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Related papers: Dark Matter: The Leptonic Connection

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We consider the possibility that fermionic dark matter (DM) interacts with the Standard Model fermions through an axial Z' boson. As long as Z' decays predominantly into dark matter, the relevant LHC bounds are rather loose. Direct dark…

High Energy Physics - Phenomenology · Physics 2015-06-19 Oleg Lebedev , Yann Mambrini

We propose a simple scenario that directly connects the dark matter (DM) and neutrino mass scales. Based on an interaction between the DM particle $\chi$ and the neutrino $\nu$ of the form $\chi\chi\nu\nu/\Lambda^2$, the DM annihilation…

High Energy Physics - Phenomenology · Physics 2015-06-03 Wei-Chih Huang , Frank F. Deppisch

We explore the potential for the direct detection of light fermionic dark matter in neutrino detectors. We consider the possible observation of the process $\bar{f} p \to e^+ n$, where $f$ is a dark matter fermion, in a model-independent…

High Energy Physics - Phenomenology · Physics 2015-05-14 Jennifer Kile

Recent preliminary results from the PAMELA experiment indicate the presence of an excess of cosmic ray positrons above 10 GeV. In this letter, we consider possibility that this signal is the result of dark matter annihilations taking place…

High Energy Physics - Phenomenology · Physics 2009-12-30 Ilias Cholis , Lisa Goodenough , Dan Hooper , Melanie Simet , Neal Weiner

Recent PAMELA and ATIC data seem to indicate an excess in positron cosmic rays above approximately 10 GeV which might be due to galactic Dark Matter particle annihilation. However the background of this signal suffers many uncertainties…

High Energy Physics - Phenomenology · Physics 2009-05-20 Timur Delahaye , Pierre Brun , Fiorenza Donato , Nicolao Fornengo , Julien Lavalle , Roberto Lineros , Richard Taillet , Pierre Salati

The cosmic ray data of PAMELA/ATIC may be explained by dark matter decay with a decay rate $\tau_{DM}^{-1}\sim 10^{-26}{sec}^{-1} \sim 10^{-45}{eV}$, an energy scale which could not be understood within the framework of the standard model…

High Energy Physics - Phenomenology · Physics 2009-09-11 Hiroki Fukuoka , Jisuke Kubo , Daijiro Suematsu

Dark matter particles annihilating in the Galactic halo can provide a flux of positrons potentially observable in upcoming experiments, such as PAMELA and AMS-02. We discuss the spectral features which may be associated with dark matter…

High Energy Physics - Phenomenology · Physics 2009-11-10 Dan Hooper , Joseph Silk

The standard model of quarks and leptons is extended to connect three outstanding issues in particle physics and astrophysics: (1) the absence of strong CP nonconservation, (2) the existence of dark matter, and (3) the mechanism of nonzero…

High Energy Physics - Phenomenology · Physics 2018-05-09 Ernest Ma

The overabundance of high-energy cosmic positrons, observed by PAMELA and AMS-02, can be considered as the consequence of dark matter decays or annihilations. We show that recent FERMI/LAT measurements of the isotropic diffuse gamma-ray…

High Energy Astrophysical Phenomena · Physics 2016-07-11 Maxim Laletin

We consider an electro-weak scale model for Dark Matter (DM) and radiative neutrino mass generation. Despite the leptophilic nature of DM with no direct couplings to quarks and gluons, scattering with nuclei is induced at the 1-loop level…

High Energy Physics - Phenomenology · Physics 2014-08-19 Daniel Schmidt , Thomas Schwetz , Takashi Toma

Laboratory experiments searching for galactic dark matter particles scattering off nuclei have so far not been able to establish a discovery. We use data from the XENON100 experiment to search for dark matter interacting with electrons.…

Observational evidences of nonzero neutrino masses and the existence of dark matter request physics beyond standard model. A model with extra scalars and leptonic vector-like fermions is introduced. By imposing a Z_2 symmetry, the neutrino…

High Energy Physics - Phenomenology · Physics 2011-04-20 Chian-Shu Chen , Chung-Hsien Chou

Dark matter pair production at high energy colliders may leave observable signatures in the energy and momentum spectra of the objects recoiling against the dark matter. We use LEP data on mono-photon events with large missing energy to…

High Energy Physics - Phenomenology · Physics 2011-08-09 Patrick J. Fox , Roni Harnik , Joachim Kopp , Yuhsin Tsai

Positron excess upto energies $\sim$350 GeV has been observed by AMS-02 result and it is consistent with the positron excess observed by PAMELA upto 100 GeV. There is no observed excess of anti-protons over the expected CR background. We…

High Energy Physics - Phenomenology · Physics 2015-06-16 Moumita Das , Subhendra Mohanty

Cosmic ray signals from dipole-interacting dark matter annihilation are considered in the positron, antiproton and photon channels. The predicted signals in the positron channel could nicely account for the excess of positron fraction from…

High Energy Astrophysical Phenomena · Physics 2013-01-23 Jae Ho Heo , C. S. Kim

In this paper we revisit constraints on the leptophilic dark matter (DM) arising from the DM indirect detection experiments. Interactions between the charged leptons and the scalar-type, Dirac-type or vector-type DM are written in terms of…

High Energy Physics - Phenomenology · Physics 2019-09-06 Wei Chao , Zhuyao Wang

This is a short review of the framework proposed in \cite{Goh:2009wg} which gives rise to indirect Dark Matter (DM) signals explaining the recent cosmic-ray anomalies and links cosmic-ray signals of DM to LHC signals of a leptonic Higgs…

High Energy Physics - Phenomenology · Physics 2015-05-14 Piyush Kumar

We reappraise the viability of asymmetric dark matter (ADM) realized as a Dirac fermion coupling dominantly to the Standard Model fermions. Treating the interactions of such a DM particle with quarks/leptons in an effective-interactions…

High Energy Physics - Phenomenology · Physics 2024-07-19 Arnab Roy , Basudeb Dasgupta , Monoranjan Guchait

Direct searches for dark matter lead to serious problems for simple models with stable neutral Weakly Interacting Massive Particles (WIMPs) as candidates for dark matter. A possibility is discussed that new stable quarks and charged leptons…

Cosmology and Nongalactic Astrophysics · Physics 2017-08-23 Maxim Yu. Khlopov

We present an economic model that establishes a link between neutrino masses and properties of the dark matter candidate. The particle content of the model can be divided into two groups: light particles with masses lighter than the…

High Energy Physics - Phenomenology · Physics 2010-09-09 Yasaman Farzan
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