D G Jenkins
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Explore the profile of D G Jenkins including associated specialties, affiliations and a list of published articles.
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76
Citations
558
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Recent Articles
1.
Zimba G, Ruotsalainen P, Jenkins D, Satula W, Uusitalo J, Wadsworth R, et al.
Phys Rev Lett
. 2025 Feb;
134(2):022502.
PMID: 39913816
At a fundamental level, the interactions between protons and protons, protons and neutrons, and neutrons and neutrons are not identical. Such isospin nonconserving interactions emerge when comparing the excitation energy...
2.
Casanovas-Hoste A, Domingo-Pardo C, Lerendegui-Marco J, Guerrero C, Tarifeno-Saldivia A, Krticka M, et al.
Phys Rev Lett
. 2024 Aug;
133(5):052702.
PMID: 39159101
Asymptotic giant branch stars are responsible for the production of most of the heavy isotopes beyond Sr observed in the solar system. Among them, isotopes shielded from the r-process contribution...
3.
Amaducci S, Colonna N, Cosentino L, Cristallo S, Finocchiaro P, Krticka M, et al.
Phys Rev Lett
. 2024 Apr;
132(12):122701.
PMID: 38579210
^{140}Ce(n,γ) is a key reaction for slow neutron-capture (s-process) nucleosynthesis due to being a bottleneck in the reaction flow. For this reason, it was measured with high accuracy (uncertainty ≈5%)...
4.
Lederer-Woods C, Aberle O, Andrzejewski J, Audouin L, Becares V, Bacak M, et al.
Eur Phys J A Hadron Nucl
. 2022 Dec;
58(12):239.
PMID: 36514540
Neutron capture reaction cross sections on Ge are of importance to determine Ge production during the astrophysical slow neutron capture process. We present new resonance data on Ge( ) reactions...
5.
Adsley P, Heine M, Jenkins D, Courtin S, Neveling R, Brummer J, et al.
Phys Rev Lett
. 2022 Sep;
129(10):102701.
PMID: 36112434
Carbon burning is a key step in the evolution of massive stars, Type 1a supernovae and superbursts in x-ray binary systems. Determining the ^{12}C+^{12}C fusion cross section at relevant energies...
6.
Doherty D, Andreyev A, Seweryniak D, Woods P, Carpenter M, Auranen K, et al.
Phys Rev Lett
. 2021 Dec;
127(20):202501.
PMID: 34860042
Two long-standing puzzles in the decay of ^{185}Bi, the heaviest known proton-emitting nucleus are revisited. These are the nonobservation of the 9/2^{-} state, which is the ground state of all...
7.
Guerrero C, Lerendegui-Marco J, Paul M, Tessler M, Heinitz S, Domingo-Pardo C, et al.
Phys Rev Lett
. 2020 Oct;
125(14):142701.
PMID: 33064503
The neutron capture cross sections of several unstable nuclides acting as branching points in the s process are crucial for stellar nucleosynthesis studies. The unstable ^{171}Tm (t_{1/2}=1.92 yr) is part...
8.
Fruet G, Courtin S, Heine M, Jenkins D, Adsley P, Brown A, et al.
Phys Rev Lett
. 2020 May;
124(19):192701.
PMID: 32469543
The ^{12}C+^{12}C fusion reaction plays a critical role in the evolution of massive stars and also strongly impacts various explosive astrophysical scenarios. The presence of resonances in this reaction at...
9.
Llewellyn R, Bentley M, Wadsworth R, Iwasaki H, Dobaczewski J, de Angelis G, et al.
Phys Rev Lett
. 2020 May;
124(15):152501.
PMID: 32357059
The lifetimes of the first excited 2^{+} states in the N=Z nuclei ^{80}Zr, ^{78}Y, and ^{76}Sr have been measured using the γ-ray line shape method following population via nucleon-knockout reactions...
10.
Timar J, Chen Q, Kruzsicz B, Sohler D, Kuti I, Zhang S, et al.
Phys Rev Lett
. 2019 Mar;
122(6):062501.
PMID: 30822069
New rotational bands built on the ν(h_{11/2}) configuration have been identified in ^{105}Pd. Two bands built on this configuration show the characteristics of transverse wobbling: the ΔI=1 transitions between them...