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Dive into the first simulations of FAZIA in 2007 and technical aspects for FAZIA physics, including EOS observables, exotic states, evaporation, and more. Explore charged particle correlations, neutron detectors, and nuclear structure in non-Weißkopf decays using various detectors and simulations.
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First simulations of FAZIA Napoli 3-5 September 2007
Technical requirements for the physics of FAZIA • Dynamics and EOS observables @ EURISOL • AIMF , b • 4p, pulse shape ( high granularity) • Exotic states @ SPIRAL/SPIRAL2 • high-resolution charged particle correlations • high granularity, |k| resolution • Evaporation, level densities @ SPIRAL/SPIRAL2 • A1 , E* • 4p, pulse shape ( high granularity), low thresholds, coupling with spectrometers, neutron detectors • …….And the other physics cases of the proposal, for further study…… • Very adaptable geometry (beams, detectors)
Simulation • Geometry : • INDRA • INDRA4 • (~ Chimera) • INDRA16 • (FAZIA?) • Configuration • for test: • 2 arrays in • 2 chambers : Neutron detector ? Target Beam • Spherical array + • Surrounded by • neutron detectors? • Annular array • High granularity (strips?) • Replaceable with a spectrometer
Simulation [deg] INDRA [deg] • Options for the detector : • Aup to element Zn, • otherwise EPAX • |k| with uncertainty 5% • Double hits A, K adds • 4p neutron detectors: • efficiency (~20%), • |kn| with uncertainty15% • Geometric coverage ~ 87%
Simulation • 36Ar+58Ni 12 A MeV Select c.n. 94Pd at 241 MeV, 1.8 cm/ns (lab) • 129Xe+Sn 50 A MeV Select q.p. 120Sn at 400 MeV, 9 cm/ns (lab) INDRA
Simulation • Reactions : • GEMINI • 12C+24Mg 100 A MeV Select 12C at 30 MeV, 5.3 cm/ns (lab) • 36Ar+58Ni 12 A MeV Select c.n. 94Pd at 241 MeV, 1.8 cm/ns (lab) • 129Xe+Sn 50 A MeV Select q.p. 120Sn at 400 MeV, 9 cm/ns (lab) • !!! : Too good agreement with EPAX • HIPSE • 58Ni+58Ni / 68Ni+68Ni40 A MeV q.p. + q.t. • 112Sn+112Sn / 132Sn+132Sn40 A MeV q.p. + q.t. • QMD • 58Ni+58Ni / 68Ni+68Ni150 A MeV q.p. + q.t. • 112Sn+112Sn / 132Sn+132Sn150 A MeV q.p. + q.t.
Charged-particle correlations @ SPIRAL/SPIRAL2 • 12C+24Mg 100 A MeV • Select 12C at 30 MeV, 5.3 cm/ns (lab) • Nuclear structure in exotic (non-Weißkopf) decays: • Probing excited heavy cluster states • 12C decays in Li+Li • |k| perfectly measured: • INDRA: not adapted • INDRA4: main peak • INDRA16: 2 peaks
|k| with uncertainty 0%, 2%, 5% Forward angles |k| is measured with an uncertainty INDRAINDRA4 INDRA16
|k| with uncertainty 0%, 2%, 5% Backward angles |k| is measured with an uncertainty INDRAINDRA4 INDRA16
Dynamics and EOS observables @ EURISOL • Etrans12 measured precisely with • any granularity INDRA • Correspondence with b (from the model) • N/Z of IMF as a function of Etrans12 • A up to Z=3: not adapted • A up to Z=28 • (all IMF identified): resolved • Small Etrans12 may suffer from • the hole of the beam
Average neutron spectra (preliminary) • Neutron multiplicity by • A-Z in complete events • Mean neutron spectrum • measured with a surrounding • array, to be defined
Conclusions • FAZIA simulator • Geometric options: OK • More detailed detector properties: Next • Physics cases model simulations filtering solutions for FAZIA