Single and double K -shell vacancy production in slow Xe54+,53+ -Xe collisions

P.-M. Hillenbrand; S. Hagmann; Y.S. Kozhedub; E.P. Benis; C. Brandau; R. J. Chen; D. Dmytriiev; O. Forstner; J. Glorius; R.E. Grisenti; A. Gumberidze; M. Lestinsky; Yu. A. Litvinov; E.B. Menz; T. Morgenroth; S. Nanos; N. Petridis; Ph. Pfafflein; H. Rothard; M.S. Sanjari; R.S. Sidhu; U. Spillmann; S. Trotsenko; I.I. Tupitsyn; L. Varga; Th. Stöhlker

doi:10.1103/physreva.105.022810

Single and double K -shell vacancy production in slow Xe54+,53+ -Xe collisions

P.-M. Hillenbrand, S. Hagmann, Y.S. Kozhedub, E.P. Benis, C. Brandau, R. J. Chen, D. Dmytriiev, O. Forstner, J. Glorius, R.E. Grisenti, A. Gumberidze, M. Lestinsky, Yu. A. Litvinov, E.B. Menz, T. Morgenroth, S. Nanos, N. Petridis, Ph. Pfafflein, H. Rothard, M.S. SanjariR.S. Sidhu, U. Spillmann, S. Trotsenko, I.I. Tupitsyn, L. Varga, Th. Stöhlker

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

We present an experimental and theoretical study of symmetric Xe54+ + Xe collisions at 50, 30, and 15 MeV/u, corresponding to strong perturbations with vK /vp = 1.20, 1.55, and 2.20, respectively (vK is the classical K-shell orbital velocity and vp is the projectile velocity), as well as Xe53+ + Xe collisions at 15 MeV/u. For each of these systems, x-ray spectra are measured under a forward angle of 35◦ with respect to the projectile beam. Target satellite and hypersatellite radiation Kαs 2,1 and Kαhs 2,1, respectively, are 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.

Original language	English
Article number	022810
Pages (from-to)	1-8
Number of pages	8
Journal	Physical Review A
Volume	105
Issue number	2
DOIs	https://doi.org/10.1103/physreva.105.022810
Publication status	Published - 11 Feb 2022

Access to Document

10.1103/physreva.105.022810

https://arxiv.org/abs/2201.10181Licence: Creative Commons: Attribution (CC-BY)

Cite this

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, Y. A., Menz, E. B., Morgenroth, T., Nanos, S., Petridis, N., Pfafflein, P., Rothard, H., ... Stöhlker, T. (2022). Single and double K -shell vacancy production in slow Xe54+,53+ -Xe collisions. Physical Review A, 105(2), 1-8. Article 022810. https://doi.org/10.1103/physreva.105.022810

@article{111078eec69143b48adbf61fec58cff4,

title = "Single and double K -shell vacancy production in slow Xe54+,53+ -Xe collisions",

abstract = "We present an experimental and theoretical study of symmetric Xe54+ + Xe collisions at 50, 30, and 15 MeV/u, corresponding to strong perturbations with vK /vp = 1.20, 1.55, and 2.20, respectively (vK is the classical K-shell orbital velocity and vp is the projectile velocity), as well as Xe53+ + Xe collisions at 15 MeV/u. For each of these systems, x-ray spectra are measured under a forward angle of 35◦ with respect to the projectile beam. Target satellite and hypersatellite radiation Kαs 2,1 and Kαhs 2,1, respectively, are 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.",

author = "P.-M. Hillenbrand and S. Hagmann and Y.S. Kozhedub and E.P. Benis and C. Brandau and Chen, {R. J.} and D. Dmytriiev and O. Forstner and J. Glorius and R.E. Grisenti and A. Gumberidze and M. Lestinsky and Litvinov, {Yu. A.} and E.B. Menz and T. Morgenroth and S. Nanos and N. Petridis and Ph. Pfafflein and H. Rothard and M.S. Sanjari and R.S. Sidhu and U. Spillmann and S. Trotsenko and I.I. Tupitsyn and L. Varga and Th. St{\"o}hlker",

note = "Funding Information: We thank M. Steck, S. Litvinov, B. Lorentz, and R. He{\ss} for operating the ESR. This research was conducted in the framework of the SPARC collaboration, experiment E132 of FAIR Phase-0 supported by GSI. It was further supported by the European Research Council under the European Union's Horizon 2020 research and innovation program through Grant No. 682841 (ASTRUm) and Grant Agreement No. 654002 (ENSAR2). We acknowledge substantial support from ErUM-FSP APPA (BMBF Grants No. 05P15RGFAA and No. 05P19SJFAA) and from the State of Hesse within the Research Cluster ELEMENTS (Project No. 500/10.006). E.P.B., S.N., and H.R. gratefully acknowledge support from the Transnational Access to GSI activity. Publisher Copyright: {\textcopyright} 2022 American Physical Society.",

year = "2022",

month = feb,

day = "11",

doi = "10.1103/physreva.105.022810",

language = "English",

volume = "105",

pages = "1--8",

journal = "Physical Review A",

issn = "2469-9926",

publisher = "American Physical Society",

number = "2",

}

Hillenbrand, P-M, Hagmann, S, Kozhedub, YS, Benis, EP, Brandau, C, Chen, RJ, Dmytriiev, D, Forstner, O, Glorius, J, Grisenti, RE, Gumberidze, A, Lestinsky, M, Litvinov, YA, Menz, EB, Morgenroth, T, Nanos, S, Petridis, N, Pfafflein, P, Rothard, H, Sanjari, MS, Sidhu, RS, Spillmann, U, Trotsenko, S, Tupitsyn, II, Varga, L & Stöhlker, T 2022, 'Single and double K -shell vacancy production in slow Xe54+,53+ -Xe collisions', Physical Review A, vol. 105, no. 2, 022810, pp. 1-8. https://doi.org/10.1103/physreva.105.022810

TY - JOUR

T1 - Single and double K -shell vacancy production in slow Xe54+,53+ -Xe collisions

AU - Hillenbrand, P.-M.

AU - Hagmann, S.

AU - Kozhedub, Y.S.

AU - Benis, E.P.

AU - Brandau, C.

AU - Chen, R. J.

AU - Dmytriiev, D.

AU - Forstner, O.

AU - Glorius, J.

AU - Grisenti, R.E.

AU - Gumberidze, A.

AU - Lestinsky, M.

AU - Litvinov, Yu. A.

AU - Menz, E.B.

AU - Morgenroth, T.

AU - Nanos, S.

AU - Petridis, N.

AU - Pfafflein, Ph.

AU - Rothard, H.

AU - Sanjari, M.S.

AU - Sidhu, R.S.

AU - Spillmann, U.

AU - Trotsenko, S.

AU - Tupitsyn, I.I.

AU - Varga, L.

AU - Stöhlker, Th.

N1 - Funding Information: We thank M. Steck, S. Litvinov, B. Lorentz, and R. Heß for operating the ESR. This research was conducted in the framework of the SPARC collaboration, experiment E132 of FAIR Phase-0 supported by GSI. It was further supported by the European Research Council under the European Union's Horizon 2020 research and innovation program through Grant No. 682841 (ASTRUm) and Grant Agreement No. 654002 (ENSAR2). We acknowledge substantial support from ErUM-FSP APPA (BMBF Grants No. 05P15RGFAA and No. 05P19SJFAA) and from the State of Hesse within the Research Cluster ELEMENTS (Project No. 500/10.006). E.P.B., S.N., and H.R. gratefully acknowledge support from the Transnational Access to GSI activity. Publisher Copyright: © 2022 American Physical Society.

PY - 2022/2/11

Y1 - 2022/2/11

N2 - We present an experimental and theoretical study of symmetric Xe54+ + Xe collisions at 50, 30, and 15 MeV/u, corresponding to strong perturbations with vK /vp = 1.20, 1.55, and 2.20, respectively (vK is the classical K-shell orbital velocity and vp is the projectile velocity), as well as Xe53+ + Xe collisions at 15 MeV/u. For each of these systems, x-ray spectra are measured under a forward angle of 35◦ with respect to the projectile beam. Target satellite and hypersatellite radiation Kαs 2,1 and Kαhs 2,1, respectively, are 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.

AB - We present an experimental and theoretical study of symmetric Xe54+ + Xe collisions at 50, 30, and 15 MeV/u, corresponding to strong perturbations with vK /vp = 1.20, 1.55, and 2.20, respectively (vK is the classical K-shell orbital velocity and vp is the projectile velocity), as well as Xe53+ + Xe collisions at 15 MeV/u. For each of these systems, x-ray spectra are measured under a forward angle of 35◦ with respect to the projectile beam. Target satellite and hypersatellite radiation Kαs 2,1 and Kαhs 2,1, respectively, are 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.

UR - http://dx.doi.org/10.1103/physreva.105.022810

U2 - 10.1103/physreva.105.022810

DO - 10.1103/physreva.105.022810

M3 - Article

SN - 2469-9926

VL - 105

SP - 1

EP - 8

JO - Physical Review A

JF - Physical Review A

IS - 2

M1 - 022810

ER -

Single and double K -shell vacancy production in slow Xe54+,53+ -Xe collisions

Abstract

Access to Document

Other files and links

Fingerprint

Cite this