Preprint

Recombination rate coefficients for astrophysical applications from storage-ring experiments


AutorenlisteSchippers, S.; Boehm, S.; Mueller, A.; Gwinner, G.; Schnell, M.; Schwalm, D.; Wolf, A.; Savin, D.W.

Jahr der Veröffentlichung2003

ZeitschriftarXiv

DOI Linkhttps://doi.org/10.48550/arXiv.astro-ph/0301170

VerlagArxiv.org


Abstract

The basic approach for measuring electron-ion recombination rate coefficients in merged-beams electron-ion collision experiments at heavy-ion storage rings is outlined. As an example experimental results for the low temperature recombination of C IV ions are compared with the recommended theoretical rate coefficient by Mazzotta et al. The latter deviates by factors of up to 5 from the experimental one.




Zitierstile

Harvard-ZitierstilSchippers, S., Boehm, S., Mueller, A., Gwinner, G., Schnell, M., Schwalm, D., et al. (2003) Recombination rate coefficients for astrophysical applications from storage-ring experiments [Preprint]. arXiv, Article astro-ph/0301170. https://doi.org/10.48550/arXiv.astro-ph/0301170

APA-ZitierstilSchippers, S., Boehm, S., Mueller, A., Gwinner, G., Schnell, M., Schwalm, D., Wolf, A., & Savin, D. (2003). Recombination rate coefficients for astrophysical applications from storage-ring experiments. arXiv. https://doi.org/10.48550/arXiv.astro-ph/0301170


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