A Tarifeno-Saldivia
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Explore the profile of A Tarifeno-Saldivia including associated specialties, affiliations and a list of published articles.
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8
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3
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Recent Articles
1.
Yeung T, Morales A, Wu J, Liu M, Yuan C, Nishimura S, et al.
Phys Rev Lett
. 2024 Aug;
133(7):072501.
PMID: 39213556
Isomer spectroscopy of heavy neutron-rich nuclei beyond the N=126 closed shell has been performed for the first time at the Radioactive Isotope Beam Factory of the RIKEN Nishina Center. New...
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.
Phong V, Nishimura S, Lorusso G, Davinson T, Estrade A, Hall O, et al.
Phys Rev Lett
. 2022 Nov;
129(17):172701.
PMID: 36332266
The β-delayed one- and two-neutron emission probabilities (P_{1n} and P_{2n}) of 20 neutron-rich nuclei with N≥82 have been measured at the RIBF facility of the RIKEN Nishina Center. P_{1n} of...
6.
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...
7.
Damone L, Barbagallo M, Mastromarco M, Mengoni A, Cosentino L, Maugeri E, et al.
Phys Rev Lett
. 2018 Aug;
121(4):042701.
PMID: 30095928
We report on the measurement of the ^{7}Be(n,p)^{7}Li cross section from thermal to approximately 325 keV neutron energy, performed in the high-flux experimental area (EAR2) of the n_TOF facility at...
8.
Barbagallo M, Musumarra A, Cosentino L, Maugeri E, Heinitz S, Mengoni A, et al.
Phys Rev Lett
. 2016 Oct;
117(15):152701.
PMID: 27768364
The energy-dependent cross section of the ^{7}Be(n,α)^{4}He reaction, of interest for the so-called cosmological lithium problem in big bang nucleosynthesis, has been measured for the first time from 10 meV...