Publication:
Dielectronic recombination of Fe xv forming Fe xiv: Laboratory measurements and theoretical calculations

dc.contributor.authorALTUN, ZİKRİ
dc.contributor.authorsLukic, D. V.; Schnell, M.; Savin, D. W.; Brandau, C.; Schmidt, E. W.; Boehm, S.; Mueller, A.; Schippers, S.; Lestinsky, M.; Sprenger, F.; Wolf, A.; Altun, Z.; Badnell, N. R.
dc.date.accessioned2022-03-14T10:06:24Z
dc.date.accessioned2026-01-11T10:36:14Z
dc.date.available2022-03-14T10:06:24Z
dc.date.issued2007-08
dc.description.abstractWe have measured resonance strengths and energies for dielectronic recombination (DR) of Mg-like Fe xv forming Al-like Fe XIV via N = 3 -> N' = 3 core excitations in the electron-ion collision energy range 0 - 45 eV. All measurements were carried out using the heavy-ion test storage ring at the Max Planck Institute for Nuclear Physics in Heidelberg, Germany. We have also carried out new multiconfiguration Breit-Pauli (MCBP) calculations using the AUTOSTRUCTURE code. For electron-ion collision energies less than or similar to 25 eV we find poor agreement between our experimental and theoretical resonance energies and strengths. From 25 to 42 eV we find good agreement between the two for resonance energies. But in this energy range the theoretical resonance strengths are approximate to 31% larger than the experimental results. This is larger than our estimated total experimental uncertainty in this energy range of +/- 26% ( at a 90% confidence level). Above 42 eV the difference in the shape between the calculated and measured 3s3p(P-1(1))nl DR series limit we attribute partly to the nl dependence of the detection probabilities of high Rydberg states in the experiment. We have used our measurements, supplemented by our AUTOSTRUCTURE calculations, to produce a Maxwellian-averaged 3 -> 3 DR rate coefficient for Fe XV forming Fe XIV. The resulting rate coefficient is estimated to be accurate to better than +/- 29% (at a 90% confidence level) for k(B)T(e) >= 1 eV. At temperatures of kBTe >= 2.5 - 15 eV, where Fe XV is predicted to form in photoionized plasmas, significant discrepancies are found between our experimentally derived rate coefficient and previously published theoretical results. Our new MCBP plasma rate coefficient is 19% Y28% smaller than our experimental results over this temperature range.
dc.identifier.doi10.1086/519073
dc.identifier.eissn1538-4357
dc.identifier.issn0004-637X
dc.identifier.urihttps://hdl.handle.net/11424/244051
dc.identifier.wosWOS:000248675000058
dc.language.isoeng
dc.publisherIOP PUBLISHING LTD
dc.relation.ispartofASTROPHYSICAL JOURNAL
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectatomic data
dc.subjectatomic processes
dc.subjectgalaxies : active
dc.subjectgalaxies : nuclei
dc.subjectplasmas
dc.subjectX-rays : galaxies
dc.subjectHIGH-RESOLUTION MEASUREMENT
dc.subjectELECTRON-ION RECOMBINATION
dc.subjectNUCLEAR ENVIRONMENT
dc.subjectIONIZED-GAS
dc.subjectXMM-NEWTON
dc.subjectPHOTOIONIZED GAS
dc.subjectRAY-ABSORPTION
dc.subjectXVIII
dc.subjectIONIZATION
dc.subjectNGC-3783
dc.titleDielectronic recombination of Fe xv forming Fe xiv: Laboratory measurements and theoretical calculations
dc.typearticle
dspace.entity.typePublication
oaire.citation.endPage1252
oaire.citation.issue2
oaire.citation.startPage1244
oaire.citation.titleASTROPHYSICAL JOURNAL
oaire.citation.volume664

Files

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
file.pdf
Size:
1.41 MB
Format:
Adobe Portable Document Format