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Related papers: Asymmetric Dark Matter in the Sun: A Multicomponen…

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Semi-annihilation is a generic feature of dark matter theories with symmetries larger than Z_2. We explore a model based on a Z_4-symmetric dark sector comprised of a scalar singlet and a "wino"-like fermion SU(2)_L triplet. This is the…

High Energy Physics - Phenomenology · Physics 2015-10-09 Andrew P. Spray , Yi Cai

Dark matter could be captured in the Sun and self-annihilate, giving rise to an observable neutrino flux. Indirect searches for dark matter looking for this signal with neutrino telescopes have resulted in tight constraints on the…

High Energy Astrophysical Phenomena · Physics 2014-06-03 Koun Choi , Carsten Rott , Yoshitaka Itow

We study the constraints from direct detection and solar capture on dark matter scenarios with a subdominant dissipative component. This dissipative dark matter component in general has both a symmetric and asymmetric relic abundance.…

High Energy Physics - Phenomenology · Physics 2015-06-18 JiJi Fan , Andrey Katz , Jessie Shelton

We study the effect of the MeV-scale asymmetric dark matter annihilation on the effective number of neutrinos $N_{\rm eff}$ at the epoch of the big bang nucleosynthesis. If the asymmetric dark matter $\chi$ couples more strongly to the…

High Energy Physics - Phenomenology · Physics 2016-03-23 Teruyuki Kitabayashi , Yoshihiro Kurosawa

We present models that can reconcile the solar and atmospheric neutrino data with the existence of a hot dark matter component in the universe. This dark matter is a quasi-Dirac neutrino whose mass $m_{DM}$ arises at the one-loop level. The…

High Energy Physics - Phenomenology · Physics 2016-09-01 J. T. Peltoniemi , J. W. F. Valle

We consider dark matter annihilation into Standard Model particles and show that the least detectable final states, namely neutrinos, define an upper bound on the total cross section. Calculating the cosmic diffuse neutrino signal, and…

Astrophysics · Physics 2008-11-26 John F. Beacom , Nicole F. Bell , Gregory D. Mack

Neutralino annihilations in the Sun to weak boson and top quark pairs lead to high-energy neutrinos that can be detected by the IceCube and KM3 experiments in the search for neutralino dark matter. We calculate the neutrino signals from…

High Energy Physics - Phenomenology · Physics 2008-11-26 Vernon Barger , Wai-Yee Keung , Gabe Shaughnessy , Adam Tregre

Two new observations have strengthened the case for the supersymmetric nature of the Cold Dark Matter component in our universe: First, it was shown that new data on the nuclear abundance, B/C - and 10Be/9Be ratios constrain the diffusion…

High Energy Physics - Phenomenology · Physics 2016-09-06 W. de Boer , M. Herold , C. Sander , V. Zhukov

Predictions for the out-going muon fluxes from the annihilation of neutralinos in the center of the Sun and the Earth in supergravity unification are given. Effects of uncertainties of the input data are analysed. It is shown that the…

High Energy Physics - Phenomenology · Physics 2014-11-17 Achille Corsetti , Pran Nath

Dark matter particles captured by the Sun through scattering may annihilate and produce neutrinos, which escape. Current searches are for the few high-energy neutrinos produced in the prompt decays of some final states. We show that…

High Energy Astrophysical Phenomena · Physics 2013-09-06 Carsten Rott , Jennifer Siegal-Gaskins , John F. Beacom

If the present dark matter in the Universe annihilates into Standard Model particles, it must contribute to the gamma ray fluxes detected on the Earth. The magnitude of such contribution depends on the particular dark matter candidate, but…

High Energy Physics - Phenomenology · Physics 2011-09-26 Álvaro de la Cruz-Dombriz , Viviana Gammaldi

Asymmetric dark matter models are based on the hypothesis that the present-day abundance of dark matter has the same origin as the abundance of ordinary or visible matter: an asymmetry in the number densities of particles and antiparticles.…

High Energy Physics - Phenomenology · Physics 2013-08-02 Kalliopi Petraki , Raymond R. Volkas

Sterile neutrinos at the eV scale have long been studied in the context of anomalies in short baseline neutrino experiments. Their cosmology can be made compatible with our understanding of the early Universe provided the sterile neutrino…

High Energy Physics - Phenomenology · Physics 2017-07-26 Francesco Capozzi , Ian M. Shoemaker , Luca Vecchi

We investigate a scenario where dark matter (DM) particles can be captured and accumulate in the Sun, and subsequently annihilate into a pair of long-lived mediators. These mediators can decay further out in the Sun or outside of the Sun.…

High Energy Astrophysical Phenomena · Physics 2019-11-15 Carl Niblaeus , Ankit Beniwal , Joakim Edsjo

The IceCube Upgrade will provide unprecedented sensitivity to dark matter particles annihilating in the core of the Sun. For dark matter candidates with spin-dependent couplings to nuclei and that annihilate significantly to tau leptons or…

High Energy Physics - Phenomenology · Physics 2025-08-20 Dan Hooper , Fabrizio Vassallo

In the context of the relationship between physics of cosmological dark matter and symmetry of elementary particles a wide list of dark matter candidates is possible. New symmetries provide stability of different new particles and their…

High Energy Physics - Phenomenology · Physics 2017-04-26 M. Yu. Khlopov

One of the most interesting mysteries of astrophysics is the puzzle of dark matter. Although numerous techniques have been explored and developed to detect this elusive substance, its nature remains unknown. One such method uses large…

High Energy Physics - Phenomenology · Physics 2008-11-26 Dan Hooper , Joseph Silk

The Sun is a promising target for dark matter (DM) searches due to its ability to accumulate DM particles via scattering and catalyze their self-annihilation. However, at low DM masses, DM particles can also "evaporate" due to subsequent…

High Energy Physics - Phenomenology · Physics 2026-03-05 Thong T. Q. Nguyen , Tim Linden

We study the fluxes of anti-deuterons that could be produced by annihilations in the galactic halo of Dark Matter particles with multi-TeV mass and a large annihilation cross section, as indicated by the recent PAMELA results. The model of…

High Energy Physics - Phenomenology · Physics 2010-12-17 Carolin B. Braeuninger , Marco Cirelli

As cosmology has entered a phase of precision experiments, the content of the universe has been established to contain interesting and not yet fully understood components, namely dark energy and dark matter. While the cause and exact nature…

High Energy Physics - Phenomenology · Physics 2015-06-25 Lars Bergstrom
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