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  "authors": [
    {
      "affiliations": [
        {
          "country": "Pakistan", 
          "value": "Institute of Physics, Gomal University, Dera Ismail Khan, Khyber Pakhtunkhwa, 29220, Pakistan", 
          "organization": "Gomal University"
        }
      ], 
      "surname": "Ilyas", 
      "email": "ilyas_mia@yahoo.com", 
      "full_name": "Ilyas, M.", 
      "given_names": "M."
    }, 
    {
      "affiliations": [
        {
          "country": "Pakistan", 
          "value": "Department of Physics, Abdul Wali khan University Mardan, Mardan, 23200, Pakistan", 
          "organization": "Abdul Wali khan University Mardan"
        }
      ], 
      "surname": "Rahman", 
      "email": "waheed71rahman@gmail.com", 
      "full_name": "Rahman, W.", 
      "given_names": "W."
    }
  ], 
  "titles": [
    {
      "source": "Springer", 
      "title": "Bounce cosmology in  $$f({\\mathcal {R}})$$  <math> <mrow> <mi>f</mi> <mo>(</mo> <mi>R</mi> <mo>)</mo> </mrow> </math>   gravity"
    }
  ], 
  "dois": [
    {
      "value": "10.1140/epjc/s10052-021-08955-7"
    }
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  "publication_info": [
    {
      "page_end": "9", 
      "journal_title": "European Physical Journal C", 
      "material": "article", 
      "journal_volume": "81", 
      "artid": "s10052-021-08955-7", 
      "year": 2021, 
      "page_start": "1", 
      "journal_issue": "2"
    }
  ], 
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    "date": "2021-05-27T13:37:58.551698", 
    "source": "Springer", 
    "method": "Springer", 
    "submission_number": "b8115dbebef011eb92440a580a640a05"
  }, 
  "page_nr": [
    9
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  "license": [
    {
      "url": "https://creativecommons.org/licenses//by/4.0", 
      "license": "CC-BY-4.0"
    }
  ], 
  "copyright": [
    {
      "holder": "The Author(s)", 
      "year": "2021"
    }
  ], 
  "control_number": "60122", 
  "record_creation_date": "2021-02-16T22:30:24.597702", 
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  "collections": [
    {
      "primary": "European Physical Journal C"
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  ], 
  "abstracts": [
    {
      "source": "Springer", 
      "value": "In this paper, we analyze the modified  $$f({\\mathcal {R}})$$  <math> <mrow> <mi>f</mi> <mo>(</mo> <mi>R</mi> <mo>)</mo> </mrow> </math>   gravity models in Friedmann\u2013Lema\u00eetre\u2013Robertson\u2013Walker (FLRW) background. The actions of bouncing cosmology are studied under consideration of different viable models in  $$f({\\mathcal {R}})$$  <math> <mrow> <mi>f</mi> <mo>(</mo> <mi>R</mi> <mo>)</mo> </mrow> </math>   gravity theory that can resolve the difficulty of singularity in standard Big-Bang cosmology. Under different viable models in  $$f({\\mathcal {R}})$$  <math> <mrow> <mi>f</mi> <mo>(</mo> <mi>R</mi> <mo>)</mo> </mrow> </math>   gravity theory, the cosmological constraints are plotted in provisions of cosmic-time, then investigated the bounce circumstance. In addition, the red-shift parameter is used to reconstruct the modified gravity, and compile the cosmological parameters that infer accelerated universe expansion. Finally, the situation stability is evaluated with a sound speed feature, which illustrates late-time stability."
    }
  ], 
  "imprints": [
    {
      "date": "2021-02-16", 
      "publisher": "Springer"
    }
  ]
}