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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


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