{
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  "authors": [
    {
      "raw_name": "Mark Mace", 
      "affiliations": [
        {
          "country": "Finland", 
          "value": "Department of Physics, University of Jyv\u00e4skyl\u00e4, P.O. Box 35, 40014 Jyv\u00e4skyl\u00e4, Finland"
        }, 
        {
          "country": "Finland", 
          "value": "Helsinki Institute of Physics, University of Helsinki, P.O. Box 64, 00014 Helsinki, Finland"
        }
      ], 
      "surname": "Mace", 
      "given_names": "Mark", 
      "full_name": "Mace, Mark"
    }, 
    {
      "raw_name": "Niklas Mueller", 
      "affiliations": [
        {
          "country": "USA", 
          "value": "Physics Department, Brookhaven National Laboratory, Building 510A, Upton, New York 11973, USA"
        }
      ], 
      "surname": "Mueller", 
      "given_names": "Niklas", 
      "full_name": "Mueller, Niklas"
    }, 
    {
      "raw_name": "S\u00f6ren Schlichting", 
      "affiliations": [
        {
          "country": "Germany", 
          "value": "Fakult\u00e4t f\u00fcr Physik, Universit\u00e4t Bielefeld, D-33615 Bielefeld, Germany"
        }
      ], 
      "surname": "Schlichting", 
      "given_names": "S\u00f6ren", 
      "full_name": "Schlichting, S\u00f6ren"
    }, 
    {
      "raw_name": "Sayantan Sharma", 
      "affiliations": [
        {
          "country": "India", 
          "value": "The Institute of Mathematical Sciences, HBNI, Chennai 600113, India"
        }
      ], 
      "surname": "Sharma", 
      "given_names": "Sayantan", 
      "full_name": "Sharma, Sayantan"
    }
  ], 
  "titles": [
    {
      "source": "APS", 
      "title": "Chiral Instabilities and the Onset of Chiral Turbulence in QED Plasmas"
    }
  ], 
  "dois": [
    {
      "value": "10.1103/PhysRevLett.124.191604"
    }
  ], 
  "publication_info": [
    {
      "journal_volume": "124", 
      "journal_title": "Physical Review Letters", 
      "material": "article", 
      "journal_issue": "19", 
      "year": 2020
    }
  ], 
  "$schema": "http://repo.scoap3.org/schemas/hep.json", 
  "acquisition_source": {
    "date": "2021-08-25T10:41:11.334082", 
    "source": "APS", 
    "method": "APS", 
    "submission_number": "810b323c058f11ecb53772fd3742099d"
  }, 
  "page_nr": [
    7
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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": "2020"
    }
  ], 
  "control_number": "54416", 
  "record_creation_date": "2020-05-15T16:30:06.850283", 
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  "collections": [
    {
      "primary": "HEP"
    }, 
    {
      "primary": "Citeable"
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    {
      "primary": "Published"
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  ], 
  "arxiv_eprints": [
    {
      "categories": [
        "hep-ph", 
        "astro-ph.HE", 
        "hep-lat", 
        "nucl-th"
      ], 
      "value": "1910.01654"
    }
  ], 
  "abstracts": [
    {
      "source": "APS", 
      "value": "We present a first principles study of chiral plasma instabilities and the onset of chiral turbulence in QED plasmas with strong gauge matter interaction (<math><msup><mi>e</mi><mn>2</mn></msup><msub><mi>N</mi><mi>f</mi></msub><mo>=</mo><mn>64</mn></math>), far from equilibrium. By performing classical-statistical lattice simulations of the microscopic theory, we show that the generation of strong helical magnetic fields from a helicity imbalance in the fermion sector proceeds via three distinct phases. During the initial linear instability regime the helicity imbalance of the fermion sector causes an exponential growth (damping) of magnetic field modes with right- (left-) handed polarization, for which we extract the characteristic growth (damping) rates. Secondary growth of unstable modes accelerates the helicity transfer from fermions to gauge fields and ultimately leads to the emergence of a self-similar scaling regime characteristic of a decaying turbulence, where magnetic helicity is efficiently transferred to macroscopic length scales. Within this turbulent regime, the evolution of magnetic helicity spectrum can be described by an infrared power spectrum with spectral exponent <math><mi>\u03ba</mi><mo>=</mo><mn>10.2</mn><mo>\u00b1</mo><mn>0.5</mn></math> and dynamical scaling exponents <math><mi>\u03b1</mi><mo>=</mo><mn>1.14</mn><mo>\u00b1</mo><mn>0.50</mn></math> and <math><mi>\u03b2</mi><mo>=</mo><mn>0.37</mn><mo>\u00b1</mo><mn>0.13</mn></math>."
    }
  ], 
  "imprints": [
    {
      "date": "2020-05-15", 
      "publisher": "APS"
    }
  ]
}