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相关论文: On the stability of particle dark matter

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There are several ways to explain the dark matter relic density other than by the ordinary freeze-out scenario. For example, the freeze-in mechanism may constitute an alternative for generating the correct relic density for dark matter…

高能物理 - 唯象学 · 物理学 2012-10-02 Andrew J. Williams , Celine Boehm , Stephen M. West , Daniel Albornoz Vasquez

Dark matter stability can result from a residual matter-parity symmetry surviving spontaneous breaking of an extended gauge symmetry. We propose the simplest scotogenic dark matter completion of the original SVS theory (Phys.Rev. D22 (1980)…

高能物理 - 唯象学 · 物理学 2020-09-08 A. E. Cárcamo Hernández , José W. F. Valle , Carlos A. Vaquera-Araujo

Quantum theory, general relativity, the standard model of particle physics, and the $\Lambda$CDM model of cosmology have all been spectacularly successful within their respective regimes of applicability, but many central problems remain…

综合物理 · 物理学 2026-05-26 Roland E. Allen

Till today, the nature of Dark Matter (DM) remains elusive despite all our efforts. This missing matter of the universe has not been observed by the already operating DM direct-detection experiments, but we can infer its gravitational…

高能天体物理现象 · 物理学 2024-06-10 M. Vikiaris , V. Petousis , M. Veselsky , Ch. C. Moustakidis

The cold dark matter model successfully explains both the emergence and evolution of cosmic structures on large scales and, when we include a cosmological constant, the properties of the homogeneous and isotropic Universe. However, the cold…

宇宙学与河外天体物理 · 物理学 2020-08-04 Ivan de Martino , Sankha S. Chakrabarty , Valentina Cesare , Arianna Gallo , Luisa Ostorero , Antonaldo Diaferio

A key prediction of the standard cosmological model -- which relies on the assumption that dark matter is cold, i.e. non-relativistic at the epoch of structure formation -- is the existence of a large number of dark matter substructures on…

宇宙学与河外天体物理 · 物理学 2018-07-31 Nilanjan Banik , Gianfranco Bertone , Jo Bovy , Nassim Bozorgnia

We embed a thermal dark matter (DM) candidate within the clockwork framework. This mechanism allows to stabilize the DM particle over cosmological time because it suppresses its decay into Standard Model (SM) particles. At the same time,…

高能物理 - 唯象学 · 物理学 2017-07-18 Thomas Hambye , Daniele Teresi , Michel H. G. Tytgat

The standard cold dark matter cosmological model, while successful in explaining the observed large scale structure of the Universe, tends to overpredict structure on small scales. It has been proposed this problem may be alleviated in a…

高能物理 - 唯象学 · 物理学 2011-03-21 Nicole F. Bell , Ahmad J. Galea , Raymond R. Volkas

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…

We explore a class of dark matter models with two dark matter candidates, only one interacts with the standard model sector. One of the dark matter is thermalized with the assistance of the other stable particle. While both stable particles…

高能物理 - 唯象学 · 物理学 2015-06-03 Genevieve Belanger , Jong-Chul Park

Models in which the dark matter is very weakly coupled to the observable sector may explain the observed dark matter density, either as a "superWIMP" or as "asymmetric dark matter." Both types of models predict displaced vertices at…

高能物理 - 唯象学 · 物理学 2009-06-30 Spencer Chang , Markus A. Luty

Dark matter (DM) charged under a dark U(1) force appears in many extensions of the Standard Model, and has been invoked to explain anomalies in cosmic-ray data, as well as a self-interacting DM candidate. In this paper, we perform a…

高能物理 - 唯象学 · 物理学 2017-05-23 Marco Cirelli , Paolo Panci , Kalliopi Petraki , Filippo Sala , Marco Taoso

The cosmology of a standard model (SM) gauge singlet complex scalar dark matter (DM), stabilized by a reflection symmetry, is studied including all renormalizable interactions that preserve the reflection symmetry but can break the larger…

高能物理 - 唯象学 · 物理学 2021-12-30 Avirup Ghosh , Deep Ghosh , Satyanarayan Mukhopadhyay

The decoupling of a cold relic, during a decaying-particle-dominated cosmological evolution is analyzed, the relic density is calculated both numerically and semi-analytically and the results are compared with each other. Using plausible…

高能物理 - 唯象学 · 物理学 2011-05-23 C. Pallis

Exotic dark matter together with dark energy or cosmological constant seem to dominate in the Universe. An even higher density of such matter seems to be gravitationally trapped in our Galaxy. The nature of dark matter can be unveiled only,…

核理论 · 物理学 2009-09-29 J. D. Vergados

It has recently been shown that if the dark matter is in thermal equilibrium with a sector that is highly decoupled from the Standard Model, it can freeze-out with an acceptable relic abundance, even if the dark matter is as heavy as ~1-100…

高能物理 - 唯象学 · 物理学 2016-12-02 Asher Berlin , Dan Hooper , Gordan Krnjaic

One of important properties of dark matter is its stability. The U(1)$_{\rm B-L}$ gauge symmetry is the most attractive symmetry to guarantee the stability. Though the symmetry is expected to be broken at very high energy scale to account…

高能物理 - 唯象学 · 物理学 2015-05-30 Masahiro Ibe , Shigeki Matsumoto , Tsutomu T. Yanagida

We demonstrate that if the universe is dominated by the massive cold dark matter, then besides the generally believed thermal distribution of the dark matter relics, there may exist some very energetic non-thermal relics of the dark matter…

高能物理 - 唯象学 · 物理学 2007-05-23 Xue-Qian Li , Zhijian Tao

Cosmology and astroparticle physics give strongest possible evidence for the incompleteness of the Standard Model of particle physics. Leaving aside misterious dark energy, which may or may not be just the cosmological constant, two…

高能物理 - 唯象学 · 物理学 2022-11-07 V. A. Rubakov

Matter and dark matter are unified under the framework of $SU(6)\to SU(5) \times U(1)_N$. A dark-matter candidate is possible, not because it is stable, but because it has a very long lifetime, in analogy to that of the proton in theories…

高能物理 - 唯象学 · 物理学 2021-03-31 Ernest Ma