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  "authors": [
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      "raw_name": "Kristjan Kannike", 
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          "country": "Estonia", 
          "value": "National Institute of Chemical Physics and Biophysics, R\u00e4vala 10, Tallinn 10143, Estonia"
        }
      ], 
      "surname": "Kannike", 
      "given_names": "Kristjan", 
      "full_name": "Kannike, Kristjan"
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    {
      "raw_name": "Kaius Loos", 
      "affiliations": [
        {
          "country": "Estonia", 
          "value": "National Institute of Chemical Physics and Biophysics, R\u00e4vala 10, Tallinn 10143, Estonia"
        }
      ], 
      "surname": "Loos", 
      "given_names": "Kaius", 
      "full_name": "Loos, Kaius"
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    {
      "raw_name": "Martti Raidal", 
      "affiliations": [
        {
          "country": "Estonia", 
          "value": "National Institute of Chemical Physics and Biophysics, R\u00e4vala 10, Tallinn 10143, Estonia"
        }
      ], 
      "surname": "Raidal", 
      "given_names": "Martti", 
      "full_name": "Raidal, Martti"
    }
  ], 
  "titles": [
    {
      "source": "APS", 
      "title": "Gravitational wave signals of pseudo-Goldstone dark matter in the <math><msub><mi>Z</mi><mn>3</mn></msub></math> complex singlet model"
    }
  ], 
  "dois": [
    {
      "value": "10.1103/PhysRevD.101.035001"
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  "publication_info": [
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      "journal_volume": "101", 
      "journal_title": "Physical Review D", 
      "material": "article", 
      "journal_issue": "3", 
      "year": 2020
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    "submission_number": "810b323c058f11ecb53772fd3742099d"
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  "page_nr": [
    10
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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": "2020"
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  "record_creation_date": "2020-02-03T17:30:05.608995", 
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  "arxiv_eprints": [
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      "categories": [
        "hep-ph"
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      "value": "1907.13136"
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  ], 
  "abstracts": [
    {
      "source": "APS", 
      "value": "We study pseudo-Goldstone dark matter in the <math><msub><mi>Z</mi><mn>3</mn></msub></math> complex scalar singlet model. Because the direct detection spin-independent cross section is suppressed, such dark matter is allowed in a large mass range. Unlike in the original model stabilized by a parity and due to the cubic coupling of the singlet, the <math><msub><mi>Z</mi><mn>3</mn></msub></math> model can accommodate first-order phase transitions that give rise to a stochastic gravitational wave signal potentially observable in future space-based detectors."
    }
  ], 
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      "date": "2020-02-03", 
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