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  Dielectronic Recombination of Fe XXIII Forming Fe XXII: Laboratory Measurements and Theoretical Calculations

Savin, D., Gwinner, G., Grieser, M., Repnow, R., Schnell, M., Schwalm, D., et al. (2006). Dielectronic Recombination of Fe XXIII Forming Fe XXII: Laboratory Measurements and Theoretical Calculations. The Astrophysical Journal, 642(2), 1275-1285.

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Savin, D.1, Autor
Gwinner, G.2, Autor           
Grieser, M.3, Autor           
Repnow, R.3, Autor           
Schnell, M.2, Autor           
Schwalm, D.2, Autor           
Wolf, A.3, Autor           
Zhou, S.G.1, Autor
Kieslich, S.1, Autor
Mueller, A.1, Autor
Schippers, S.3, Autor           
Colgan, J.1, Autor
Loch, S.1, Autor
Badnell, N.1, Autor
Chen, M.1, Autor
Gu, M.1, Autor
Affiliations:
1Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, Mail Code 5247, New York, NY 10027; Institut für Atom- und Molekülphysik, Justus-Liebig-Universität, D-35392 Giessen, Germany Los Alamos National Laboratory, P.O. Box 1663, Los Alamos, NM 87545 Physics Department, Auburn University, 206 Allison Laboratory, Auburn, AL 36849 Department of Physics, University of Strathclyde, Glasgow G4 0NG, UK Lawrence Livermore National Laboratory, P.O. Box 808, Livermore, CA 94551 Department of Physics and Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305, ou_persistent22              
2Prof. Dirk Schwalm, Emeriti, MPI for Nuclear Physics, Max Planck Society, ou_907546              
3Division Prof. Dr. Klaus Blaum, MPI for Nuclear Physics, Max Planck Society, ou_904548              

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 Zusammenfassung: We have measured resonance strengths and energies for dielectronic recombination (DR) of beryllium-like Fe XXIII forming boron-like Fe XXII via N = 2 → N′ = 2 and N = 2 → N′ = 3 core excitations. All measurements were carried out using the heavy-ion Test Storage Ring at the Max Planck Institute for Nuclear Physics (MPI-K) in Heidelberg, Germany. We have also calculated these resonance strengths and energies using three independent, perturbative, state-of-the-art theoretical techniques: the multiconfiguration Breit-Pauli (MCBP) method, the multiconfiguration Dirac-Fock (MCDF) method, and the Flexible Atomic Code (FAC). Overall reasonable agreement is found between our experimental results and these theoretical calculations. We have used our measurements to produce a Maxwellian-averaged DR rate coefficient for Fe XXIII. Our experimentally derived rate coefficient is estimated to be accurate to better that ≈20%. At temperatures where Fe XXIII is predicted to form in both photoionized and electron-ionized gas, we find mixed agreement between our experimental rate coefficient and previously published rate coefficients. We find good agreement at these temperatures between the experimentally derived rate coefficient and our MCBP, MCDF, and FAC results.

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Sprache(n): eng - English
 Datum: 2006-05
 Publikationsstatus: Erschienen
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 Art der Begutachtung: Expertenbegutachtung
 Identifikatoren: eDoc: 280987
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Titel: The Astrophysical Journal
Genre der Quelle: Zeitschrift
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Seiten: - Band / Heft: 642 (2) Artikelnummer: - Start- / Endseite: 1275 - 1285 Identifikator: -