Publications of P. Adsley sorted by first author
Authors associated with the Cyclotron Institute are , and those associated with Center of Excellence in Nuclear Training And University-based Research (CENTAUR) have a * next to their name.
A
Extending the Hoyle-State Paradigm to $^{12}$C$+^{12}$C Fusion, *, , , , , , , , , , , , , , , and , Phys. Rev. Lett. 129, 102701 (2022) | pub id: 1249 [DOI] [URL] |
$^{21}\mathrm{Ne}$ energy levels approaching the $\alpha$-particle threshold, , , , *, , , , , and , Phys. Rev. C 109, 044323 (2024) | pub id: 1380 [DOI] [URL] |
B
Isoscalar giant monopole resonance in $^{24}\mathrm{Mg}$ and $^{28}\mathrm{Si}$: Effect of coupling between the isoscalar monopole and quadrupole strength, , , , , , , , , *, , , , , , , , , , , , , , , , , and , Phys. Rev. C 105, 024311 (2022) | pub id: 1210 [DOI] [URL] |
Isoscalar giant monopole strength in $^{58}\mathrm{Ni}$, $^{90}\mathrm{Zr}$, $^{120}\mathrm{Sn}$, and $^{208}\mathrm{Pb}$, , , , , , *, , , , , , , , , , , , , , , , , , and , Phys. Rev. C 107, 034312 (2023) | pub id: 1326 [DOI] [URL] |
Fine structure of the isoscalar giant monopole resonance in $^{58}$Ni, $^{90}$Zr, $^{120}$Sn, and $^{208}$Pb, , , , , , , , , , *, , , , , , , , , , , , , , , , , , and , Phys. Rev. C 109, 014325 (2024) | pub id: 1345 [DOI] [URL] |
Proton decays from $\alpha$-unbound states in $^{22}\mathrm{Mg}$ and the $^{18}\mathrm{Ne}(\alpha,p_0)^{21}\mathrm{Na}$ cross section, , *, , , , , , , , , , , , , , , and , Phys. Rev. C 107, 055802 (2023) | pub id: 1316 [DOI] [URL] |
C
Searching for resonance states in $^{22}\mathrm{Ne}(p,\gamma)^{23}\mathrm{Na}$, , , *, , , , , , , , , , , , , , , and , Phys. Rev. C 108, 045802 (2023) | pub id: 1350 [DOI] [URL] |
Exploring the astrophysical energy range of the $^{27}\mathrm{Al}(p,\alpha)^{24}\mathrm{Mg}$ reaction: A new recommended reaction rate, , , *, , , , , , , , , , , , , , , , , , and , Physics Letters B 826, 136917 (2022) | pub id: 1207 [DOI] [URL] |
A New Reaction Rate of the $^{27}\mathrm{Al}(p/\alpha)^{24}\mathrm{Mg}$ Reaction Based on Indirect Measurements at Astrophysical Energies and Implications for $^{27}\mathrm{Al}$ Yields of Intermediate-mass Stars, , , *, , , , , , , , , , , , , , , , , , , , and , The Astrophysical Journal 941, 96 (2022) | pub id: 1307 [DOI] [URL] |
D
Photo-response of the $N=Z$ nucleus $^{24}\mathrm{Mg}$, , , , , , , , , , , , , , , , , *, , , , , , , , , , , , , , , , , , , , , , , , , and , The European Physical Journal A 59, 10 (2023) | pub id: 1334 [DOI] [URL] |
F
The impact of $^{17}\mathrm{O}+\alpha$ reaction rate uncertainties on the $s$-process in rotating massive stars, , *, , , , , , , , , and , Monthly Notices of the Royal Astronomical Society 514, 2650--2657 (2022) | pub id: 1243 [DOI] [URL] |
G
New narrow resonances observed in the unbound nucleus $^{15}\mathrm{F}$, , , , , , , , , , , , , , , , *, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and , Phys. Rev. C 105, L051301 (2022) | pub id: 1225 [DOI] [URL] |
Examination of how properties of a fissioning system impact isomeric yield ratios of the fragments, , , , , , , , , , , , , , , *, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and , Phys. Rev. C 108, 064602 (2023) | pub id: 1354 [DOI] [URL] |
H
Experimental Determination of $\alpha$ Widths of $^{21}\mathrm{Ne}$ Levels in the Region of Astrophysical Interest: New $^{17}\mathrm{O}+\alpha$ Reaction Rates and Impact on the Weak $s$ Process, , *, , , , , , , , , , , , , , , , and , Phys. Rev. Lett. 132, 182701 (2024) | pub id: 1379 [DOI] [URL] |
Experimental study of the $^{30}\mathrm{Si}(^3\mathrm{He},d)^{31}\mathrm{P}$ reaction and thermonuclear reaction rate of $^{30}\mathrm{Si}(p,\gamma)^{31}\mathrm{P}$, , , *, , , , , , , , , , , , and , Phys. Rev. C 105, 015805 (2022) | pub id: 1195 [DOI] [URL] |
K
Isospin mixing and the cubic isobaric multiplet mass equation in the lowest $T=2$, $A=32$ quintet, , , , , , *, , , , , , , , , , , , , , , , , , , , and , Phys. Rev. C 104, L061303 (2021) | pub id: 1187 [DOI] [URL] |
L
Progress on nuclear reaction rates affecting the stellar production of $^{26}\mathrm{Al}$, , , , *, , , , , , , , , , , , , , , , , , , , , , and , Journal of Physics G: Nuclear and Particle Physics 50, 033002 (2023) | pub id: 1298 [DOI] [URL] |
Multiprobe study of excited states in $^{12}\mathrm{C}$: Disentangling the sources of monopole strength between the energy of the Hoyle state and $E_x=13~\mathrm{MeV}$, , *, , , , , , , , , , , , , , , , , , , , , , , , , and , Phys. Rev. C 105, 024308 (2022) | pub id: 1209 [DOI] [URL] |
Understanding the total width of the $3^?_1$ state in $^{12}$C, , , *, , , , , , , , , , , and , Phys. Rev. C 109, 015806 (2024) | pub id: 1346 [DOI] [URL] |
Investigating the predicted breathing-mode excitation of the Hoyle state, , , *, , , , , , , , , , , , , , , , , , , , , , , , and , Physics Letters B 827, 136928 (2022) | pub id: 1208 [DOI] [URL] |
M
A new $^{12}\mathrm{C}+^{12}\mathrm{C}$ nuclear reaction rate: Impact on stellar evolution, , , , , , , , *, , , , and , Astronomy & Astrophysics 660, A47 (2022) | pub id: 1217 [DOI] [URL] |
Search for in-band transitions in the candidate superdeformed band in $^{28}\mathrm{Si}$, , , , , , , , *, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and , Phys. Rev. C 104, 054323 (2021) | pub id: 1188 [DOI] [URL] |
O
Evolution of the isoscalar giant monopole resonance in the Ca isotope chain, , , , , , *, , , , , , , , , , , , , , , , , , , , , and , Phys. Rev. C 105, 054319 (2022) | pub id: 1239 [DOI] [URL] |
R
$^{138}\mathrm{Ba}(d,\alpha)$ Study of States in $^{136}\mathrm{Cs}$: Implications for New Physics Searches with Xenon Detectors, , , , , , , , *, , , , , , , , , , , , , , , and , Phys. Rev. Lett. 131, 052501 (2023) | pub id: 1328 [DOI] [URL] |
S
Horizons: nuclear astrophysics in the 2020s and beyond, , *, , , , , *, , and , Journal of Physics G: Nuclear and Particle Physics 49, 110502 (2022) | pub id: 1276 [DOI] [URL] |
Occupation probabilities of valence orbitals relevant to neutrinoless double $\beta$ decay of $^{124}\mathrm{Sn}$, , , , , *, , , , , , , , , , and , Phys. Rev. C 105, 014605 (2022) | pub id: 1211 [DOI] [URL] |
Neutron occupancies and single-particle energies across the stable tin isotopes, , , , , , *, , , , , , , , , , , and , Phys. Rev. C 104, 054308 (2021) | pub id: 1183 [DOI] [URL] |
T
Study of $N=50$ gap evolution around $Z=32$: new structure information for ${}^{82}\mathrm{Ge}$, , , , , , , , , *, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and , The European Physical Journal A 59, 153 (2023) | pub id: 1325 [DOI] [URL] |
W
New measurement of the $E_\mathrm{c.m.}=323$ keV resonance in the $^{19}\mathrm{F}(p,\gamma)^{20}\mathrm{Ne}$ reaction, , *, , , , , , and , Phys. Rev. C 103, 055805 (2021) | pub id: 1124 [DOI] [URL] |
Constraints on key $^{17}\mathrm{O}(\alpha,\gamma)^{21}\mathrm{Ne}$ resonances and impact on the weak $s$ process, , , , *, , , , , and , Phys. Rev. C 105, 065805 (2022) | pub id: 1244 [DOI] [URL] |