<?xml version="1.0" encoding="ISO-8859-1"?><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
<front>
<journal-meta>
<journal-id>0370-3908</journal-id>
<journal-title><![CDATA[Revista de la Academia Colombiana de Ciencias Exactas, Físicas y Naturales]]></journal-title>
<abbrev-journal-title><![CDATA[Rev. acad. colomb. cienc. exact. fis. nat.]]></abbrev-journal-title>
<issn>0370-3908</issn>
<publisher>
<publisher-name><![CDATA[Academia Colombiana de Ciencias Exactas, Físicas y Naturales]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S0370-39082020000100133</article-id>
<article-id pub-id-type="doi">10.18257/raccefyn.966</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[The Scalar Field Model of Dark Energy in the Framework of the Holographic Principle]]></article-title>
<article-title xml:lang="es"><![CDATA[El modelo del campo escalar de la energía oscura en el marco del principio holográfico]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Granda]]></surname>
<given-names><![CDATA[Luis Norberto]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
</contrib-group>
<aff id="Af1">
<institution><![CDATA[,Universidad del Valle  ]]></institution>
<addr-line><![CDATA[Cali ]]></addr-line>
<country>Colombia</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>03</month>
<year>2020</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>03</month>
<year>2020</year>
</pub-date>
<volume>44</volume>
<numero>170</numero>
<fpage>133</fpage>
<lpage>141</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.co/scielo.php?script=sci_arttext&amp;pid=S0370-39082020000100133&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.co/scielo.php?script=sci_abstract&amp;pid=S0370-39082020000100133&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.co/scielo.php?script=sci_pdf&amp;pid=S0370-39082020000100133&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[Abstract We study cosmological solutions for a scalar field minimally coupled to the curvature, in the framework of holographic dark energy. Phantom solutions can be obtained without introducing ghosts' degrees of freedom, and the autonomous system contains stable accelerated expansion solutions and de Sitter attractors. For the non-minimally coupled scalar field the special case of the conformal coupling is analyzed, and it is shown that dynamically evolving scalar field produces the effect of the cosmological constant.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[Resumen Se estudian soluciones cosmológicas para un campo escalar acoplado mínimamente a la curvatura, en el marco del principio holográfico. Se pueden obtener soluciones phantom sin introducir grados de libertad fantasma, y el sistema autónomo contiene soluciones de expansión acelerada estables y atractores de Sitter. Para el campo con acoplamiento no-mínimo se analiza el caso especial del acoplamiento conforme y se demuestra que un campo escalar que evoluciona dinámicamente puede producir el efecto de la constante cosmológica.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Dark Energy]]></kwd>
<kwd lng="en"><![CDATA[Holographic Principle]]></kwd>
<kwd lng="en"><![CDATA[Scalar Field]]></kwd>
<kwd lng="es"><![CDATA[Energía Oscura]]></kwd>
<kwd lng="es"><![CDATA[Principio Holográfico]]></kwd>
<kwd lng="es"><![CDATA[Campo Escalar]]></kwd>
</kwd-group>
</article-meta>
</front><back>
<ref-list>
<ref id="B1">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Ade]]></surname>
<given-names><![CDATA[P. A. R.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Planck 2015 Results. XIII. Cosmological Parameters]]></article-title>
<source><![CDATA[Astron. And Astrophys]]></source>
<year>2016</year>
<volume>594</volume>
<page-range>1-63</page-range></nlm-citation>
</ref>
<ref id="B2">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Arkani-Hamed]]></surname>
<given-names><![CDATA[N.]]></given-names>
</name>
<name>
<surname><![CDATA[Cheng]]></surname>
<given-names><![CDATA[H.]]></given-names>
</name>
<name>
<surname><![CDATA[Luty]]></surname>
<given-names><![CDATA[M A.]]></given-names>
</name>
<name>
<surname><![CDATA[Mukohyama]]></surname>
<given-names><![CDATA[S.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Ghost Condensation and consistent infrared Modification of Gravity]]></article-title>
<source><![CDATA[JHEP]]></source>
<year>2004</year>
<volume>074</volume>
<page-range>1-35</page-range></nlm-citation>
</ref>
<ref id="B3">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Armendariz-Picon]]></surname>
<given-names><![CDATA[C.]]></given-names>
</name>
<name>
<surname><![CDATA[Mukhanov]]></surname>
<given-names><![CDATA[V.]]></given-names>
</name>
<name>
<surname><![CDATA[Steinhardt]]></surname>
<given-names><![CDATA[P. J.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[A dynamical solution to the problem of a small cosmological constant and late-time cosmic acceleration]]></article-title>
<source><![CDATA[Phys. Rev. Lett]]></source>
<year>2000</year>
<volume>85</volume>
<page-range>4438-21</page-range></nlm-citation>
</ref>
<ref id="B4">
<nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Birrell]]></surname>
<given-names><![CDATA[N.D.]]></given-names>
</name>
<name>
<surname><![CDATA[Davis]]></surname>
<given-names><![CDATA[P.C.W.]]></given-names>
</name>
</person-group>
<source><![CDATA[Quantum fields in curved space-time]]></source>
<year>1982</year>
<publisher-loc><![CDATA[Cambridge, United Kingdom ]]></publisher-loc>
<publisher-name><![CDATA[Cambridge University Press]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B5">
<nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Bousso]]></surname>
<given-names><![CDATA[R.]]></given-names>
</name>
</person-group>
<source><![CDATA[A Covariant Entropy Conjecture]]></source>
<year>1999</year>
<volume>9907</volume>
<page-range>1-33</page-range><publisher-name><![CDATA[JHEP]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B6">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Caldwell]]></surname>
<given-names><![CDATA[R. R.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[A phantom menace? Cosmological consequences of a dark energy component with super-negative equation of state]]></article-title>
<source><![CDATA[Phys. Lett]]></source>
<year>2002</year>
<volume>545</volume>
<page-range>23-9</page-range></nlm-citation>
</ref>
<ref id="B7">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Cohen]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
<name>
<surname><![CDATA[Kaplan]]></surname>
<given-names><![CDATA[D.]]></given-names>
</name>
<name>
<surname><![CDATA[Nelson]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Effective Field Theory, Black Holes, and the Cosmological Constant]]></article-title>
<source><![CDATA[Phys. Rev. Lett]]></source>
<year>1999</year>
<volume>82</volume>
<page-range>4971-4</page-range></nlm-citation>
</ref>
<ref id="B8">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Ford]]></surname>
<given-names><![CDATA[L.H]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Gravitational Particle creation and Inflation]]></article-title>
<source><![CDATA[Phys. Rev]]></source>
<year>1987</year>
<volume>D35</volume>
<page-range>2955-60</page-range></nlm-citation>
</ref>
<ref id="B9">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Granda]]></surname>
<given-names><![CDATA[L. N.]]></given-names>
</name>
<name>
<surname><![CDATA[Jimenez]]></surname>
<given-names><![CDATA[D. F.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Dynamical Analysis for a Scalar-Tensor Model with Gauss-Bonnet and Non-Minimal couplings]]></article-title>
<source><![CDATA[Eur. Phys. J. C]]></source>
<year>2017</year>
<volume>77</volume>
<numero>679</numero>
<issue>679</issue>
<page-range>1-12</page-range></nlm-citation>
</ref>
<ref id="B10">
<nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Granda]]></surname>
<given-names><![CDATA[L. N.]]></given-names>
</name>
<name>
<surname><![CDATA[Jimenez]]></surname>
<given-names><![CDATA[D. F.]]></given-names>
</name>
</person-group>
<source><![CDATA[Dynamical Analysis for a Scalar-Tensor Model with Kinetic and Non-Minimal couplings]]></source>
<year>2018</year>
<volume>27</volume>
<page-range>1-22</page-range><publisher-name><![CDATA[IJMPD]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B11">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Granda]]></surname>
<given-names><![CDATA[L. N.]]></given-names>
</name>
<name>
<surname><![CDATA[Oliveros]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Infrared Cut-off Proposal for the Holographic Density]]></article-title>
<source><![CDATA[Phys. Lett]]></source>
<year>2008</year>
<volume>669</volume>
<page-range>275-7</page-range></nlm-citation>
</ref>
<ref id="B12">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Granda]]></surname>
<given-names><![CDATA[L. N.]]></given-names>
</name>
<name>
<surname><![CDATA[Oliveros]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[New Infrared Cut-off for the Holographic Scalar Fields Models of Dark Energy]]></article-title>
<source><![CDATA[Phys. Lett]]></source>
<year>2008</year>
<month>a</month>
<volume>671</volume>
<page-range>199-202</page-range></nlm-citation>
</ref>
<ref id="B13">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Hicken]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Improved dark Energy Constraints from ~100 New CFA Supernova Type Ia Light Curves]]></article-title>
<source><![CDATA[Astrophys. J]]></source>
<year>2009</year>
<volume>700</volume>
<page-range>1097-140</page-range></nlm-citation>
</ref>
<ref id="B14">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Hsu]]></surname>
<given-names><![CDATA[S. D.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Entropy Bounds and Dark Energy]]></article-title>
<source><![CDATA[Phys. Lett]]></source>
<year>2004</year>
<volume>594</volume>
<page-range>13-6</page-range></nlm-citation>
</ref>
<ref id="B15">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Ito]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Holographic Dark Energy Model with Non-minimal Coupling]]></article-title>
<source><![CDATA[Europhys. Lett]]></source>
<year>2005</year>
<volume>71</volume>
<page-range>712-5</page-range></nlm-citation>
</ref>
<ref id="B16">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Kowalski]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Improved Cosmological Constraints from New, Old and Combined Supernova Datasets]]></article-title>
<source><![CDATA[Astrophys. Journal]]></source>
<year>2008</year>
<volume>686</volume>
<page-range>749-78</page-range></nlm-citation>
</ref>
<ref id="B17">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Padmanabhan]]></surname>
<given-names><![CDATA[T.]]></given-names>
</name>
<name>
<surname><![CDATA[Choudhury]]></surname>
<given-names><![CDATA[T. R.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Can the Clustered dark matter and the smooth dark energy arise from the same scalar field?]]></article-title>
<source><![CDATA[Phys. Rev]]></source>
<year>2002</year>
<volume>66</volume>
<page-range>081301</page-range></nlm-citation>
</ref>
<ref id="B18">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Perlmutter]]></surname>
<given-names><![CDATA[S.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Constant]]></article-title>
<source><![CDATA[Nature]]></source>
<year>1988</year>
<volume>391</volume>
<page-range>51-4</page-range></nlm-citation>
</ref>
<ref id="B19">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Perivolaropoulos]]></surname>
<given-names><![CDATA[L.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Crossing the Phantom Divide Barrier with Scalar-Tensor Theories]]></article-title>
<source><![CDATA[JCAP]]></source>
<year>2005</year>
<volume>001</volume>
<page-range>1-16</page-range></nlm-citation>
</ref>
<ref id="B20">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Ratra]]></surname>
<given-names><![CDATA[B.]]></given-names>
</name>
<name>
<surname><![CDATA[Peebles]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Cosmological consequences of a rolling homogeneous scalar field]]></article-title>
<source><![CDATA[Phys. Rev]]></source>
<year>1988</year>
<volume>D37</volume>
<page-range>3406-27</page-range></nlm-citation>
</ref>
<ref id="B21">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Riess]]></surname>
<given-names><![CDATA[A.G.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant]]></article-title>
<source><![CDATA[Astron. J]]></source>
<year>1998</year>
<volume>116</volume>
<page-range>1009-38</page-range></nlm-citation>
</ref>
<ref id="B22">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Sami]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<name>
<surname><![CDATA[Shahalam]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<name>
<surname><![CDATA[Skugoreva]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<name>
<surname><![CDATA[Toporensky]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Cosmological Dynamics of Non-Minimally Coupled scalar Field system and Its late Time Cosmic Relevance]]></article-title>
<source><![CDATA[Phys. Rev]]></source>
<year>2012</year>
<volume>86</volume>
<page-range>1-17</page-range></nlm-citation>
</ref>
<ref id="B23">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Setare]]></surname>
<given-names><![CDATA[M.R.]]></given-names>
</name>
<name>
<surname><![CDATA[Saridakis]]></surname>
<given-names><![CDATA[E.N.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Non-minimally Coupled Canonical, Phantom and Quintom Models of Holographic Dark Energy]]></article-title>
<source><![CDATA[Phys. Lett]]></source>
<year>2009</year>
<volume>B671</volume>
<page-range>331-8</page-range></nlm-citation>
</ref>
<ref id="B24">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Susskind]]></surname>
<given-names><![CDATA[L.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[The World as a Hologram]]></article-title>
<source><![CDATA[J. Math. Phys]]></source>
<year>1995</year>
<volume>36</volume>
<page-range>6377-96</page-range></nlm-citation>
</ref>
<ref id="B25">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA['t Hooft]]></surname>
<given-names><![CDATA[G.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Dimensional Reduction in Quantum Gravity]]></article-title>
<source><![CDATA[arXiv]]></source>
<year>1993</year>
</nlm-citation>
</ref>
</ref-list>
</back>
</article>
