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相关论文: Asymmetric Dark Matter in the Sun: A Multicomponen…

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The annihilation of dark matter (DM) particles accumulated in the Sun could produce a flux of neutrinos, which is potentially detectable with neutrino detectors/telescopes and the DM elastic scattering cross section can be constrained.…

高能物理 - 唯象学 · 物理学 2017-05-16 Raghuveer Garani , Sergio Palomares-Ruiz

The need for dark matter is briefly reviewed. A wealth of observational information points to the existence of a non-baryonic component. To the theoretically favoured candidates today belong axions, supersymmetric particles, and to some…

天体物理学 · 物理学 2015-06-24 L. Bergstrom

We calculate the muon flux from annihilation of the dark matter in the core of the Sun, in the core of the Earth and from cosmic diffuse neutrinos produced in dark matter annihilation in the halos. We consider model-independent direct…

高能物理 - 唯象学 · 物理学 2009-09-02 Arif Emre Erkoca , Mary Hall Reno , Ina Sarcevic

Dark matter (DM) coupled to light mediators has been invoked to resolve the putative discrepancies between collisionless cold DM and galactic structure observations. However, $\gamma$-ray searches and the CMB strongly constrain such…

高能物理 - 唯象学 · 物理学 2018-06-27 Iason Baldes , Marco Cirelli , Paolo Panci , Kalliopi Petraki , Filippo Sala , Marco Taoso

We review the prospects for discovering supersymmetric dark matter in a recently proposed set of post-LEP supersymmetric benchmark scenarios. We consider direct detection through spin-independent nuclear scattering, as well as indirect…

高能物理 - 唯象学 · 物理学 2009-09-11 John Ellis , Jonathan L. Feng , Andrew Ferstl , Konstantin T. Matchev , Keith A. Olive

Cold dark matter particles with an intrinsic matter-antimatter asymmetry do not annihilate after gravitational capture by the Sun and can affect its interior structure. The rate of capture is exponentially enhanced when such particles have…

高能物理 - 唯象学 · 物理学 2014-11-20 Mads T. Frandsen , Subir Sarkar

Asymmetric Dark Matter (ADM) models invoke a particle-antiparticle asymmetry, similar to the one observed in the Baryon sector, to account for the Dark Matter (DM) abundance. Both asymmetries are usually generated by the same mechanism and…

高能物理 - 唯象学 · 物理学 2015-06-04 Mattias Blennow , Enrique Fernandez-Martinez , Olga Mena , Javier Redondo , Paolo Serra

We evaluate the fluxes of up--going muons detectable in a neutrino telescope and due to the annihilation of relic neutralinos in the Earth and in the Sun, taking realistically into account the fact that neutralinos might provide only a…

高能物理 - 唯象学 · 物理学 2011-05-23 A. Bottino , N. Fornengo , G. Mignola , L. Moscoso

The annihilation of dark matter particles captured by the Sun can lead to a neutrino flux observable in neutrino detectors. Considering the fact that these dark matter particles are non-relativistic, if a pair of dark matter annihilates to…

高能物理 - 唯象学 · 物理学 2014-11-20 Arman Esmaili , Yasaman Farzan

With the augmentation of IceCube by DeepCore, the prospect for detecting dark matter annihilation in the Sun is much improved. To complement this experimental development, we provide a thorough template analysis of the particle physics…

高能物理 - 唯象学 · 物理学 2015-03-17 V. Barger , Y. Gao , D. Marfatia

The goal of this work is to find the simplest UV completions of Accidental Composite Dark Matter models that can dynamically generate an asymmetry for the Dark Matter candidate, the lightest dark baryon, and simultaneously annihilate the…

高能物理 - 唯象学 · 物理学 2022-05-19 Salvatore Bottaro , Marco Costa , Oleg Popov

If dark matter annihilates to light quarks in the core of the Sun, then a flux of 236 MeV neutrinos will be produced from the decay of stopped kaons. We consider strategies for DUNE to not only observe such a signal, but to determine the…

高能物理 - 唯象学 · 物理学 2017-10-12 Carsten Rott , Seongjin In , Jason Kumar , David Yaylali

As is well-known, if the scattering cross section of the Dark Matter (DM) particles off the nuclei inside the Sun is large enough, the Sun can trap DM particles. In principle, the annihilation of DM pair inside the Sun can then lead to the…

高能物理 - 唯象学 · 物理学 2015-06-03 Yasaman Farzan

Dark matter particles captured in the Sun would annihilate producing a neutrino flux that could be detected at the Earth. In some channels, however, the neutrino flux lies in the MeV range and is thus undetectable at IceCube, namely when…

高能物理 - 唯象学 · 物理学 2015-06-18 Alejandro Ibarra , Maximilian Totzauer , Sebastian Wild

Under the hypothesis of a Dark Matter composed by supersymmetric particles like neutralinos, we investigate the possibility that their annihilation in the haloes of nearby galaxies could produce detectable fluxes of $\gamma$-photons.…

天体物理学 · 物理学 2009-11-10 Lidia Pieri , Enzo Branchini

We extend the analysis of asymmetric Dark Matter relic density with Sommerfeld enhancement to the case where the mediator is massive. In asymmetric Dark Matter models, the asymmetric Dark Matter is assumed to couple to light scalar or…

高能物理 - 唯象学 · 物理学 2021-02-24 Aerman Sulitan , Hoernisa Iminniyaz , Mu Baoxia

Broad disagreement persists between helioseismological observables and predictions of solar models computed with the latest surface abundances. Here we show that most of these problems can be solved by the presence of asymmetric dark matter…

高能物理 - 唯象学 · 物理学 2015-03-05 Aaron C. Vincent , Pat Scott , Aldo Serenelli

Most models for asymmetric dark matter allow for dark matter self annihilation processes, which can wash out the asymmetry at temperatures near and below the dark matter mass. We study the coupled set of Boltzmann equations for the…

高能物理 - 唯象学 · 物理学 2015-06-05 Ulrich Ellwanger , Pantelis Mitropoulos

A new set of supersymmetric benchmark scenarios has recently been proposed in the context of the constrained MSSM (CMSSM) with universal soft supersymmetry-breaking masses, taking into account the constraints from LEP, $b \to s \gamma$ and…

天体物理学 · 物理学 2009-09-11 John Ellis , Jonathan L. Feng , Andrew Ferstl , Konstantin T. Matchev , Keith A. Olive

We calculate the annihilation rate of weakly interacting massive particles (WIMPs) in the Sun as a function of their mass and elastic scattering cross section. One byproduct of the annihilation, muon neutrinos, may be observed by the next…

高能天体物理现象 · 物理学 2009-07-30 Annika H. G. Peter