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Double KK excited states in highly charged sulphur

P Amaro, J P Marques, P Indelicato, T K Mukherjee, J K Saha, L C Tribedi, J P Santos

To cite this version:

P Amaro, J P Marques, P Indelicato, T K Mukherjee, J K Saha, et al.. Double KK excited states

in highly charged sulphur. Journal of Physics: Conference Series, IOP Publishing, 2015, 635 (2),

pp.022071 �10.1088/1742-6596/635/2/022071�. �hal-01265591�

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Double KK excited states in highly charged sulphur

View the table of contents for this issue, or go to the journal homepage for more 2015 J. Phys.: Conf. Ser. 635 022071

(http://iopscience.iop.org/1742-6596/635/2/022071)

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Double KK excited states in highly charged sulphur

P. Amaro

1

, J. P. Marques

, P. Indelicato

, T. K. Mukherjee

#

, J. K. Saha

q

, L. C. Tribedi

&

, J. P. Santos

2

Laboratório de Instrumentação, Engenharia Biomédica e Física da Radiação (LIBPhys-UNL), Departamento de Física, Faculdade de Ciências e Tecnologia, FCT, Universidade Nova de Lisboa, 2829-516 Caparica,

Portugal

BioISI - Biosystems & Integrative Sciences Institute, Faculdade de Ciências da Universidade de Lisboa, Campo Grande, C8, 1749-016 Lisboa, Portugal

Laboratoire Kastler Brossel, École Normale Supérieure, CNRS, Université P. et M. Curie – Paris 6, Case 74;

4, place Jussieu, 75252 Paris CEDEX 05, France

#Narula Institute of Technology, Agarpara, Kolkata-700109, India

q Indian Association for the Cultivation of Science, Jadavpur, Kolkata-700032, India

& Department of Nuclear and Atomic Physics, Tata Institute of Fundamental Research, Colaba, Mumbai

400005, India

Synopsis Calculation of energies and radiative decays was performed for several highly charge states of sulphur in order to identify experimental lines associated to double excitedKK atomic states.

Double

KK

excited states have several im- portant applications in astrophysics as well as in plasma diagnostics [1,

2].

Besides its ap- plicability, the fundamental interest of domi- nance of fluorescence over autoionization decay for some

KK

excited states has attract much attention, both from theoreticians and experi- mentalists [3,

4]. Recently, it was observed the 2p3d(1

P

0

)

→ 1s3d(1

D

e

) in helium with sufficient accuracy to distinguish from the H-like

Kα

line, showing an enhanced fluorescence rate compared to the one assuming standard selection rules [5].In this work, we continue the investigation of

KK

excited states for sulphur by performing a syste- matic identification of experimental lines, which includes both single

K

and double

KK

excited states. The relativistic calculations were made within the MCDF approach using the general re- lativistic MCDF code (MDFGME) [6]. Experi- mental measurements were performed at the Pel- letron accelerator facility in TIFR Mumbai.

In these preliminary calculations, all transi- tion energies and probabilities were computed in a monoconfiguration approach. Almost all possi- ble combinations of excitations for

Kα

,

Kβ

and

Kγ

transitions of He through Be charge states were considered. The positions of the experimen- tal lines are displayed in Fig. 1 along with the decay rates of the computed transitions. Transi- tions from

KK

excited states were also conside- red in both He- and Li-like states. It can obser- ved in Fig. 1 that all experimental lines lines are unambiguously identified, with the exception of one line next to the He-like

Kα

line. Lines near

the H-like

Kα

line can only be associated to the

KK

excited states of He or Li charge states. A precise identification can be done by calculating the respective autoionization rate.

Energy (eV)

2400 2500 2600 2700 2800 2900 3000 3100

)-1 (sW

102

103

104

105

106

107

108

109

1010

1011

1012

1013

1014

α K H

α K He

α K Li

α K Be

β K H

β K He

β K Li

β K Be

γ K He

γ K Li

γ K Be

KK He

KK Li Exp.

Figure 1. Comparison of obtained theoretical lines with experimental lines.

Referências

[1] A. B. C. Walker and Jr., H. R. Rugge, 1971 As- trophys. J. 164181

[2] T. Fujimoto and T. Kato, 1981Astrophys. J. 264 994

[3] T.W. Gorczycaat al2000Phys.Rev.Lett.851202 [4] J. G. Lambourne at al 2003 Phys.Rev.Lett. 90

153004

[5] S. Kasthurirangan at al 2013 Phys.Rev.Lett. 24 243201

[6] P. Indelicato and J. P. Desclaux 1990Phys.Rev.A 42 5139-5149

1E-mail: pdamaro@fct.unl.pt

2E-mail: jps@fct.unl.pt

XXIX International Conference on Photonic, Electronic, and Atomic Collisions (ICPEAC2015) IOP Publishing Journal of Physics: Conference Series 635 (2015) 022071 doi:10.1088/1742-6596/635/2/022071

Content from this work may be used under the terms of theCreative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.

Published under licence by IOP Publishing Ltd 1

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