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  "authors": [
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      "affiliations": [
        {
          "country": "Chile", 
          "value": "Universidad Adolfo Ib\u00e0\u00f1ez, Departamento de Ciencias, Facultad de Artes Liberales, Av. Padre Hurtado, Vi\u00f1a del Mar, 750, Chile", 
          "organization": "Universidad Adolfo Ib\u00e0\u00f1ez, Departamento de Ciencias, Facultad de Artes Liberales"
        }
      ], 
      "surname": "Anabal\u00f3n", 
      "email": "andres.anabalon@uai.cl", 
      "full_name": "Anabal\u00f3n, A.", 
      "given_names": "A."
    }, 
    {
      "affiliations": [
        {
          "country": "Chile", 
          "value": "Pontificia Universidad Cat\u00f3lica de Valpara\u00edso, Instituto de F\u00edsica, Av. Brasil, Valpara\u00edso, 2950, Chile", 
          "organization": "Pontificia Universidad Cat\u00f3lica de Valpara\u00edso, Instituto de F\u00edsica"
        }
      ], 
      "surname": "Astefanesei", 
      "email": "dumitru.astefanesei@pucv.cl", 
      "full_name": "Astefanesei, D.", 
      "given_names": "D."
    }, 
    {
      "affiliations": [
        {
          "country": "Chile", 
          "value": "Universidad Adolfo Ib\u00e0\u00f1ez, Departamento de Ciencias, Facultad de Artes Liberales, Av. Padre Hurtado, Vi\u00f1a del Mar, 750, Chile", 
          "organization": "Universidad Adolfo Ib\u00e0\u00f1ez, Departamento de Ciencias, Facultad de Artes Liberales"
        }
      ], 
      "surname": "Choque", 
      "email": "david.choque@pucv.cl", 
      "full_name": "Choque, D.", 
      "given_names": "D."
    }, 
    {
      "affiliations": [
        {
          "country": "Italy", 
          "value": "Politecnico di Torino, Dipartimento DISAT, Corso Duca degli Abruzzi 24, Torino, 10129, Italy", 
          "organization": "Politecnico di Torino, Dipartimento DISAT"
        }, 
        {
          "country": "Italy", 
          "value": "Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Torino, Via Pietro Giuria 1, Torino, Italy", 
          "organization": "Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Torino"
        }
      ], 
      "surname": "Gallerati", 
      "email": "antonio.gallerati@polito.it", 
      "full_name": "Gallerati, A.", 
      "given_names": "A."
    }, 
    {
      "affiliations": [
        {
          "country": "Italy", 
          "value": "Politecnico di Torino, Dipartimento DISAT, Corso Duca degli Abruzzi 24, Torino, 10129, Italy", 
          "organization": "Politecnico di Torino, Dipartimento DISAT"
        }, 
        {
          "country": "Italy", 
          "value": "Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Torino, Via Pietro Giuria 1, Torino, Italy", 
          "organization": "Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Torino"
        }
      ], 
      "surname": "Trigiante", 
      "email": "mario.trigiante@polito.it", 
      "full_name": "Trigiante, M.", 
      "given_names": "M."
    }
  ], 
  "titles": [
    {
      "source": "Springer", 
      "title": "Exact holographic RG flows in extended SUGRA"
    }
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  "dois": [
    {
      "value": "10.1007/JHEP04(2021)053"
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  "publication_info": [
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      "page_end": "29", 
      "journal_title": "Journal of High Energy Physics", 
      "material": "article", 
      "journal_volume": "2021", 
      "artid": "JHEP04(2021)053", 
      "year": 2021, 
      "page_start": "1", 
      "journal_issue": "4"
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      "url": "https://creativecommons.org/licenses//by/4.0", 
      "license": "CC-BY-4.0"
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  "copyright": [
    {
      "holder": "The Author(s)", 
      "year": "2021"
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  "control_number": "61234", 
  "record_creation_date": "2021-04-08T14:30:26.310937", 
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  "arxiv_eprints": [
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      "value": "2012.01289"
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  "abstracts": [
    {
      "source": "Springer", 
      "value": "We present a family of exact planar hairy neutral black hole solutions in extended supergravity with Fayet-Iliopoulos (FI) terms. We consider a model where the magnetic part of FI sector vanishes and obtain the superpotential at finite temperature in analytic form. Then, we discuss the thermodynamics and some holographic properties of these solutions. We regularize the action by two different methods, one with gravitational and scalar counterterms and the other using the thermal superpotential as a counterterm, and compute the holographic stress tensor. We also construct the c-function of the corresponding RG flow and obtain an exact holographic \u03b2-function for this model."
    }
  ], 
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    {
      "date": "2021-04-07", 
      "publisher": "Springer"
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