activity
20202026
most citedEvolution of the isoscalar giant monopole resonance in the Ca isotope chain

18 citations · 18 across the 7 of their papers we have counts for

collaborators

7 papers

nucl-ex2026

Direct measurement of Enhanced octupole collectivity in 148Dy

P. Spagnoletti, V. Vedia, E. Yuksel +36

Excited states in Dy were populated via decay of Ho using the GRIFFIN spectrometer at the TRIUMF ISAC-I facility. A combined measurement of the mean…

nucl-ex2026

Independent Validation of Octupole Collectivity in radium-224 through lifetime measurements of low-lying negative-parity states

D. White, D. O'Donnell, A. Avaa +30

The nucleus Ra is a key benchmark for octupole deformation and for theoretical descriptions of enhanced Schiff moments in reflection-asymmetric nuclei. While Coulomb-excita…

nucl-ex2026

Statistical properties of Xe and the Xe cross section

H. C. Berg, V. W. Ingeberg, S. Siem +17

Xe is an interesting case for plasma physics to explore nuclear excitation by electron capture, as the process can be studied using statistical properties of Xe. In…

nucl-ex2024

Coulomb Excitation of Sr and the limits of the island of deformation

R. Russell, J. Heery, J. Henderson +33

The region of has long been associated with strongly deformed nuclear configurations. The presence of this strong deformation was recently confirmed through…

nucl-ex2022

Nuclear Level Density and -ray Strength Function of

Vetle W. Ingeberg, Pete Jones, Lumkile Msebi +9

The nuclear level density (NLD) and -ray strength function (SF) of have been investigated using the Oslo method. The extracted NLD is compared with previou…

nucl-ex2022★ 18 cited

Evolution of the isoscalar giant monopole resonance in the Ca isotope chain

S. D. Olorunfunmi, R. Neveling, J. Carter +25

Two recent studies of the evolution of the isoscalar giant monopole resonance (ISGMR) within the calcium isotope chain report conflicting results. One study suggests that the monop…

nucl-ex2020

Improved precision on the experimental E0 decay branching ratio of the Hoyle state

T. K. Eriksen, T. Kibédi, M. W. Reed +35

Stellar carbon synthesis occurs exclusively via the process, in which three particles fuse to form C in the excited Hoyle state, followed by electromagnetic decay t…