Indirect detection of neutrino portal dark matter

Batell, Brian; Han, Tao; Shams Es Haghi, Barmak

doi:10.1103/physrevd.97.095020

Title: Indirect detection of neutrino portal dark matter

Journal Article · 17 May 2018 · Physical Review. D.

DOI: https://doi.org/10.1103/physrevd.97.095020 · OSTI ID:1437507

Batell, Brian ^[1]; Han, Tao ^[1]; Shams Es Haghi, Barmak ^[1]

Univ. of Pittsburgh, PA (United States)

We investigate the feasibility of the indirect detection of dark matter in a simple model using the neutrino portal. The model is very economical, with right-handed neutrinos generating neutrino masses through the type-I seesaw mechanism and simultaneously mediating interactions with dark matter. Given the small neutrino Yukawa couplings expected in a type-I seesaw, direct detection and accelerator probes of dark matter in this scenario are challenging. However, dark matter can efficiently annihilate to right-handed neutrinos, which then decay via active-sterile mixing through the weak interactions, leading to a variety of indirect astronomical signatures. We derive the existing constraints on this scenario from Planck cosmic microwave background measurements, Fermi dwarf spheroidal galaxy and Galactic center gamma-ray observations, and AMS-02 antiproton observations, and we also discuss the future prospects of Fermi and the Cherenkov Telescope Array. Thermal annihilation rates are already being probed for dark matter lighter than about 50 GeV, and this can be extended to dark matter masses of 100 GeV and beyond in the future. This scenario can also provide a dark matter interpretation of the Fermi Galactic center gamma-ray excess, and we confront this interpretation with other indirect constraints. Finally we discuss some of the exciting implications of extensions of the minimal model with large neutrino Yukawa couplings and Higgs portal couplings.

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Research Organization:: Univ. of Wisconsin, Madison, WI (United States); Univ. of Pittsburgh, PA (United States)

Sponsoring Organization:: USDOE

Grant/Contract Number:: FG02-95ER40896; SC0015634

OSTI ID:: 1437507

Alternate ID(s):: OSTI ID: 1498912

Journal Information:: Physical Review. D., Vol. 97, Issue 9; ISSN 2470-0010

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Search for annihilating dark matter in the Sun with 3 years of IceCube data Aartsen, M. G.; Ackermann, M.; Adams, J. RWTH Aachen University https://doi.org/10.18154/rwth-2017-04742	text	January 2017
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Optimized dark matter searches in deep observations of Segue 1 with MAGIC Aleksić, J.; Ansoldi, S.; Antonelli, L. A. RWTH Aachen University https://doi.org/10.18154/rwth-conv-222443	text	January 2014
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Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500 ${\rm deg}^2$ SPT-SZ Survey Hou, Z.; Reichardt, C. L.; Story, K. T. arXiv https://doi.org/10.48550/arxiv.1212.6267	text	January 2012
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Constraints on dark matter annihilation from CMB observations before Planck Lopez-Honorez, Laura; Mena, Olga; Palomares-Ruiz, Sergio arXiv https://doi.org/10.48550/arxiv.1303.5094	text	January 2013
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The Sensitivity of HAWC to High-Mass Dark Matter Annihilations Abeysekara, A. U.; Alfaro, R.; Alvarez, C. arXiv https://doi.org/10.48550/arxiv.1405.1730	text	January 2014
Background model systematics for the Fermi GeV excess Calore, Francesca; Cholis, Ilias; Weniger, Christoph arXiv https://doi.org/10.48550/arxiv.1409.0042	text	January 2014
WIMPs at the Galactic Center Agrawal, Prateek; Batell, Brian; Fox, Patrick J. arXiv https://doi.org/10.48550/arxiv.1411.2592	text	January 2014
A fussy revisitation of antiprotons as a tool for Dark Matter searches Boudaud, Mathieu; Cirelli, Marco; Giesen, Gaëlle arXiv https://doi.org/10.48550/arxiv.1412.5696	text	January 2014
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Indirect Dark Matter Signatures in the Cosmic Dark Ages I. Generalizing the Bound on s-wave Dark Matter Annihilation from Planck Slatyer, Tracy R. arXiv https://doi.org/10.48550/arxiv.1506.03811	text	January 2015
Dark matter annihilation into right-handed neutrinos and the galactic center gamma-ray excess Tang, Yi-Lei; Zhu, Shou-hua arXiv https://doi.org/10.48550/arxiv.1512.02899	text	January 2015
Fully-Automated Precision Predictions for Heavy Neutrino Production Mechanisms at Hadron Colliders Degrande, Celine; Mattelaer, Olivier; Ruiz, Richard arXiv https://doi.org/10.48550/arxiv.1602.06957	text	January 2016
Sterile neutrino portal to Dark Matter I: The $U(1)_{B-L}$ case Escudero, Miguel; Rius, Nuria; Sanz, Verónica arXiv https://doi.org/10.48550/arxiv.1606.01258	text	January 2016
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Mono-Neutrino at DUNE: New Signals From Neutrinophilic Thermal Dark Matter Kelly, Kevin J.; Zhang, Yue arXiv https://doi.org/10.48550/arxiv.1901.01259	text	January 2019
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