{
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  "authors": [
    {
      "raw_name": "Xiaoyong Chu", 
      "affiliations": [
        {
          "country": "Austria", 
          "value": "Institute of High Energy Physics, Austrian Academy of Sciences, Nikolsdorfer Gasse 18, 1050 Vienna, Austria"
        }
      ], 
      "surname": "Chu", 
      "given_names": "Xiaoyong", 
      "full_name": "Chu, Xiaoyong"
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    {
      "raw_name": "Camilo Garcia-Cely", 
      "affiliations": [
        {
          "country": "Germany", 
          "value": "Deutsches Elektronen-Synchrotron DESY, Notkestrasse 85, 22607 Hamburg, Germany"
        }
      ], 
      "surname": "Garcia-Cely", 
      "given_names": "Camilo", 
      "full_name": "Garcia-Cely, Camilo"
    }, 
    {
      "raw_name": "Hitoshi Murayama", 
      "affiliations": [
        {
          "country": "USA", 
          "value": "Department of Physics, University of California, Berkeley, California 94720, USA"
        }, 
        {
          "country": "Japan", 
          "value": "Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa 277-8583, Japan"
        }, 
        {
          "country": "USA", 
          "value": "Ernest Orlando Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA"
        }, 
        {
          "country": "Germany", 
          "value": "Deutsches Elektronen-Synchrotron DESY, Notkestrasse 85, 22607 Hamburg, Germany"
        }
      ], 
      "surname": "Murayama", 
      "given_names": "Hitoshi", 
      "full_name": "Murayama, Hitoshi"
    }
  ], 
  "titles": [
    {
      "source": "APS", 
      "title": "Velocity Dependence from Resonant Self-Interacting Dark Matter"
    }
  ], 
  "dois": [
    {
      "value": "10.1103/PhysRevLett.122.071103"
    }
  ], 
  "publication_info": [
    {
      "journal_volume": "122", 
      "journal_title": "Physical Review Letters", 
      "material": "article", 
      "journal_issue": "7", 
      "year": 2019
    }
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    "method": "APS", 
    "submission_number": "bca49440b8c511eaad8602163e01809a"
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  "page_nr": [
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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": "2019"
    }
  ], 
  "control_number": "45798", 
  "record_creation_date": "2019-02-22T14:30:15.139575", 
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  "arxiv_eprints": [
    {
      "categories": [
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      "value": "1810.04709"
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  ], 
  "abstracts": [
    {
      "source": "APS", 
      "value": "The dark matter density distribution in small-scale astrophysical objects may indicate that dark matter is self-interacting, while observations from clusters of galaxies suggest that the corresponding cross section depends on the velocity. Using a model-independent approach, we show that resonant self-interacting dark matter can naturally explain such a behavior. In contrast to what is often assumed, this does not require a light mediator. We present explicit realizations of this mechanism and discuss the corresponding astrophysical constraints."
    }
  ], 
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