0000000000116794

AUTHOR

F. Hammache

showing 4 related works from this author

Study of $^{45}$Ar through (d, p) reaction at SPIRAL

2005

NESTER; International audience; The structure of the neutron-rich nucleus $^{45}$Ar has been investigated through the d($^{44}$Ar,$^{45}$Ar)p transfer reaction. Radioactive beam of $^{44}$Ar at 10 A MeV has been provided by the SPIRAL facility at GANIL. The protons corresponding to a neutron pick-up on bound or unbound states mechanism in $^{45}$Ar nuclei were detected at backward angles by the detector array MUST. The transfer-like ejectiles were detected in the SPEG spectrometer. Level scheme, spin assignments and spectroscopic factors have been deduced for $^{45}$Ar and compared to shell model predictions. These parameters will be subsequently used to infer (n, $\gamma$) cross sections i…

PhysicsNuclear and High Energy PhysicsSpectrometer010308 nuclear & particles physicsSHELL modelNuclear Theory[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyNuclear physicsmedicine.anatomical_structure0103 physical sciencesPhysics::Space PhysicsmedicineAstrophysics::Solar and Stellar AstrophysicsNeutronAtomic physicsDetector array010306 general physicsSpin (physics)Nuclear ExperimentNucleusRadioactive beamSpiral
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Coulomb dissociation of 27P

2011

International audience; In this work the astrophysical 26Si(p,γ)27P reaction is studied using the Coulomb dissociation technique. We performed a 27P Coulomb Dissociation experiment at GSI, Darmstadt (28 May-5 June 2007) using the ALADIN-LAND setup which allows complete-kinematic studies. A secondary 27P beam at 498 AMeV impinging a 515mg/cm2 Pb target was used. The relative energy of the outgoing system (26Si+p) is measured obtaining the resonant states of the 27P. Preliminary results show four resonant states measured at 0.36±0.07, 0.88±0.09, 1.5±0.2, 2.3±0.3 MeV and evidence of a higher state at around 3.1 MeV. The preliminary total cross section obtained for relative energies between 0 a…

History010308 nuclear & particles physicsChemistry[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesDissociation (chemistry)Computer Science ApplicationsEducationNuclear physics0103 physical sciencesCoulombAtomic physics010306 general physicsRelative energy
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Structure of theN=27isotones derived from theAr44(d,p)Ar45reaction

2008

The $^{44}\mathrm{Ar}$($d,p$)$^{45}\mathrm{Ar}$ neutron transfer reaction was performed at $10A$ MeV. Measured excitation energies, deduced angular momenta, and spectroscopic factors of the states populated in $^{45}\mathrm{Ar}$ are reported. A satisfactory description of these properties is achieved in the shell model framework using a new $\mathit{sdpf}$ interaction. The model analysis is extended to more exotic even-$Z$ nuclei down to ${}_{14}^{41}{\mathrm{Si}}_{27}$ to study how collectivity impacts the low-lying structure of $N=27$ neutron-rich nuclei.

PhysicsNuclear reactionNuclear and High Energy PhysicsAngular momentum010308 nuclear & particles physicsNuclear TheoryStructure (category theory)01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsNeutronIsotopes of siliconAtomic physicsNuclear Experiment010306 general physicsRadioactive decayExcitationDimensionless quantityPhysical Review C
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Coulomb dissociation of 27P: A reaction of astrophysical interest

2011

The ground-state decay of 26Al(0+) (T 1/2=1.05× 106) has a shorter life-time than the Universe. The presence of this element in the Galaxy was measured via g-ray spectroscopy, showing that the nucleosynthesis of this element is an ongoing process in stars. The proton-capture reaction 26Si(p,γ) 27P competes with the production of 26Al(0+) by β-decay. Coulomb dissociation of 27P has been suggested as an indirect method to measure radiative-proton capture when the direct reaction is not feasible. Such an experiment was performed at GSI with a secondary 27P beam produced by fragmenting a 36Ar primary beam at 500 A MeV. Two main observables are preliminarily presented in this work: the reaction …

PhysicsStarsNucleosynthesisCoulombCoulomb barrierObservableAtomic physicsSpectroscopyDissociation (chemistry)Galaxy
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