{
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  "authors": [
    {
      "raw_name": "Ann Mukuno", 
      "affiliations": [
        {
          "country": "Japan", 
          "value": "Department of Physics, Kobe University, Kobe 657-8501, Japan"
        }
      ], 
      "surname": "Mukuno", 
      "given_names": "Ann", 
      "full_name": "Mukuno, Ann"
    }, 
    {
      "raw_name": "Jiro Soda", 
      "affiliations": [
        {
          "country": "Japan", 
          "value": "Department of Physics, Kobe University, Kobe 657-8501, Japan"
        }, 
        {
          "country": "Japan", 
          "value": "International Center for Quantum-field Measurement Systems for Studies of the Universe and Particles (QUP), KEK, Tsukuba 305-0801, Japan"
        }
      ], 
      "surname": "Soda", 
      "given_names": "Jiro", 
      "full_name": "Soda, Jiro"
    }
  ], 
  "titles": [
    {
      "source": "APS", 
      "title": "Chromonatural warm inflation"
    }
  ], 
  "dois": [
    {
      "value": "10.1103/PhysRevD.109.123504"
    }
  ], 
  "publication_info": [
    {
      "journal_volume": "109", 
      "journal_title": "Physical Review D", 
      "material": "article", 
      "journal_issue": "12", 
      "year": 2024
    }
  ], 
  "$schema": "http://repo.scoap3.org/schemas/hep.json", 
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    "source": "APS", 
    "method": "APS", 
    "submission_number": "93d179dc220911ef9fecbe60ec5a7b90"
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  "page_nr": [
    11
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  "license": [
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      "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": "2024"
    }
  ], 
  "control_number": "85987", 
  "record_creation_date": "2024-06-03T14:30:04.540506", 
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      "primary": "HEP"
    }, 
    {
      "primary": "Citeable"
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      "primary": "Published"
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  "arxiv_eprints": [
    {
      "categories": [
        "hep-th", 
        "hep-ph"
      ], 
      "value": "2402.08849"
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  ], 
  "abstracts": [
    {
      "source": "APS", 
      "value": "Chromonatural inflation is a model where non-Abelian gauge fields are sustained by the coupling of the axion with the gauge field through the Chern-Simons term, while minimal warm inflation is a model where the axion produces a thermal bath of non-Abelian gauge particles through the Chern-Simons term. Since both axion inflation models are based on the same action, a natural question is if they are compatible or not. We study axion inflation with the Chern-Simons term and find that chromonatural inflation can accommodate radiation with a temperature much larger than the Hubble parameter during inflation, which is a characteristic feature of warm inflation. Thus, we conclude that chromonatural warm inflation exists, which must have phenomenologically interesting consequences."
    }
  ], 
  "imprints": [
    {
      "date": "2024-06-03", 
      "publisher": "APS"
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}