are then axions and the…

高能物理 - 唯象学 · 物理学 2008-02-03 Manuel Drees

We review progress in understanding dark matter by astrophysics, and particularly via the effect of gravitational lensing. Evidence from many different directions now all imply that five sixths of the material content of the universe is in…

宇宙学与河外天体物理 · 物理学 2015-05-14 Richard Massey , Thomas Kitching , Johan Richard

Multidimensional modification of gravity with a smaller mass scale of the gravitational interaction is considered. Stable by assumption dark matter particles could decay via interactions with virtual black holes. The decay rates of such…

高能物理 - 唯象学 · 物理学 2023-12-12 E. V. Arbuzova , A. D. Dolgov , A. A. Nikitenko

We study the capture of galactic dark matter particles in the Solar System produced by rotation of Jupiter. It is shown that the capture cross section is much larger than the area of Jupiter orbit being inversely diverging at small particle…

地球与行星天体物理 · 物理学 2013-02-26 J. Lages , D. L. Shepelyansky

The mechanism of the generation of dark matter and dark radiation from the evaporation of primordial black holes is very interesting. We consider the case of Kerr black holes to generalize previous results obtained in the Schwarzschild…

广义相对论与量子宇宙学 · 物理学 2021-12-22 Isabella Masina

The QCD axion is a good dark matter candidate. The observed dark matter abundance can arise from misalignment or defect mechanisms, which generically require an axion decay constant $f_a \sim \mathcal{O}(10^{11})$ GeV (or higher). We…

高能物理 - 唯象学 · 物理学 2018-07-27 Raymond T. Co , Lawrence J. Hall , Keisuke Harigaya

Cosmic rays of the highest energy, above the Greisen-Zatsepin-Kuzmin cut-off of the spectrum, may originate in decays of superheavy long-living X-particles. These particles may be produced in the early Universe from vacuum fluctuations…

高能物理 - 唯象学 · 物理学 2009-10-31 V. A. Kuzmin , I. I. Tkachev

We propose a novel particle physics model in which vector dark matter (VDM) and dark radiation (DR) originate from the same non-Abelian dark sector. We show an illustrating example where dark $SU(3)$ is spontaneously broken into $SU(2)$…

高能物理 - 唯象学 · 物理学 2017-03-01 P. Ko , Yong Tang

If dark matter is an axion-like-particle a significant fraction of the present day relic abundance could be concentrated in compact gravitationally bound miniclusters. We study the minicluster masses compatible with the dark matter relic…

高能物理 - 唯象学 · 物理学 2017-03-08 Edward Hardy

The stability of the dark matter particle could be attributed to the remnant $Z_2$ symmetry that arises from the spontaneous breaking of a global U(1) symmetry. This plausible scenario contains a Goldstone boson which, as recently shown by…

高能物理 - 唯象学 · 物理学 2015-06-17 Camilo Garcia-Cely , Alejandro Ibarra , Emiliano Molinaro