{
  "_oai": {
    "updated": "2022-10-27T06:30:43Z", 
    "id": "oai:repo.scoap3.org:62642", 
    "sets": [
      "EPJC"
    ]
  }, 
  "authors": [
    {
      "affiliations": [
        {
          "country": "Poland", 
          "value": "Institute of Theoretical physics, University of Wroclaw, pl. Maxa Borna 9, Wroc\u0142aw, 50-206, Poland", 
          "organization": "University of Wroclaw"
        }
      ], 
      "surname": "Kozak", 
      "email": "aleksander.kozak@uwr.edu.pl", 
      "full_name": "Kozak, Aleksander", 
      "given_names": "Aleksander"
    }, 
    {
      "affiliations": [
        {
          "country": "Estonia", 
          "value": "Laboratory of Theoretical Physics, Institute of Physics, University of Tartu, W. Ostwaldi 1, Tartu, 50411, Estonia", 
          "organization": "University of Tartu"
        }
      ], 
      "surname": "Wojnar", 
      "email": "aneta.magdalena.wojnar@ut.ee", 
      "full_name": "Wojnar, Aneta", 
      "given_names": "Aneta"
    }
  ], 
  "titles": [
    {
      "source": "Springer", 
      "title": "Invariant quantities of scalar\u2013tensor theories for stellar structure"
    }
  ], 
  "dois": [
    {
      "value": "10.1140/epjc/s10052-021-09277-4"
    }
  ], 
  "publication_info": [
    {
      "page_end": "12", 
      "journal_title": "European Physical Journal C", 
      "material": "article", 
      "journal_volume": "81", 
      "artid": "s10052-021-09277-4", 
      "year": 2021, 
      "page_start": "1", 
      "journal_issue": "6"
    }
  ], 
  "$schema": "http://repo.scoap3.org/schemas/hep.json", 
  "acquisition_source": {
    "date": "2022-10-27T06:30:27.766596", 
    "source": "Springer", 
    "method": "Springer", 
    "submission_number": "c8601f5855c011eda33ab6e03099cfc1"
  }, 
  "page_nr": [
    12
  ], 
  "license": [
    {
      "url": "https://creativecommons.org/licenses//by/4.0", 
      "license": "CC-BY-4.0"
    }
  ], 
  "copyright": [
    {
      "holder": "The Author(s)", 
      "year": "2021"
    }
  ], 
  "control_number": "62642", 
  "record_creation_date": "2021-06-04T00:30:34.361866", 
  "_files": [
    {
      "checksum": "md5:f2dbb29e4267cb6e977d72391a0f290c", 
      "filetype": "xml", 
      "bucket": "ca8c4d8e-0eb6-40a2-abb7-35299df0ec09", 
      "version_id": "91c86bd9-4c75-420d-963c-01fc7883acde", 
      "key": "10.1140/epjc/s10052-021-09277-4.xml", 
      "size": 10559
    }, 
    {
      "checksum": "md5:4aa45ceb1cb24d1873e092683bd8d0be", 
      "filetype": "pdf/a", 
      "bucket": "ca8c4d8e-0eb6-40a2-abb7-35299df0ec09", 
      "version_id": "22e2d1e5-5d53-4d21-b39a-fea93c52abe3", 
      "key": "10.1140/epjc/s10052-021-09277-4_a.pdf", 
      "size": 375807
    }
  ], 
  "collections": [
    {
      "primary": "European Physical Journal C"
    }
  ], 
  "abstracts": [
    {
      "source": "Springer", 
      "value": "We present the relativistic hydrostatic equilibrium equations for a wide class of gravitational theories possessing a scalar\u2013tensor representation. It turns out that the stellar structure equations can be written with respect to the scalar\u2013tensor invariants, allowing to interpret their physical role."
    }
  ], 
  "imprints": [
    {
      "date": "2021-06-03", 
      "publisher": "Springer"
    }
  ]
}