<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:creator>Altarev, I.</dc:creator>
  <dc:creator>Ban, G.</dc:creator>
  <dc:creator>Bison, Georg</dc:creator>
  <dc:creator>Bodek, K.</dc:creator>
  <dc:creator>Daum, M.</dc:creator>
  <dc:creator>Fertl, M.</dc:creator>
  <dc:creator>Fierlinger, P.</dc:creator>
  <dc:creator>Franke, B.</dc:creator>
  <dc:creator>Gutsmiedl, E.</dc:creator>
  <dc:creator>Heil, W.</dc:creator>
  <dc:creator>Henneck, R.</dc:creator>
  <dc:creator>Horras, M.</dc:creator>
  <dc:creator>Khomutov, N.</dc:creator>
  <dc:creator>Kirch, K.</dc:creator>
  <dc:creator>Kistryn, S.</dc:creator>
  <dc:creator>Kraft, A.</dc:creator>
  <dc:creator>Knecht, A.</dc:creator>
  <dc:creator>Knowles, Paul E.</dc:creator>
  <dc:creator>Kozela, A.</dc:creator>
  <dc:creator>Lauer, T.</dc:creator>
  <dc:creator>Lauss, B.</dc:creator>
  <dc:creator>Lefort, T.</dc:creator>
  <dc:creator>Lemière, Y.</dc:creator>
  <dc:creator>Mtchedlishvili, A.</dc:creator>
  <dc:creator>Naviliat-Cuncic, O.</dc:creator>
  <dc:creator>Pazgalev, Anatoly S.</dc:creator>
  <dc:creator>Petzoldt, G.</dc:creator>
  <dc:creator>Piegsa, F. M.</dc:creator>
  <dc:creator>Pierre, E.</dc:creator>
  <dc:creator>Pignol, G.</dc:creator>
  <dc:creator>Quéméner, G.</dc:creator>
  <dc:creator>Rebetez, M.</dc:creator>
  <dc:creator>Rebreyend, D.</dc:creator>
  <dc:creator>Roccia, S.</dc:creator>
  <dc:creator>Schmidt-Wellenburg, P.</dc:creator>
  <dc:creator>Severijns, N.</dc:creator>
  <dc:creator>Sobolev, Yu.</dc:creator>
  <dc:creator>Weis, Antoine</dc:creator>
  <dc:creator>Zejma, J.</dc:creator>
  <dc:creator>Zenner, J.</dc:creator>
  <dc:creator>Zsigmond, G.</dc:creator>
  <dc:date>2010-10-06</dc:date>
  <dc:description xmlns:ns0="xml" ns0:lang="en">Physics at the Planck scale could be revealed by looking for tiny violations of fundamental symmetries in low energy experiments. In 2008, a sensitive test of the isotropy of the universe has been performed with stored ultracold neutrons (UCN), this is the first clock-comparison experiment performed with free neutrons. During several days we monitored the Larmor frequency of neutron spins in a weak magnetic field using the Ramsey resonance technique. A nonzero cosmic axial field, violating rotational symmetry, would induce a daily variation of the precession frequency. Our null result constitutes one of the most stringent tests of Lorentz invariance to date.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>https://folia.unifr.ch/global/documents/302081</dc:identifier>
  <dc:identifier>https://folia.unifr.ch/documents/302081/files/wei_tiu.pdf</dc:identifier>
  <dc:language>eng</dc:language>
  <dc:relation>info:eu-repo/semantics/altIdentifier/doi/10.1016/j.physb.2010.09.044</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>License undefined</dc:rights>
  <dc:source>Physica B: Condensed Matter. - 2011, vol. 406, no. 12, p. 2365-2369</dc:source>
  <dc:subject>info:eu-repo/classification/udc/53</dc:subject>
  <dc:title xmlns:ns1="xml" ns1:lang="en">Testing isotropy of the universe using the Ramsey resonance technique on ultracold neutron spins</dc:title>
  <dc:type>http://purl.org/coar/resource_type/c_6501</dc:type>
</oai_dc:dc>
