<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>García-Fernández, Pablo</dc:creator>
  <dc:creator>Senn, Florian</dc:creator>
  <dc:creator>Daul, Claude</dc:creator>
  <dc:creator>Aramburu, Jose Antonio</dc:creator>
  <dc:creator>Barriuso, Maria Teresa</dc:creator>
  <dc:creator>Moreno, Miguel</dc:creator>
  <dc:date>2009-06-17</dc:date>
  <dc:description xmlns:ns0="xml" ns0:lang="en">We show that values of the magnetic anisotropy energy (MAE), which are about two orders of magnitude larger than the usual ones for transition metal cations in insulators (∼0.01–1 cm⁻¹), can be found for the less common ion Fe⁺. In SrCl₂ : Fe⁺, the MAE is 93 cm⁻¹ when calculated using second-order perturbation multi-configurational calculations (CASPT2) while a similar value is found using multi-reference density functional theory (MR-DFT). This result is even larger than other recently reported giant MAEs for atoms on surfaces or magnetic clusters. The microscopic origin of this giant MAE is discussed in detail.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>https://folia.unifr.ch/global/documents/301406</dc:identifier>
  <dc:identifier>https://folia.unifr.ch/documents/301406/files/daul_gma.pdf</dc:identifier>
  <dc:language>eng</dc:language>
  <dc:relation>info:eu-repo/semantics/altIdentifier/doi/10.1039/b908110k</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>License undefined</dc:rights>
  <dc:source>Physical Chemistry Chemical Physics. - 2009, vol. 11, p. 7545-7548</dc:source>
  <dc:subject>info:eu-repo/classification/udc/54</dc:subject>
  <dc:title xmlns:ns1="xml" ns1:lang="en">The giant magnetic anisotropy energy of Fe⁺ ions in SrCl₂</dc:title>
  <dc:type>http://purl.org/coar/resource_type/c_6501</dc:type>
</oai_dc:dc>
