<?xml version="1.0" encoding="UTF-8"?>
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  <title>DSpace Collection:</title>
  <link rel="alternate" href="http://hdl.handle.net/10362/2468" />
  <subtitle />
  <id>http://hdl.handle.net/10362/2468</id>
  <updated>2013-06-19T13:34:11Z</updated>
  <dc:date>2013-06-19T13:34:11Z</dc:date>
  <entry>
    <title>Production and decay of Sulphur excited species in a ECRIS plasma</title>
    <link rel="alternate" href="http://hdl.handle.net/10362/2506" />
    <author>
      <name>Martins, Maria Conceição</name>
    </author>
    <author>
      <name>Marques, José Pires</name>
    </author>
    <author>
      <name>Costa, Ana Maria</name>
    </author>
    <author>
      <name>Santos, José Paulo</name>
    </author>
    <author>
      <name>Parente, Fernando</name>
    </author>
    <author>
      <name>Schlesser, Sophie</name>
    </author>
    <author>
      <name>Le Bigot, Eric-Olivier</name>
    </author>
    <author>
      <name>Indelicato, Paul</name>
    </author>
    <id>http://hdl.handle.net/10362/2506</id>
    <updated>2010-01-25T11:30:39Z</updated>
    <published>2009-01-01T00:00:00Z</published>
    <summary type="text">Title: Production and decay of Sulphur excited species in a ECRIS plasma
Authors: Martins, Maria Conceição; Marques, José Pires; Costa, Ana Maria; Santos, José Paulo; Parente, Fernando; Schlesser, Sophie; Le Bigot, Eric-Olivier; Indelicato, Paul
Abstract: The most important processes for the creation of S12+ to S14+ ions excited states from the ground configurations of S9+ to S14+ ions in an electron cyclotron resonance ion source, leading to the emission of K X-ray lines, are studied. Theoretical values for inner-shell excitation and ionization cross sections, including double KL and triple KLL ionization, transition probabilities and energies for the deexcitation processes, are calculated in the framework of the multi-configuration Dirac-Fock method. With reasonable assumptions about the electron energy distribution, a theoretical K$\alpha$ X-ray spectrum is obtained, which is compared to recent experimental data.</summary>
    <dc:date>2009-01-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>QED and relativistic corrections in superheavy elements</title>
    <link rel="alternate" href="http://hdl.handle.net/10362/2478" />
    <author>
      <name>Indelicato, Paul</name>
    </author>
    <author>
      <name>Santos, José Paulo</name>
    </author>
    <author>
      <name>Boucard, Stephan</name>
    </author>
    <author>
      <name>Desclaux, Jean-Paul</name>
    </author>
    <id>http://hdl.handle.net/10362/2478</id>
    <updated>2010-01-22T09:29:23Z</updated>
    <published>2007-01-01T00:00:00Z</published>
    <summary type="text">Title: QED and relativistic corrections in superheavy elements
Authors: Indelicato, Paul; Santos, José Paulo; Boucard, Stephan; Desclaux, Jean-Paul
Abstract: In this paper we review the different relativistic and QED contributions to energies, ionic radii, transition probabilities and Landé g-factors in super-heavy elements, with the help of the MultiConfiguration Dirac-Fock method (MCDF). The effects of taking into account the Breit interaction to all orders by including it in the self-consistent field process are demonstrated. State of the art radiative corrections are included in the calculation and discussed. We also study the non-relativistic limit of MCDF calculation and find that the non-relativistic offset can be unexpectedly large.</summary>
    <dc:date>2007-01-01T00:00:00Z</dc:date>
  </entry>
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