{
  "_oai": {
    "updated": "2020-01-30T16:24:06Z", 
    "id": "oai:repo.scoap3.org:52405", 
    "sets": [
      "JHEP"
    ]
  }, 
  "authors": [
    {
      "affiliations": [
        {
          "country": "USA", 
          "value": "Leinweber Center for Theoretical Physics, Department of Physics, University of Michigan, Ann Arbor, MI, 48109, USA", 
          "organization": "University of Michigan"
        }
      ], 
      "surname": "Lei", 
      "email": "minjilei@umich.edu", 
      "full_name": "Lei, Minjie", 
      "given_names": "Minjie"
    }, 
    {
      "affiliations": [
        {
          "country": "USA", 
          "value": "Leinweber Center for Theoretical Physics, Department of Physics, University of Michigan, Ann Arbor, MI, 48109, USA", 
          "organization": "University of Michigan"
        }
      ], 
      "surname": "Steinberg", 
      "email": "nastein@umich.edu", 
      "full_name": "Steinberg, Noah", 
      "given_names": "Noah"
    }, 
    {
      "affiliations": [
        {
          "country": "USA", 
          "value": "Leinweber Center for Theoretical Physics, Department of Physics, University of Michigan, Ann Arbor, MI, 48109, USA", 
          "organization": "University of Michigan"
        }
      ], 
      "surname": "Wells", 
      "email": "jwells@umich.edu", 
      "full_name": "Wells, James", 
      "given_names": "James"
    }
  ], 
  "titles": [
    {
      "source": "Springer", 
      "title": "Probing non-standard neutrino interactions with supernova neutrinos at Hyper-K"
    }
  ], 
  "dois": [
    {
      "value": "10.1007/JHEP01(2020)179"
    }
  ], 
  "publication_info": [
    {
      "page_end": "16", 
      "journal_title": "Journal of High Energy Physics", 
      "material": "article", 
      "journal_volume": "2020", 
      "artid": "JHEP01(2020)179", 
      "year": 2020, 
      "page_start": "1", 
      "journal_issue": "1"
    }
  ], 
  "$schema": "http://repo.scoap3.org/schemas/hep.json", 
  "acquisition_source": {
    "date": "2020-01-30T16:30:29.717803", 
    "source": "Springer", 
    "method": "Springer", 
    "submission_number": "60c69f76437511eaad1402163e01809a"
  }, 
  "page_nr": [
    16
  ], 
  "license": [
    {
      "url": "https://creativecommons.org/licenses/by/3.0", 
      "license": "CC-BY-3.0"
    }
  ], 
  "copyright": [
    {
      "holder": "The Author(s)", 
      "year": "2020"
    }
  ], 
  "control_number": "52405", 
  "record_creation_date": "2020-01-30T16:30:29.717835", 
  "_files": [
    {
      "checksum": "md5:b484ba411ac0c3567d8e19b16924b442", 
      "filetype": "xml", 
      "bucket": "3153d45f-f7a4-4ec3-8e86-e9dfa462adae", 
      "version_id": "c7b96562-24d8-49bd-8530-522269fa359a", 
      "key": "10.1007/JHEP01(2020)179.xml", 
      "size": 11393
    }, 
    {
      "checksum": "md5:8b414857bff1e68168b2eb1195c4b59c", 
      "filetype": "pdf/a", 
      "bucket": "3153d45f-f7a4-4ec3-8e86-e9dfa462adae", 
      "version_id": "c0e82c47-656d-477c-9128-97c1848c6e26", 
      "key": "10.1007/JHEP01(2020)179_a.pdf", 
      "size": 1435522
    }
  ], 
  "collections": [
    {
      "primary": "Journal of High Energy Physics"
    }
  ], 
  "arxiv_eprints": [
    {
      "categories": [
        "hep-ph"
      ], 
      "value": "1907.01059"
    }
  ], 
  "abstracts": [
    {
      "source": "Springer", 
      "value": "Non-standard neutrino self interactions (NSSI) could be stronger than Fermi interactions. We investigate the ability to constrain these four-neutrino interactions by their effect on the flux of neutrinos originating from a galactic supernova. In the dense medium of a core collapse supernova, these new self interactions can have a significant impact on neutrino oscillations, leading to changes at the flavor evolution and spectra level. We use simulations of the neutrino flux from a 13 solar mass, core collapse supernova at 10 kpc away, and numerically propagate these neutrinos through the stellar medium taking into account vacuum/MSW oscillations, SM \u03bd \u2212 \u03bd scattering as well as \u03bd \u2212 \u03bd interactions that arise from NSSI. We pass the resulting neutrino flux to a simulation of the future Hyper-Kamiokande detector to see what constraints on NSSI parameters are possible when the next galactic supernova becomes visible. We find that these constraints depend strongly on the neutrino mass hierarchy and if the NSSI is flavor-violating or preserving. Sensitivity to NSSI in the normal hierarchy (NH) at Hyper-K is limited by the experiment\u2019s ability to efficiently detect \u03bd  e , but deviations from no NSSI could be seen if the NSSI is particularly strong. In the inverted hierarchy (IH) scenario, Hyper-K can significantly improve constraints on flavor-violating NSSI down to   <math> <mi>O</mi> </math>  $$ \\mathcal{O} $$ (10 \u22121)G  F ."
    }
  ], 
  "imprints": [
    {
      "date": "2020-01-29", 
      "publisher": "Springer"
    }
  ]
}