Single and double $K$-shell vacancy production in slow Xe$^\textrm{54+,53+}$-Xe collisions
| Autor: | Hillenbrand, P. -M., Hagmann, S., Kozhedub, Y. S., Benis, E. P., Brandau, C., Chen, R. J., Dmytriiev, D., Forstner, O., Glorius, J., Grisenti, R. E., Gumberidze, A., Lestinsky, M., Litvinov, Yu. A., Menz, E. B., Morgenroth, T., Nanos, S., Petridis, N., Pfäfflein, Ph., Rothard, H., Sanjari, M. S., Sidhu, R. S., Spillmann, U., Trotsenko, S., Tupitsyn, I. I., Varga, L., Stöhlker, Th. |
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| Rok vydání: | 2022 |
| Předmět: | |
| Zdroj: | Phys. Rev. A 105, 022810 (2022) |
| Druh dokumentu: | Working Paper |
| DOI: | 10.1103/PhysRevA.105.022810 |
| Popis: | We present an experimental and theoretical study of symmetric $\textrm{Xe}^{54+}+\textrm{Xe}$ collisions at 50, 30, and 15 MeV/u, corresponding to strong perturbations with $v_K/v_\text{p}$ = 1.20, 1.55, and 2.20, respectively ($v_K$: classical $K$-shell orbital velocity, $v_\text{p}$: projectile velocity), as well as $\textrm{Xe}^{53+}+\textrm{Xe}$ collisions at 15 MeV/u. For each of these systems, x-ray spectra were measured under a forward angle of $35^\circ$ with respect to the projectile beam. Target satellite and hypersatellite radiation, $K\alpha_{2,1}^\mathrm{s}$ and $K\alpha_{2,1}^\mathrm{hs}$, respectively, were analyzed and used to derive cross section ratios for double-to-single target $K$-shell vacancy production. We compare our experimental results to relativistic time-dependent two-center calculations. Comment: 8 pages, 4 figures |
| Databáze: | arXiv |
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