Journal article

Electron-ion recombination of mg6+ forming Mg5+ and of Mg7+ forming Mg6+: Laboratory measurements and theoretical calculations


Authors listLestinsky, M.; Badnell, N. R.; Bernhardt, D.; Bing, D.; Grieser, M.; Hahn, M.; Hoffmann, J.; Jordon-Thaden, B.; Krantz, C.; Novotny, O.; Orlov, D. A.; Repnow, R.; Shornikov, A.; Müller, A.; Schippers, S.; Wolf, A.; Savin, D. W.

Publication year2012

JournalThe Astrophysical Journal

Volume number758

Issue number1

ISSN0004-637X

eISSN1538-4357

Open access statusGreen

DOI Linkhttps://doi.org/10.1088/0004-637X/758/1/40

PublisherAmerican Astronomical Society


Abstract
We have measured electron-ion recombination for C-like Mg6+ forming Mg5+, and for B-like Mg7+ forming Mg6+. These studies were performed using a merged electron-ion beam arrangement at the TSR heavy ion storage ring located in Heidelberg, Germany. Both primary ions have metastable levels with significant lifetimes. Using a simple cascade model we estimate the population fractions in these metastable levels. For the Mg6+ results, we find that the majority of the stored ions are in a metastable level, while for Mg7+ the metastable fraction is insignificant. We present the Mg6+ merged beams recombination rate coefficient for DR via N = 2 -> N' = 2 core electron excitations (Delta N = 0 DR) and for Mg7+ via 2 -> 2 and 2 -> 3 core excitations. Taking the estimated metastable populations into account, we compare our results to state-of-the-art multiconfiguration Breit-Pauli theoretical calculations. Significant differences are found at low energies where theory is known to be unreliable. Moreover, for both ions we observe a discrepancy between experiment and theory for Delta N = 0 DR involving capture into high-n Rydberg levels and where the stabilization is primarily due to a radiative transition of the excited core electron. This is consistent with previous DR experiments on M-shell iron ions which were performed at TSR. The large metastable content of the Mg6+ ion beam precludes generating a plasma recombination rate coefficient (PRRC). However, this is not an issue for Mg7+ and we present an experimentally derived Mg7+ PRRC for plasma temperatures from 400 K to 107 K with an estimated uncertainty of less than 27% at a 90% confidence level. We also provide a fit to our experimentally derived PRRC for use in plasma modeling codes.



Citation Styles

Harvard Citation styleLestinsky, M., Badnell, N., Bernhardt, D., Bing, D., Grieser, M., Hahn, M., et al. (2012) Electron-ion recombination of mg6+ forming Mg5+ and of Mg7+ forming Mg6+: Laboratory measurements and theoretical calculations, The Astrophysical Journal, 758(1), Article 40. https://doi.org/10.1088/0004-637X/758/1/40

APA Citation styleLestinsky, M., Badnell, N., Bernhardt, D., Bing, D., Grieser, M., Hahn, M., Hoffmann, J., Jordon-Thaden, B., Krantz, C., Novotny, O., Orlov, D., Repnow, R., Shornikov, A., Müller, A., Schippers, S., Wolf, A., & Savin, D. (2012). Electron-ion recombination of mg6+ forming Mg5+ and of Mg7+ forming Mg6+: Laboratory measurements and theoretical calculations. The Astrophysical Journal. 758(1), Article 40. https://doi.org/10.1088/0004-637X/758/1/40



Keywords


ATOMIC DATAatomic processesCORE EXCITATIONSDIELECTRONIC RECOMBINATIONFINITE-DENSITY PLASMASHIGH-RESOLUTION MEASUREMENTIONIZATION EQUILIBRIUMISOELECTRONIC SEQUENCELOW ENERGIESNA-LIKE ARRADIATIVE RECOMBINATIONRATE COEFFICIENTS

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