7–12 Sept 2025
PSI
Europe/Zurich timezone

Mirror beta transitions as an additional probe for $V_{ud}$

11 Sept 2025, 12:00
30m
WHGA/001 - Auditorium (PSI)

WHGA/001 - Auditorium

PSI

Oral presentation Session

Speaker

Nathal Severijns (Katholieke Univ. Leuven)

Description

Since the potential of mirror beta transitions to provide an independent determination of the $V_{ud}$ quark-mixing matrix element was pointed out, about 15 years ago [1], many measurements of spectroscopic quantities have been performed and more detailed theoretical corrections have been addressed. These significantly improved the precision on the Ft-values of these transitions [2, 3]. In addition, several precise measurements of the asymmetry parameter have been reported and future measurements of other correlation parameters are being prepared. Although mirror transitions have (like neutron decay) the extra complication of requiring a correlation measurement to extract the axial vector-to-vector mixing ratio, the current precision on $V_{ud}$ from nuclear mirror transitions is still comparable to that from free neutron decay and is a factor of about 3 larger than the precision of the value extracted from pure Fermi transitions.
In recent years, important progress was made in the calculation of the nucleus-independent radiative correction ($∆_R$), in the nuclear structure-dependent radiative corrections ($δ_{NS}$) as well as in isospin-symmetry breaking effects ($δ_C$).
This progress will maintain nuclear mirror decays as a solid additional source for the determination of $V_{ud}$, along with superallowed pure Fermi transitions and free neutron decay. In this presentation we will discuss the current status and future prospects of these activities.

[1] O. Naviliat-Cuncic and N. Severijns, Phys. Rev. Lett. 102, 142302 (2009).
[2] N. Severijns, M. Tandecki, T. Phalet, I.S. Towner, Phys. Rev. C 78, 055501 (2008).
[3] N. Severijns, L. Hayen, V. De Leebeeck, S. Vanlangendonck, K. Bodek, D. Rozpedzik, I.S. Towner, Phys. Rev. C 107, 015502 (2023).

Authors

Nathal Severijns (Katholieke Univ. Leuven) Prof. Oscar Naviliat-Cuncic (1 Facility for Rare Isotope Beams and Department of Physics and Astronomy, Michigan State University; 2 International Laboratory for Nuclear Physics and Nuclear Astrophysics, CNRS-MSU)

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