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  "authors": [
    {
      "raw_name": "Ding, Ran", 
      "affiliations": [
        {
          "country": "China", 
          "value": "Center for High Energy Physics, Peking University, Beijing 100871, China"
        }
      ], 
      "surname": "Ding", 
      "given_names": "Ran", 
      "full_name": "Ding, Ran"
    }, 
    {
      "raw_name": "Han, Zhi-Long", 
      "affiliations": [
        {
          "country": "China", 
          "value": "School of Physics and Technology, University of Jinan, Jinan, Shandong 250022, China"
        }
      ], 
      "surname": "Han", 
      "given_names": "Zhi-Long", 
      "full_name": "Han, Zhi-Long"
    }, 
    {
      "raw_name": "Huang, Li", 
      "affiliations": [
        {
          "country": "China", 
          "value": "State Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China"
        }
      ], 
      "surname": "Huang", 
      "given_names": "Li", 
      "full_name": "Huang, Li"
    }, 
    {
      "raw_name": "Liao, Yi", 
      "affiliations": [
        {
          "country": "China", 
          "value": "School of Physics, Nankai University, Tianjin 300071, China"
        }, 
        {
          "country": "China", 
          "value": "Center for High Energy Physics, Peking University, Beijing 100871, China"
        }, 
        {
          "country": "China", 
          "value": "State Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China"
        }
      ], 
      "surname": "Liao", 
      "given_names": "Yi", 
      "full_name": "Liao, Yi"
    }
  ], 
  "titles": [
    {
      "source": "Institute of Physics Publishing/Chinese Academy of Sciences", 
      "title": "Phenomenology of colored radiative neutrino mass model and its implications on cosmic-ray observationsSupported by the NSFC (11575089, 11025525), the National Key Research and Development Program of China (2017YFA0402200) and the CAS Center for Excellence in Particle Physics (CCEPP)"
    }
  ], 
  "dois": [
    {
      "value": "10.1088/1674-1137/42/10/103101"
    }
  ], 
  "publication_info": [
    {
      "journal_title": "Chinese Physics C", 
      "page_start": "103101", 
      "material": "article", 
      "journal_issue": "10", 
      "year": 2018
    }
  ], 
  "$schema": "http://repo.scoap3.org/schemas/hep.json", 
  "acquisition_source": {
    "date": "2018-11-15T12:30:04.875461", 
    "source": "Institute of Physics Publishing/Chinese Academy of Sciences", 
    "method": "Institute of Physics Publishing/Chinese Academy of Sciences", 
    "submission_number": "cb5ddc6ce8c911e89d1402163e01809a"
  }, 
  "page_nr": [
    18
  ], 
  "license": [
    {
      "url": "http://creativecommons.org/licenses/by/3.0/", 
      "license": "CC-BY-3.0"
    }
  ], 
  "copyright": [
    {
      "statement": "\u00a9 2018 Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Sciences and the Institute of Modern Physics of the Chinese Academy of Sciences and IOP Publishing Ltd", 
      "year": "2018"
    }
  ], 
  "control_number": "28426", 
  "record_creation_date": "2018-10-08T00:00:00", 
  "_files": [
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      "checksum": "md5:9fbecdef590477d100db84819a4ff75b", 
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      "bucket": "15eb6364-cef4-42bb-bc66-58aac4cfb62b", 
      "version_id": "d85fc6fc-6cc6-4481-8ee7-1a23e6b3f9d5", 
      "key": "10.1088/1674-1137/42/10/103101.pdf", 
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  ], 
  "arxiv_eprints": [
    {
      "categories": [
        "hep-ph"
      ], 
      "value": "1802.05248"
    }
  ], 
  "abstracts": [
    {
      "source": "Institute of Physics Publishing/Chinese Academy of Sciences", 
      "value": "We extend the colored Zee\u2013Babu model with a gauged U(1)B\u2212L symmetry, and a scalar singlet dark matter (DM) candidate S. The spontaneous breaking of U(1)B\u2212L leaves a residual Z2 symmetry that stabilizes the DM, and generates a tiny neutrino mass at the two-loop level with the color seesaw mechanism. After investigating the DM and flavor phenomenology of this model systematically, we further focus on its imprint on two cosmic-ray anomalies: The Fermi-LAT gamma-ray excess at the Galactic Center (GCE), and the PeV ultra-high energy (UHE) neutrino events at the IceCube. We found that the Fermi-LAT GCE spectrum can be well-fitted by DM annihilation into a pair of on-shell singlet Higgs mediators while being compatible with the constraints from the relic density, direct detections, and dwarf spheroidal galaxies, in the Milky Way. Although the UHE neutrino events at the IceCube could be accounted for by the resonance production of a TeV-scale leptoquark, the relevant Yukawa couplings have been severely limited by the current low-energy flavor experiments. We subsequently derive the IceCube limits on the Yukawa couplings by employing its latest six-year data."
    }
  ], 
  "imprints": [
    {
      "date": "2018-10-08", 
      "publisher": "Institute of Physics Publishing/Chinese Academy of Sciences"
    }
  ]
}