J. Williams

most citedCross Sections of the

^{83}

Rb(p,

γ)^{84}

Sr and

^{84}

Kr(p,

γ)^{85}

Rb Reactions at Energies Characteristic of the Astrophysical

γ

Process

9 citations · 21 across the 3 of their papers we have counts for

collaborators

3 papers

nucl-ex2023★ 6 cited

Identifying the spin trapped character of the $^{32}$ Si isomeric state

J. Williams, G. Hackman, K. Starosta +30

The properties of a nanosecond isomer in $^{32}$ Si, disputed in previous studies, depend on the evolution of proton and neutron shell gaps near the `island of inversion'. We have p…

nucl-ex2023★ 9 cited

Cross Sections of the $^{83}$ Rb(p, $γ)^{84}$ Sr and $^{84}$ Kr(p, $γ)^{85}$ Rb Reactions at Energies Characteristic of the Astrophysical $γ$ Process

M. Williams, B. Davids, G. Lotay +22

We have measured the cross section of the $^{83}$ Rb(p, $γ)^{84}$ Sr radiative capture reaction in inverse kinematics using a radioactive beam of $^{83}$ Rb at incident energies of 2.4…

nucl-ex2022★ 6 cited

Improved measurement of the $0_{2}^{+} \to 0_{1}^{+}$ E0 transition strength for $^{72}$ Se using the SPICE spectrometer

J. Smallcombe, A. B. Garnsworthy, W. Korten +22

The selenium isotopes lie at the heart of a tumultuous region of the nuclear chart where shape coexistence effects grapple with neutron-proton pairing correlations, triaxiality, an…

Identifying the spin trapped character of the 32Si isomeric state

Cross Sections of the 83Rb(p,γ)84Sr and 84Kr(p,γ)85Rb Reactions at Energies Characteristic of the Astrophysical γ Process

Improved measurement of the 02+​→01+​ E0 transition strength for 72Se using the SPICE spectrometer

Identifying the spin trapped character of the $^{32}$ Si isomeric state

Cross Sections of the $^{83}$ Rb(p, $γ)^{84}$ Sr and $^{84}$ Kr(p, $γ)^{85}$ Rb Reactions at Energies Characteristic of the Astrophysical $γ$ Process

Improved measurement of the $0_{2}^{+} \to 0_{1}^{+}$ E0 transition strength for $^{72}$ Se using the SPICE spectrometer