<?xml version="1.0" encoding="UTF-8"?>
<collection xmlns="http://www.loc.gov/MARC21/slim">
<record>
  <controlfield tag="001">75418</controlfield>
  <controlfield tag="005">20250113143110.0</controlfield>
  <datafield tag="024" ind1="7" ind2=" ">
    <subfield code="2">doi</subfield>
    <subfield code="a">10.1088/1475-7516/2017/10/010</subfield>
  </datafield>
  <datafield tag="024" ind1="8" ind2=" ">
    <subfield code="2">sideral</subfield>
    <subfield code="a">103627</subfield>
  </datafield>
  <datafield tag="037" ind1=" " ind2=" ">
    <subfield code="a">ART-2017-103627</subfield>
  </datafield>
  <datafield tag="041" ind1=" " ind2=" ">
    <subfield code="a">eng</subfield>
  </datafield>
  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="a">Giannotti, M.</subfield>
    <subfield code="0">(orcid)0000-0001-9823-6262</subfield>
  </datafield>
  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">Stellar recipes for Axion hunters</subfield>
  </datafield>
  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">2017</subfield>
  </datafield>
  <datafield tag="506" ind1="0" ind2=" ">
    <subfield code="a">Access copy available to the general public</subfield>
    <subfield code="f">Unrestricted</subfield>
  </datafield>
  <datafield tag="520" ind1="3" ind2=" ">
    <subfield code="a">There are a number of observational hints from astrophysics which point to the existence of stellar energy losses beyond the ones accounted for by neutrino emission. These excessive energy losses may be explained by the existence of a new sub-keV mass pseudoscalar Nambu-Goldstone boson with tiny couplings to photons, electrons, and nucleons. An attractive possibility is to identify this particle with the axion-the hypothetical pseudo Nambu-Goldstone boson predicted by the Peccei-Quinn solution to the strong CP problem. We explore this possibility in terms of a DFSZ-type axion and of a KSVZ-type axion/majoron, respectively. Both models allow a good globalt to the data, prefering an axion mass around 10 meV. We show that future axion experiments-the fifth force experiment ARIADNE and the helioscope IAXO-can attack the preferred mass range from the lower and higher end, respectively. An axion in this mass range can also be the main constituent of dark matter.</subfield>
  </datafield>
  <datafield tag="536" ind1=" " ind2=" ">
    <subfield code="9">info:eu-repo/grantAgreement/ES/MINECO/FPA2015-65745-P</subfield>
    <subfield code="9">info:eu-repo/grantAgreement/ES/MINECO/RYC-2012-10597</subfield>
  </datafield>
  <datafield tag="540" ind1=" " ind2=" ">
    <subfield code="9">info:eu-repo/semantics/openAccess</subfield>
    <subfield code="a">by-nc-nd</subfield>
    <subfield code="u">http://creativecommons.org/licenses/by-nc-nd/3.0/es/</subfield>
  </datafield>
  <datafield tag="590" ind1=" " ind2=" ">
    <subfield code="a">5.126</subfield>
    <subfield code="b">2017</subfield>
  </datafield>
  <datafield tag="591" ind1=" " ind2=" ">
    <subfield code="a">PHYSICS, PARTICLES &amp; FIELDS</subfield>
    <subfield code="b">6 / 29 = 0.207</subfield>
    <subfield code="c">2017</subfield>
    <subfield code="d">Q1</subfield>
    <subfield code="e">T1</subfield>
  </datafield>
  <datafield tag="591" ind1=" " ind2=" ">
    <subfield code="a">ASTRONOMY &amp; ASTROPHYSICS</subfield>
    <subfield code="b">13 / 65 = 0.2</subfield>
    <subfield code="c">2017</subfield>
    <subfield code="d">Q1</subfield>
    <subfield code="e">T1</subfield>
  </datafield>
  <datafield tag="592" ind1=" " ind2=" ">
    <subfield code="a">1.089</subfield>
    <subfield code="b">2017</subfield>
  </datafield>
  <datafield tag="593" ind1=" " ind2=" ">
    <subfield code="a">Astronomy and Astrophysics</subfield>
    <subfield code="c">2017</subfield>
    <subfield code="d">Q2</subfield>
  </datafield>
  <datafield tag="655" ind1=" " ind2="4">
    <subfield code="a">info:eu-repo/semantics/article</subfield>
    <subfield code="v">info:eu-repo/semantics/acceptedVersion</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Irastorza, I.G.</subfield>
    <subfield code="u">Universidad de Zaragoza</subfield>
    <subfield code="0">(orcid)0000-0003-1163-1687</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Redondo, J.</subfield>
    <subfield code="u">Universidad de Zaragoza</subfield>
    <subfield code="0">(orcid)0000-0002-1044-8197</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Ringwald, A.</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Saikawa, K.</subfield>
  </datafield>
  <datafield tag="710" ind1="2" ind2=" ">
    <subfield code="1">2004</subfield>
    <subfield code="2">405</subfield>
    <subfield code="a">Universidad de Zaragoza</subfield>
    <subfield code="b">Dpto. Física Teórica</subfield>
    <subfield code="c">Área Física Teórica</subfield>
  </datafield>
  <datafield tag="710" ind1="2" ind2=" ">
    <subfield code="1">2004</subfield>
    <subfield code="2">390</subfield>
    <subfield code="a">Universidad de Zaragoza</subfield>
    <subfield code="b">Dpto. Física Teórica</subfield>
    <subfield code="c">Área Física Atóm.Molec.y Nucl.</subfield>
  </datafield>
  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="g">2017, 10 (2017), [33 pp]</subfield>
    <subfield code="p">J. Cosmol. Astropart. Phys.</subfield>
    <subfield code="t">Journal of Cosmology and Astroparticle Physics</subfield>
    <subfield code="x">1475-7516</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2=" ">
    <subfield code="s">918263</subfield>
    <subfield code="u">http://zaguan.unizar.es/record/75418/files/texto_completo.pdf</subfield>
    <subfield code="y">Postprint</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2=" ">
    <subfield code="s">63176</subfield>
    <subfield code="u">http://zaguan.unizar.es/record/75418/files/texto_completo.jpg?subformat=icon</subfield>
    <subfield code="x">icon</subfield>
    <subfield code="y">Postprint</subfield>
  </datafield>
  <datafield tag="909" ind1="C" ind2="O">
    <subfield code="o">oai:zaguan.unizar.es:75418</subfield>
    <subfield code="p">articulos</subfield>
    <subfield code="p">driver</subfield>
  </datafield>
  <datafield tag="951" ind1=" " ind2=" ">
    <subfield code="a">2025-01-13-14:30:22</subfield>
  </datafield>
  <datafield tag="980" ind1=" " ind2=" ">
    <subfield code="a">ARTICLE</subfield>
  </datafield>
</record>
</collection>