Energy dependence of ${}_{}{}^{24}{}_{}{}^{}(\mathrm{p}\to$,d) cross section and analyzing-power measurements from 50 to 150 MeV

Detector telescope measurements of cross sections and analyzing powers for the ${}_{}{}^{24}{}_{}{}^{}(\mathrm{p}\to$,d) reaction to states of ${}_{}{}^{23}{}_{}{}^{}\mathrm{Mg}$ up to 4.36 MeV in excitation are reported for bombarding energies of 49.2 and 150.3 MeV. Taken together with earlier spectrometer measurements at 94.8 MeV at the same laboratory, a smooth energy dependence of the results for transitions leading to ${1/2}^{+}$, ${1/2}^{\mathrm{-}}$, ${\mathrm{}(3/2)\mathrm{}}^{\mathrm{-}}$, ${\mathrm{}(3/2)\mathrm{}}^{+}$, ${\mathrm{}(5/2)\mathrm{}}^{+}$, and ${\mathrm{}(7/2)\mathrm{}}^{+}$ states is obtained. Exact finite-range, adiabatic, distorted-wave analyses give reasonable fits in most cases to the cross-section angular distributions using an rms radius prescription for the bound-state geometry, and the energy-dependent set of proton optical potentials employed by Hatanaka extrapolated to higher energies; however, the calculated analyzing powers often differ in magnitude and shape from experiment. With the exception of the $l_{\mathrm{n}}$=0 transitions, spectroscopic factors derived from this particular comparison exhibit only a relatively small energy dependence.