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Introduccion ot detector test (for g-flash) at n_TOF (October 2012). Carlos GUERRERO CERN Fellow , Physics Department. Proposals EAR-2. Still planed for EAR-2 (in EAR-1 we would need to much Pu mass) Detection for g-rays: in principle C6D6
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Introduccionot detector test (for g-flash) at n_TOF (October 2012) Carlos GUERRERO CERN Fellow, PhysicsDepartment
Proposals EAR-2 Still planed for EAR-2 (in EAR-1 we would need to much Pu mass) Detection for g-rays: in principle C6D6 Detection for fission: in principle MGAS (maybe PPAC s) Samples: see ‘samples’ slides
Proposals EAR-2 Still planed for EAR-2 (in EAR-1 we would need to much Se mass) (See Cesar’s talk) Detection for g-rays: in principle 4p detect needed (optimize edet + separate backg.) Samples: see ‘samples’ slides
Proposals EAR-2 Prompt fission g-rays from fission in 233,235U and 239,241Pu (All in NEA-HPRL) C. Guerrero and collaborators MGAS with high resolution scintillators (NaI or better [LaCl3, LaBr3, CeBr3, HPGe]) n Scintillator g’s Sample