Journal article

Dielectronic recombination of xenonlike tungsten ions


Authors listSchippers, S.; Bernhardt, D.; Müller, A.; Krantz, C.; Grieser, M.; Repnow, R.; Wolf, A.; Lestinsky, M.; Hahn, M.; Novotny, O.; Savin, D. W.

Publication year2011

JournalPhysical review A

Volume number83

Issue number1

ISSN1050-2947

eISSN1094-1622

Open access statusGreen

DOI Linkhttps://doi.org/10.1103/PhysRevA.83.012711

PublisherAmerican Physical Society


Abstract
Dielectronic recombination (DR) of xenonlike W20+ forming W19+ has been studied experimentally at a heavy-ion storage ring. A merged-beams method has been employed for obtaining absolute rate coefficients for electron-ion recombination in the collision-energy range 0-140 eV. The measured rate coefficient is dominated by strong DR resonances even at the lowest experimental energies. At plasma temperatures where the fractional abundance of W20+ is expected to peak in a fusion plasma, the experimentally derived plasma recombination rate coefficient is over a factor of 4 larger than the theoretically calculated rate coefficient which is currently used in fusion plasma modeling. The largest part of this discrepancy stems most probably from the neglect in the theoretical calculations of DR associated with fine-structure excitations of the W20+([Kr]4d(10)4 integral (8)) ion core.



Citation Styles

Harvard Citation styleSchippers, S., Bernhardt, D., Müller, A., Krantz, C., Grieser, M., Repnow, R., et al. (2011) Dielectronic recombination of xenonlike tungsten ions, Physical review A, 83(1), Article 012711. https://doi.org/10.1103/PhysRevA.83.012711

APA Citation styleSchippers, S., Bernhardt, D., Müller, A., Krantz, C., Grieser, M., Repnow, R., Wolf, A., Lestinsky, M., Hahn, M., Novotny, O., & Savin, D. (2011). Dielectronic recombination of xenonlike tungsten ions. Physical review A. 83(1), Article 012711. https://doi.org/10.1103/PhysRevA.83.012711



Keywords


COEFFICIENTSELECTRONEXCITED-STATESHIGH-RESOLUTION MEASUREMENTPHOTOIONIZED GAS

Last updated on 2025-23-06 at 10:29