<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>Maillard, Yves-Patrick</dc:creator>
  <dc:creator>Dousse, Jean-Claude</dc:creator>
  <dc:creator>Hoszowska, Joanna</dc:creator>
  <dc:creator>Berset, Michel</dc:creator>
  <dc:creator>Mauron, Olivier</dc:creator>
  <dc:creator>Raboud, Pierre-Alexandre</dc:creator>
  <dc:creator>Kavčič, Matjaz</dc:creator>
  <dc:creator>Rzadkiewicz, J.</dc:creator>
  <dc:creator>Banaś, Dariusz</dc:creator>
  <dc:creator>Tökési, K.</dc:creator>
  <dc:date>2018-07-10</dc:date>
  <dc:description xmlns:ns0="xml" ns0:lang="en">We report on the radiative decay of double K-shell vacancy states produced in solid  Ca, V, Fe, and Cu targets by impact with about 10 MeV/amu C and Ne ions. The  resulting K hypersatellite x-ray emission spectra were measured by means of high- energy-resolution spectroscopy using a von Hamos bent crystal spectrometer. The  experiment was carried out at the Philips variable energy cyclotron of the Paul  Scherrer Institute. From the fits of the x-ray spectra the energies, line widths, and  relative intensities of the hypersatellite x-ray lines could be determined. The fitted  intensities were corrected to account for the energy-dependent solid angle of the  spectrometer, effective source size, target self-absorption, crystal reflectivity, and  detector efficiency. The single-to-double K-shell ionization cross-section ratios were  deduced from the corrected relative intensities of the hypersatellites and compared to  theoretical predictions from the semiclassical approximation model using hydrogenlike  and Dirac-Hartree-Fock wave functions and from classical trajectory Monte Carlo  calculations.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>https://folia.unifr.ch/global/documents/307181</dc:identifier>
  <dc:identifier>https://folia.unifr.ch/documents/307181/files/dou_hxr.pdf</dc:identifier>
  <dc:language>eng</dc:language>
  <dc:relation>info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevA.98.012705</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>License undefined</dc:rights>
  <dc:source>Physical Review A. - 2018, vol. 98, no. 1, p. 012705</dc:source>
  <dc:subject>info:eu-repo/classification/udc/53</dc:subject>
  <dc:title xmlns:ns1="xml" ns1:lang="en">Hypersatellite x-ray decay of $3d$ hollow-$K$-shell atoms produced by heavy-ion impact</dc:title>
  <dc:type>http://purl.org/coar/resource_type/c_6501</dc:type>
</oai_dc:dc>
