57 citations · 453 across the 25 of their papers we have counts for
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Decay Pattern of Pygmy States Observed in Neutron-Rich 26 Ne
J. Gibelin, D. Beaumel, T. Motobayashi +23
Coulomb excitation of the exotic neutron-rich nucleus Ne26 on a Pb208 target was measured at 58 MeV/u in order to search for low-lying E1 strength above the neutron emission thresh…
N=16 magicity revealed at the proton drip-line through the study of 35Ca
L. Lalanne, O. Sorlin, A. Poves +27
The last proton bound calcium isotope Ca has been studied for the first time, using the Ca()Ca two neutron transfer reaction. The radioactive Ca n…
Multiple Mechanisms in Proton-Induced Nucleon Removal at 100 MeV/Nucleon
T. Pohl, Y. L. Sun, A. Obertelli +48
We report on the first proton-induced single proton- and neutron-removal reactions from the neutron-deficient O nucleus with large Fermi-surface asymmetry = 18.6 M…
The structure of Ca under the Coulomb magnifying glass
L. Lalanne, O. Sorlin, A. Poves +28
Detailed spectroscopy of the neutron-deficient nucleus Ca was obtained up to 9 MeV using the Ca(,)Ca and the Ca(,)Ca transfer reactio…
Narrow resonances in the continuum of the unbound nucleus F
V. Girard-Alcindor, A. Mercenne, I. Stefan +100
The structure of the unbound F nucleus is investigated using the inverse kinematics resonant scattering of a radioactive O beam impinging on a CH target. The anal…
Evaluation of the K(,)Ca reaction rate using the Ca(,)Ca transfer reaction
L. Lalanne, O. Sorlin, M. Assié +28
A recent sensitivity study has shown that the KCa reaction is one of the ten reaction rates that could significantly impact the shape of the calculated X…
Probing nuclear forces beyond the nuclear drip line: The cases of F and F
V. Girard-Alcindor, I. Stefan, F. de Oliveira Santos +53
The unbound proton-rich nuclei F and F are investigated experimentally and theoretically. Several experiments using the resonant elastic scattering method were perfor…
Charged-particle branching ratios above the neutron threshold in F: constraining N production in core-collapse supernovae
P. Adsley, F. Hammache, N. de Séréville +28
Spatially-correlated overabundances of N and O observed in some low-density graphite meteoritic grains have been connected to nucleosynthesis taking place in the heli…
Evaluation of the N(,p)O thermonuclear reaction rate and its impact on the isotopic composition of supernova grains
A. Meyer, N. de Séréville, A. M. Laird +12
It has been suggested that hydrogen ingestion into the helium shell of massive stars could lead to high C and N excesses when the shock of a core-collapse supernova p…
Study of multi-neutron systems with SAMURAI spectrometer
Z. H. Yang, F. M. Marqués, N. L. Achouri +95
The tetraneutron has been drawing the attention of the nuclear physics community for decades, but a firm conclusion on its existence and properties is still far from being reached…
How different is the core of F from O?
T. L. Tang, T. Uesaka, S. Kawase +43
The neutron-shell structure of F was studied using quasi-free (p,2p) knockout reaction at 270A MeV in inverse kinematics. The sum of spectroscopic factors of 0d o…
Charged-particle decays of highly excited states in F
P. Adsley, F. Hammache, N. de Séréville +23
Neutron-capture reactions on F in the helium-burning shell play an important role in the production of N during core-collapse supernovae. The competition between the…
Experimental study of the two-body spin-orbit force
G. Burgunder, O. Sorlin, F. Nowacki +31
Energies and spectroscopic factors of the first , , and states in the Si nucleus were determined by means of the (d,p) transfer reaction…
Search for new resonant states in 10C and 11C and their impact on the cosmological lithium problem
F. Hammache, A. Coc, N. de Séréville +28
The observed primordial 7Li abundance in metal-poor halo stars is found to be lower than its Big-Bang nucleosynthesis (BBN) calculated value by a factor of approximately three. Som…
Structure of unbound neutron-rich He studied using single-neutron transfer
T. Al Kalanee, J. Gibelin, P. Roussel-Chomaz +23
The 8He(d,p) reaction was studied in inverse kinematics at 15.4A MeV using the MUST2 Si-CsI array in order to shed light on the level structure of 9He. The well known 16O(d,p)17O r…
Emergence of the N=16 shell gap in 21O
B. Fernandez-Dominguez, J. S. Thomas, W. N. Catford +39
The spectroscopy of 21O has been investigated using a radioactive 20O beam and the (d,p) reaction in inverse kinematics. The ground and first excited states have been determined to…
Probing pre-formed alpha particles in the ground state of nuclei
J. A. Scarpaci, M. Fallot, D. Lacroix +18
In this Letter, we report on alpha particle emission through the nuclear break-up in the reaction 40Ca on a 40Ca target at 50A MeV. It is observed that, similarly to nucleons, alph…
Search for low lying dipole strength in the neutron rich nucleus Ne
J. Gibelin, D. Beaumel, T. Motobayashi +22
Coulomb excitation of the exotic neutron-rich nucleus Ne on a Pb target was measured at 58 A.MeV in order to search for low-lying E1 strength above the neutron emiss…
Indirect study of 19Ne states near the 18F+p threshold
N. de Sereville, A. Coc, C. Angulo +22
The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. Unfortunately the reaction rate of the 18F(p,a)15O reaction is still largely unc…
D(18F,pa)15N reaction applied to nova gamma-ray emission
N. de Sereville, A. Coc, C. Angulo +22
The 18F(p,alpha)15O reaction is recognized to be one of the most important reactions for nova gamma-ray astronomy as it governs the early E <= 511keV gamma emission. However in the…
Study of the ^18F(p, alpha)^15O reaction for application to nova gamma-ray emission
N. de Sereville, A. Coc, C. Angulo +22
The ^18F(p, alpha)^15O reaction is recognized as one of the most important reaction for nova gamma-ray astronomy as it governs the early =< 511 keV emission. However, its rate rema…
A new experiment for the determination of the 18F(p,alpha) reaction rate at nova temperatures
N. de Sereville, A. Coc, C. Angulo +22
The 18F(p,alpha) reaction was recognized as one of the most important for gamma ray astronomy in novae as it governs the early 511 keV emission. However, its rate remains largely u…