• Open Access

Scalar dark matter explanation of the DAMPE data in the minimal left-right symmetric model

Junjie Cao, Xiaofei Guo, Liangliang Shang, Fei Wang, Peiwen Wu, and Lei Zu
Phys. Rev. D 97, 063016 – Published 30 March 2018

Abstract

The left-right symmetric model (LRSM) is an attractive extension of the Standard Model (SM) that can address the origin of parity violation in the SM electroweak interactions, generate tiny neutrino masses, accommodate dark matter (DM) candidates, and provide a natural framework for baryogenesis through leptogenesis. In this work, we utilize the minimal LRSM to study the recently reported DAMPE results of the cosmic e+e spectrum, which exhibits a tentative peak around 1.4 TeV, while satisfying the current neutrino data. We propose to explain the DAMPE peak with a complex scalar DM χ in two scenarios: (1) χχ*H1++H1i+i+jj, and (2) χχ*Hk++Hki+i+jj accompanied by χχ*H1+H1i+νijνj, with i,j=e, μ, τ and k=1, 2. We fit the theoretical prediction of the e+e spectrum to relevant experimental data to determine the scalar mass spectrum favored by the DAMPE excess. We also consider various constraints from theoretical principles and collider experiments, as well as DM relic density and direct search experiments. We find that there is ample parameter space to interpret the DAMPE data while also passing the constraints. On the other hand, our explanations usually imply the existence of other new physics at an energy scale ranging from 107 to 1011GeV. Collider tests of our explanations are also discussed.

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  • Received 23 January 2018
  • Revised 6 March 2018

DOI:https://doi.org/10.1103/PhysRevD.97.063016

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Junjie Cao1,2,‡, Xiaofei Guo1,§, Liangliang Shang1,∥, Fei Wang1,3,*, Peiwen Wu4,†, and Lei Zu5,6,¶

  • 1College of Physics and Materials Science, Henan Normal University, Xinxiang 453007, China
  • 2Center for High Energy Physics, Peking University, Beijing 100871, China
  • 3School of Physics, Zhengzhou University, 450000 ZhengZhou, People’s Republic of China
  • 4School of Physics, KIAS, 85 Hoegiro, Seoul 02455, Republic of Korea
  • 5Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China
  • 6School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, Anhui, China

  • *Corresponding author. feiwang@zzu.edu.cn
  • Corresponding author. pwwu@kias.re.kr
  • junjiec@itp.ac.cn
  • §guoxf@gs.zzu.edu.cn
  • shlwell1988@foxmail.com
  • zulei@pmo.ac.cn

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Issue

Vol. 97, Iss. 6 — 15 March 2018

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