中文
相关论文

相关论文: Mirror dark matter

200 篇论文

Although well established observations on cosmological, cluster, and galactic scales strongly suggest the existence of dark matter (DM), our understanding of its non-gravitational properties is still lacking. I review basic aspects of…

高能物理 - 唯象学 · 物理学 2010-08-04 Marco Regis

We discuss arguments both in favor of and against dark matter. With the repeated failure of experiment to date to detect dark matter we discuss what could be done instead, and to this end look for clues in the data themselves. We identify…

星系天体物理 · 物理学 2020-01-08 Philip D. Mannheim

We explore the dark matter interpretation of the anomalies claimed by the DAMA and CoGeNT experiments, in conjunction with the various null direct-detection experiments. An independent analysis of the CoGeNT data is employed and several…

高能物理 - 唯象学 · 物理学 2015-05-28 Marco Farina , Duccio Pappadopulo , Alessandro Strumia , Tomer Volansky

Cosmological observations offer unique and robust avenues for probing the fundamental nature of dark matter particles-they broadly test a range of compelling theoretical scenarios, often surpassing or complementing the reach of terrestrial…

The DAMA annual modulation signature, interpreted as evidence for a spin-independent WIMP coupling, seems in conflict with null results from CDMS. However, in models of ``inelastic dark matter'', the experiments are compatible. Inelastic…

天体物理学 · 物理学 2008-11-26 David R. Smith , Neal Weiner

In this note we present an extension of our previous analysis of some preliminary experimental results of the DAMA/NaI Collaboration which might be indicative of a yearly modulation effect. Here we present a direct way for obtaining from…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Bottino , F. Donato , N. Fornengo , S. Scopel

About 80\% of the mass of the present Universe is made up of the unknown (dark matter), while the rest is made up of ordinary matter. It is a very intriguing question why the {\it mass} densities of dark matter and ordinary matter (mainly…

高能物理 - 唯象学 · 物理学 2019-10-23 Masahiro Ibe , Ayuki Kamada , Shin Kobayashi , Takumi Kuwahara , Wakutaka Nakano

The DAMA collaboration reported an annually modulated rate with a phase compatible with a Dark Matter induced signal. We point out that a slowly varying rate can bias or even simulate an annual modulation if data are analyzed in terms of…

高能物理 - 实验 · 物理学 2020-05-20 Dario Buttazzo , Paolo Panci , Nicola Rossi , Alessandro Strumia

Dark matter (comprising a quarter of the Universe) is usually assumed to be due to one and only one weakly interacting particle which is neutral and absolutely stable. We consider the possibility that there are several coexisting…

高能物理 - 唯象学 · 物理学 2007-12-03 Qing-Hong Cao , Ernest Ma , Jose Wudka , C. -P. Yuan

We discuss the positive indications of a possible dark matter signal in direct detection experiments in terms of a mechanism of interaction between the dark matter particle and the nuclei occurring via the exchange of a light mediator,…

高能物理 - 唯象学 · 物理学 2013-05-29 N. Fornengo , P. Panci , M. Regis

We present two examples of velocity distributions for light dark matter particles that reconcile the annual modulation signal observed by DAMA with all other negative results from dark matter searches. They are: (1) a conventional…

高能物理 - 唯象学 · 物理学 2009-11-11 Paolo Gondolo , Graciela Gelmini

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

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

We consider a simple generic dissipative dark matter model: a hidden sector featuring two dark matter particles charged under an unbroken $U(1)'$ interaction. Previous work has shown that such a model has the potential to explain dark…

高能物理 - 唯象学 · 物理学 2018-12-13 R. Foot , S. Vagnozzi

The evidence for the dark matter of the hot big bang cosmology is about as good as it gets in natural science. The exploration of its nature is now led by direct and indirect detection experiments, to be complemented by advances in the full…

宇宙学与河外天体物理 · 物理学 2017-03-15 P. J. E. Peebles

We review the status of sterile neutrino dark matter and discuss astrophysical and cosmological bounds on its properties as well as future prospects for its experimental searches. We argue that if sterile neutrinos are the dominant fraction…

宇宙学与河外天体物理 · 物理学 2013-06-24 Alexey Boyarsky , Dmytro Iakubovskyi , Oleg Ruchayskiy

Dark matter has been introduced to explain many independent gravitational effects at different astronomical scales, in galaxies, groups of galaxies, clusters, superclusters and even across the full horizon. This review describes the…

宇宙学与河外天体物理 · 物理学 2010-10-19 Matts Roos

One of the simplest extensions of the Standard Model that explains the observed abundance of dark matter is the inert doublet model. In this theory a discrete symmetry ensures that the neutral component of an additional electroweak doublet…

高能物理 - 唯象学 · 物理学 2010-04-21 Prateek Agrawal , Ethan M. Dolle , Christopher A. Krenke

The search for dark matter is a very wide and active field of research. Many potential hints of dark matter have appeared recently which led to a burst of theoretical activity and model building. I necessarily concentrate here only in some…

高能物理 - 唯象学 · 物理学 2010-09-13 Graciela B Gelmini

Mirror matter has been proposed as a dark matter candidate. It has several very attractive features, including automatic stability and darkness, the ability to mimic the broad features of cold dark matter while in the linear density…

天体物理学 · 物理学 2008-11-26 R. Foot , R. R. Volkas