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  "authors": [
    {
      "raw_name": "Francesco Capozzi", 
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          "country": "USA", 
          "value": "Center for Cosmology and AstroParticle Physics (CCAPP), Ohio State University, Columbus, Ohio 43210, USA"
        }, 
        {
          "country": "USA", 
          "value": "Department of Physics, Ohio State University, Columbus, Ohio 43210, USA"
        }, 
        {
          "country": "Germany", 
          "value": "Max-Planck-Institut f\u00fcr Physik (Werner-Heisenberg-Institut), 80805 M\u00fcnchen, Germany"
        }
      ], 
      "surname": "Capozzi", 
      "given_names": "Francesco", 
      "full_name": "Capozzi, Francesco"
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    {
      "raw_name": "Shirley Weishi Li", 
      "affiliations": [
        {
          "country": "USA", 
          "value": "Center for Cosmology and AstroParticle Physics (CCAPP), Ohio State University, Columbus, Ohio 43210, USA"
        }, 
        {
          "country": "USA", 
          "value": "Department of Physics, Ohio State University, Columbus, Ohio 43210, USA"
        }, 
        {
          "country": "USA", 
          "value": "SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA"
        }
      ], 
      "surname": "Li", 
      "given_names": "Shirley Weishi", 
      "full_name": "Li, Shirley Weishi"
    }, 
    {
      "raw_name": "Guanying Zhu", 
      "affiliations": [
        {
          "country": "USA", 
          "value": "Center for Cosmology and AstroParticle Physics (CCAPP), Ohio State University, Columbus, Ohio 43210, USA"
        }, 
        {
          "country": "USA", 
          "value": "Department of Physics, Ohio State University, Columbus, Ohio 43210, USA"
        }
      ], 
      "surname": "Zhu", 
      "given_names": "Guanying", 
      "full_name": "Zhu, Guanying"
    }, 
    {
      "raw_name": "John F. Beacom", 
      "affiliations": [
        {
          "country": "USA", 
          "value": "Center for Cosmology and AstroParticle Physics (CCAPP), Ohio State University, Columbus, Ohio 43210, USA"
        }, 
        {
          "country": "USA", 
          "value": "Department of Physics, Ohio State University, Columbus, Ohio 43210, USA"
        }, 
        {
          "country": "USA", 
          "value": "Department of Astronomy, Ohio State University, Columbus, Ohio 43210, USA"
        }
      ], 
      "surname": "Beacom", 
      "given_names": "John F.", 
      "full_name": "Beacom, John F."
    }
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  "titles": [
    {
      "source": "APS", 
      "title": "DUNE as the Next-Generation Solar Neutrino Experiment"
    }
  ], 
  "dois": [
    {
      "value": "10.1103/PhysRevLett.123.131803"
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      "journal_volume": "123", 
      "journal_title": "Physical Review Letters", 
      "material": "article", 
      "journal_issue": "13", 
      "year": 2019
    }
  ], 
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    "source": "APS", 
    "method": "APS", 
    "submission_number": "810b323c058f11ecb53772fd3742099d"
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  "page_nr": [
    7
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  "license": [
    {
      "url": "https://creativecommons.org/licenses/by/4.0/", 
      "license": "CC-BY-4.0"
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  "copyright": [
    {
      "statement": "Published by the American Physical Society", 
      "year": "2019"
    }
  ], 
  "control_number": "50004", 
  "record_creation_date": "2019-09-27T16:30:05.084151", 
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      "primary": "HEP"
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  "arxiv_eprints": [
    {
      "categories": [
        "hep-ph", 
        "astro-ph.SR", 
        "hep-ex", 
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        "physics.ins-det"
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      "value": "1808.08232"
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  "abstracts": [
    {
      "source": "APS", 
      "value": "We show that the Deep Underground Neutrino Experiment (DUNE), with significant but feasible new efforts, has the potential to deliver world-leading results in solar neutrinos. With a <math><mrow><mn>100</mn><mtext> </mtext><mtext> </mtext><mi>kton</mi><mtext>\u2212</mtext><mi>yr</mi></mrow></math> exposure, DUNE could detect <math><mo>\u2273</mo><msup><mn>10</mn><mn>5</mn></msup></math> signal events above 5 MeV electron energy. Separate precision measurements of neutrino-mixing parameters and the <math><mrow><mmultiscripts><mrow><mi>B</mi></mrow><mprescripts></mprescripts><none></none><mrow><mn>8</mn></mrow></mmultiscripts></mrow></math> flux could be made using two detection channels (<math><mrow><msub><mrow><mi>\u03bd</mi></mrow><mrow><mi>e</mi></mrow></msub><mo>+</mo><mmultiscripts><mrow><mi>Ar</mi></mrow><mprescripts></mprescripts><none></none><mrow><mn>40</mn></mrow></mmultiscripts></mrow></math> and <math><mrow><msub><mrow><mi>\u03bd</mi></mrow><mrow><mi>e</mi><mo>,</mo><mi>\u03bc</mi><mo>,</mo><mi>\u03c4</mi></mrow></msub><mo>+</mo><msup><mrow><mi>e</mi></mrow><mrow><mo>\u2212</mo></mrow></msup></mrow></math>) and the day-night effect (<math><mo>&gt;</mo><mn>10</mn><mi>\u03c3</mi></math>). New particle physics may be revealed through the comparison of solar neutrinos (with matter effects) and reactor neutrinos (without), which is discrepant by <math><mo>\u223c</mo><mn>2</mn><mi>\u03c3</mi></math> (and could become <math><mn>5.6</mn><mi>\u03c3</mi></math>). New astrophysics may be revealed through the most precise measurement of the <math><mrow><mmultiscripts><mrow><mi>B</mi></mrow><mprescripts></mprescripts><none></none><mrow><mn>8</mn></mrow></mmultiscripts></mrow></math> flux (to 2.5%) and the first detection of the hep flux (to 11%). DUNE is required: No other experiment, even proposed, has been shown capable of fully realizing these discovery opportunities."
    }
  ], 
  "imprints": [
    {
      "date": "2019-09-27", 
      "publisher": "APS"
    }
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