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  "authors": [
    {
      "raw_name": "Munehiro Kubo", 
      "affiliations": [
        {
          "country": "Japan", 
          "value": "Department of Physics, Saitama University, Shimo-Okubo 255, 338-8570 Saitama Sakura-ku, Japan"
        }
      ], 
      "surname": "Kubo", 
      "given_names": "Munehiro", 
      "full_name": "Kubo, Munehiro"
    }, 
    {
      "raw_name": "Joe Sato", 
      "affiliations": [
        {
          "country": "Japan", 
          "value": "Department of Physics, Saitama University, Shimo-Okubo 255, 338-8570 Saitama Sakura-ku, Japan"
        }
      ], 
      "surname": "Sato", 
      "given_names": "Joe", 
      "full_name": "Sato, Joe"
    }, 
    {
      "raw_name": "Takashi Shimomura", 
      "affiliations": [
        {
          "country": "Japan", 
          "value": "Faculty of Education, University of Miyazaki, Gakuen-Kibanadai-Nishi 1-1, 889-2192 Miyazaki, Japan"
        }
      ], 
      "surname": "Shimomura", 
      "given_names": "Takashi", 
      "full_name": "Shimomura, Takashi"
    }, 
    {
      "raw_name": "Yasutaka Takanishi", 
      "affiliations": [
        {
          "country": "Japan", 
          "value": "Department of Physics, Saitama University, Shimo-Okubo 255, 338-8570 Saitama Sakura-ku, Japan"
        }
      ], 
      "surname": "Takanishi", 
      "given_names": "Yasutaka", 
      "full_name": "Takanishi, Yasutaka"
    }, 
    {
      "raw_name": "Masato Yamanaka", 
      "affiliations": [
        {
          "country": "Japan", 
          "value": "Maskawa Institute, Kyoto Sangyo University, Kyoto 603-8555, Japan"
        }
      ], 
      "surname": "Yamanaka", 
      "given_names": "Masato", 
      "full_name": "Yamanaka, Masato"
    }
  ], 
  "titles": [
    {
      "source": "APS", 
      "title": "Big-bang nucleosynthesis and leptogenesis in the CMSSM"
    }
  ], 
  "dois": [
    {
      "value": "10.1103/PhysRevD.97.115013"
    }
  ], 
  "publication_info": [
    {
      "journal_volume": "97", 
      "journal_title": "Physical Review D", 
      "material": "article", 
      "journal_issue": "11", 
      "year": 2018
    }
  ], 
  "$schema": "http://repo.scoap3.org/schemas/hep.json", 
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    "submission_number": "bca49440b8c511eaad8602163e01809a"
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  "page_nr": [
    15
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  "license": [
    {
      "url": "https://creativecommons.org/licenses/by/4.0/", 
      "license": "CC-BY-4.0"
    }
  ], 
  "copyright": [
    {
      "statement": "Published by the American Physical Society", 
      "year": "2018"
    }
  ], 
  "control_number": "40689", 
  "record_creation_date": "2018-07-06T09:00:27.541782", 
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      "primary": "HEP"
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    {
      "primary": "Citeable"
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      "primary": "Published"
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  ], 
  "arxiv_eprints": [
    {
      "categories": [
        "hep-ph"
      ], 
      "value": "1803.07686"
    }
  ], 
  "abstracts": [
    {
      "source": "APS", 
      "value": "We have studied the constrained minimal supersymmetric standard model with three right-handed neutrinos, and investigated whether there still is a parameter region consistent with all experimental data/limits such as the baryon asymmetry of the Universe, the dark matter abundance and the lithium primordial abundance. Using Casas-Ibarra parametrization, we have found a very narrow parameter space of the complex orthogonal matrix elements where the lightest slepton can have a long lifetime, which is necessary for solving the lithium problem. We have studied three cases of the right-handed neutrino mass ratio (i) <math><msub><mi>M</mi><mn>2</mn></msub><mo>=</mo><mn>2</mn><mo>\u00d7</mo><msub><mi>M</mi><mn>1</mn></msub></math>, (ii) <math><msub><mi>M</mi><mn>2</mn></msub><mo>=</mo><mn>4</mn><mo>\u00d7</mo><msub><mi>M</mi><mn>1</mn></msub></math>, (iii) <math><msub><mi>M</mi><mn>2</mn></msub><mo>=</mo><mn>10</mn><mo>\u00d7</mo><msub><mi>M</mi><mn>1</mn></msub></math>, while <math><msub><mi>M</mi><mn>3</mn></msub><mo>=</mo><mn>40</mn><mo>\u00d7</mo><msub><mi>M</mi><mn>1</mn></msub></math> is fixed. We have obtained the mass range of the lightest right-handed neutrino that lies between <math><mn>1</mn><msup><mn>0</mn><mn>9</mn></msup></math> and <math><mn>1</mn><msup><mn>0</mn><mn>11</mn></msup><mtext> </mtext><mtext> </mtext><mi>GeV</mi></math>. The important result is that its upper limit is derived by solving the lithium problem and the lower limit comes from leptogenesis. Lepton flavor violating decays such as <math><mrow><mrow><mi>\u03bc</mi><mo>\u2192</mo><mi>e</mi><mi>\u03b3</mi></mrow></mrow></math> in our scenario are in the reach of MEG-II and Mu3e."
    }
  ], 
  "imprints": [
    {
      "date": "2018-06-08", 
      "publisher": "APS"
    }
  ]
}