activity
20052020
most citedSearch for new resonant states in 10C and 11C and their impact on the cosmological lithium problem

48 citations · 244 across the 12 of their papers we have counts for

collaborators

12 papers

nucl-ex2020★ 6 cited

Sub-threshold states in Ne relevant to F(p,)O

J. E. Riley, A. M. Laird, N. de Séréville +24

Classical novae result from thermonuclear explosions producing several -ray emitters which are prime targets for satellites observing in the MeV range. The early 511 keV gamma-r…

nucl-ex2020★ 1 cited

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…

nucl-ex2020★ 10 cited

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…

nucl-ex2018

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…

nucl-ex2016★ 41 cited

An above-barrier narrow resonance in F

F. De Grancey, A. Mercenne, F. de Oliveira Santos +37

Intense and purified radioactive beam of post-accelerated O was used to study the low-lying states in the unbound F nucleus. Exploiting resonant elastic scattering in…

nucl-ex2014★ 46 cited

Probing Nuclear forces beyond the drip-line using the mirror nuclei N and F

I. Stefan, F. de Oliveira Santos, O. Sorlin +29

Radioactive beams of O and O were used to populate the resonant states 1/2, 5/2 and in the unbound F and F nuclei respectively by…