8–10 Apr 2024
SMI, Postsparkasse, Georg Coch Platz 2, 1010 Wien
Europe/Vienna timezone

Resonance states in antiprotonic helium

10 Apr 2024, 11:15
35m
3rd floor (SMI, Postsparkasse, Georg Coch Platz 2, 1010 Wien)

3rd floor

SMI, Postsparkasse, Georg Coch Platz 2, 1010 Wien

Presence talk Exotic Hadronic and Leptonic Atoms

Speaker

Jean Servais (Université libre de Bruxelles)

Description

In the last decades, exotic few-body atoms, in which an electron is replaced by an exotic particle, have attracted great scientific interest. These systems are indeed very useful to determine accurately the properties of their constituting exotic particles. For instance, an antiproton can be captured by a helium atom in a high orbital momentum state (typically L = 30 to 35) to form the so-called antiprotonic helium, a three-body system made of an alpha-particle, an electron, and an antiproton. This atom is in a high-L quasibound resonant state with very narrow width, hence long Auger lifetime. The radiative transitions between these quasibound states enable one to study these systems experimentally, and the recent study of antiprotonic helium led to the up-to-now most precise value of the antiproton mass [1,2]. Similar studies have been conducted with other exotic atoms, such as the pionic helium [3,4].

In order to give a comprehensive theoretical understanding of antiprotonic helium, I will present a method for computing non-relativistic resonance energies and widths for a wide range of the total orbital momentum L. I developed an approach combining the Lagrange-mesh method in perimetric coordinates [5,6] and the complex Kohn variational principle [7,8] in order to obtain the S-matrix related to the emission of the electron from the three-body system. By extrapolating this S-matrix in the complex plane from the real axis [9], the widths of the states are determined. These widths are directly related to the Auger lifetimes of the system. I will show that this approach is suited for studying very accurately the resonances of these systems for a wide range of the orbital momentum L. In addition, I will present how to take some relativistic corrections into account, as well as how to compute the radiative lifetimes between quasibound states.

References :
[1] M. Hori, A. Sótér, D. Barna et al. Nature 475, 484–488 (2011).
[2] V. I. Korobov, Physical Review A 77, 042506 (2008).
[3] M. Hori, H. Aghai-Khozani, A. Sótér et al. Nature 581, 37–41 (2020).
[4] Z. D. Bai, V. I. Korobov, Z. C. Yan, et al. Physical Review Letters, 128, 183001 (2022).
[5] D. Baye, J. Dohet-Eraly, and P. Schoofs, Physical Review A 99, 22508 (2019).
[6] D. Baye and J. Dohet-Eraly, Physical Review A 103, 022823 (2021).
[7] V. I. Korobov and I. Shimamura, Physical Review A 56, 4587 (1997).
[8] A. Kievsky, Nuclear Physics A, 624, 125-139 (1997).
[9] S. A. Rakityansky, S. A. Sofianos, and N. Elander, Journal of Physics A, 40, 14857 (2007).

Primary author

Jean Servais (Université libre de Bruxelles)

Co-author

Prof. Jérémy DOHET-ERALY (Université libre de Bruxelles (ULB))

Presentation materials