6533b86ffe1ef96bd12cd340

RESEARCH PRODUCT

Mass measurements towards doubly magic Ni-78 : Hydrodynamics versus nuclear mass contribution in core-collapse supernovae

S. GiraudL. CaneteB. BastinA. KankainenA.f. FantinaF. GulminelliP. AscherT. EronenV. Girard-alcindorA. JokinenA. KhanamI.d. MooreD.a. NesterenkoF. De Oliveira SantosH. PenttiläC. PetroneI. PohjalainenA. De RoubinV.a. RubchenyaM. VilenJ. ÄYstö

subject

NUCLEOSYNTHESISIONSCore-collapse supernovaNuclear and High Energy PhysicsScience & TechnologyIMPACTPhysicsPenning trapR-PROCESSneutronitAstronomy & Astrophysics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]114 Physical sciencesSTATEPhysics Particles & FieldsPhysics NuclearSPECTROMETRYPhysical SciencesISOTOPESNuclear massNuclear Physics - ExperimentydinfysiikkaShell gap

description

International audience; We report the first high-precision mass measurements of the neutron-rich nuclei 74,75Ni and the clearly identified ground state of 76Cu, along with a more precise mass-excess value of 78Cu, performed with the double Penning trap JYFLTRAP at the Ion Guide Isotope Separator On-Line (IGISOL) facility. These new results lead to a quantitative estimation of the quenching for the N=50 neutron shell gap. The impact of this shell quenching on core-collapse supernova dynamics is specifically tested using a dedicated statistical equilibrium approach that allows a variation of the mass model independent of the other microphysical inputs. We conclude that the impact of nuclear masses is strong when implemented using a fixed trajectory as in the previous studies, but the effect is substantially reduced when implemented self-consistently in the simulation.

10.1016/j.physletb.2022.137309http://hdl.handle.net/10138/350386