
<ns0:uwmetadata xmlns:ns0="http://phaidra.univie.ac.at/XML/metadata/V1.0" xmlns:ns1="http://phaidra.univie.ac.at/XML/metadata/lom/V1.0" xmlns:ns10="http://phaidra.univie.ac.at/XML/metadata/provenience/V1.0" xmlns:ns11="http://phaidra.univie.ac.at/XML/metadata/provenience/V1.0/entity" xmlns:ns12="http://phaidra.univie.ac.at/XML/metadata/digitalbook/V1.0" xmlns:ns13="http://phaidra.univie.ac.at/XML/metadata/etheses/V1.0" xmlns:ns2="http://phaidra.univie.ac.at/XML/metadata/extended/V1.0" xmlns:ns3="http://phaidra.univie.ac.at/XML/metadata/lom/V1.0/entity" xmlns:ns4="http://phaidra.univie.ac.at/XML/metadata/lom/V1.0/requirement" xmlns:ns5="http://phaidra.univie.ac.at/XML/metadata/lom/V1.0/educational" xmlns:ns6="http://phaidra.univie.ac.at/XML/metadata/lom/V1.0/annotation" xmlns:ns7="http://phaidra.univie.ac.at/XML/metadata/lom/V1.0/classification" xmlns:ns8="http://phaidra.univie.ac.at/XML/metadata/lom/V1.0/organization" xmlns:ns9="http://phaidra.univie.ac.at/XML/metadata/histkult/V1.0">
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    <ns1:identifier>o:1392</ns1:identifier>
    <ns1:title language="sr">Inflatorni kosmološki modeli sa tahionskim i radionskim poljima</ns1:title>
    <ns2:alt_title language="sr">Infationary cosmological models with tachyon and radion fields  : doctoral dissertation</ns2:alt_title>
    <ns1:language>sr</ns1:language>
    <ns1:description language="en">A popular class of the inflationary cosmological models is based
on an introduction of a scalar field with nonstandard tachyonic
Lagrangian of the Dirac-Born-Infeld (DBI) type. A potentially
fundamental role of the tachyon fields in the braneworld cosmology
was proposed by A. Sen. Research in this PhD thesis is
motivated by Randall-Sundrum (RSII) cosmological model. The
main objective of the research is to formulate and solve an analytical-
numerical inflationary model with DBI-tachyon field and
RSII model with an additional radion field, as well computation
of observational parameters. Obtained results are in a good
agreement with the real astrophysical data and provide a better
understanding of the role of strings and branes in modern cosmology.
The results indicated that role of radion in an initial
RSII setup is less important than expected.</ns1:description>
    <ns1:description language="sr">Biografija autora: list 95  Datum odbrane: 15.06.2017. Cosmology</ns1:description>
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    <ns1:status>45</ns1:status>
    <ns2:peer_reviewed>no</ns2:peer_reviewed>
    <ns1:contribute seq="0">
      <ns1:role>46</ns1:role>
      <ns1:ext_role>mentor</ns1:ext_role>
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        <ns3:firstname> Milan D. 1981- </ns3:firstname>
        <ns3:lastname>Milošević</ns3:lastname>
      </ns1:entity>
      <ns1:date>2017</ns1:date>
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      <ns1:role>63</ns1:role>
      <ns1:ext_role>mentor</ns1:ext_role>
      <ns1:entity seq="0">
        <ns3:firstname> Goran 1963- </ns3:firstname>
        <ns3:lastname>Đorđević</ns3:lastname>
      </ns1:entity>
      <ns1:date>2017</ns1:date>
    </ns1:contribute>
    <ns1:contribute seq="2">
      <ns1:role>63</ns1:role>
      <ns1:ext_role>član komisije</ns1:ext_role>
      <ns1:entity seq="0">
        <ns3:firstname> Ljubiša 1966- </ns3:firstname>
        <ns3:lastname>Nešić</ns3:lastname>
      </ns1:entity>
      <ns1:date>2017</ns1:date>
    </ns1:contribute>
    <ns1:contribute seq="3">
      <ns1:role>63</ns1:role>
      <ns1:ext_role>član komisije</ns1:ext_role>
      <ns1:entity seq="0">
        <ns3:firstname> Predrag </ns3:firstname>
        <ns3:lastname>Jovanović</ns3:lastname>
      </ns1:entity>
      <ns1:date>2017</ns1:date>
    </ns1:contribute>
  </ns1:lifecycle>
  <ns1:technical>
    <ns1:format>95 listova</ns1:format>
    <ns1:size>2915724</ns1:size>
    <ns1:location>http://phaidrabg.bg.ac.rs/o:1392</ns1:location>
  </ns1:technical>
  <ns1:rights>
    <ns1:cost>no</ns1:cost>
    <ns1:copyright>yes</ns1:copyright>
    <ns1:license>5</ns1:license>
  </ns1:rights>
  <ns1:annotation>
    <ns6:annotations>
      <ns6:date>2017-09-04T18:22:27.320Z</ns6:date>
    </ns6:annotations>
  </ns1:annotation>
  <ns1:classification>
    <ns1:purpose>70</ns1:purpose>
    <ns7:keyword language="sr" seq="1">Kosmologija, inflacija, Randal-Sundrum model, DBI la-granžijan, tahioni</ns7:keyword>
    <ns7:keyword language="sr" seq="1">Cosmology, inflation, Randal-Sundrum model, DBI Lagrangian,tachyons</ns7:keyword>
    <ns7:keyword language="sr" seq="1">524.82:524.834</ns7:keyword>
    <ns7:keyword language="sr" seq="1">P 210</ns7:keyword>
  </ns1:classification>
  <ns1:organization>
    <ns8:hoschtyp>1738</ns8:hoschtyp>
    <ns8:orgassignment>
      <ns8:faculty>18A07</ns8:faculty>
      <ns8:department>18A0702</ns8:department>
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  <ns12:digitalbook>
    <ns12:releaseyear>2017</ns12:releaseyear>
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