STATUS OF THE GALILEO PROJECT
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1 STATUS OF THE GALILEO PROJECT AT LNL Jose Javier Valiente Dobon LNL (INFN) 27/9/2012 SPES One dayworkshop September 2012
2 The GALILEO project take advantage of the recent technical developments for AGATA preamplifiers, digital sampling, preprocessing, DAQ high counting rates (30 50 khz/det) use of existing detectors EB cluster detectors capsules GASP detectors high photopeak efficiency use beam facilities at LNL Tandem, ALPI, PIAVE stable SPES RIB production of new nuclei 30 GASP 22.5cm o 51 o 59 o 121 o 129 o 151 o 10 triple cluster (EB 24cm 90 o ε ph ~ 8% P/T ~ 50%
3 GALILEO Mechanics & Detectors Triple cluster cryostat o end cap, cold finger, dewar o use of the EB cluster capsules Anti Compton shield for the TC detector o recover the crystals from the original EB cluster shields Holding structure o highly flexible, space for ancillary detectors Pb collimator o divided in 4 parts Reaction chamber o accomodate different ancillary detectors Beam line o the structure opens along the beam line Ancillary detectors o integration with the holding structure
4 Triple Cluster Detector R&D Development of the triple cryostat end cap in carbon fiber dewar optimizing the thermal conduction (LN 2 consumption) EB cluster detectors 7 encapsulated n type HPGe detectors FWHM < kev ε int kev common cryostat independent HV/LV
5 Triple Cluster Detector First Prototype End cap in Carbon fiber EB capsules Cold finger Dewar Electronics (warm section) Zeolites container GALILEO criostat First prototype under test It is being modified in the workshop
6 AC shields for the triple TC detectors q a proposal for the construction of the triple cluster AC shield out of the individual crystals of the original EB cluster shield one can build only one new shield from the original one
7 The Triple Cluster Detector AC Shields q one can safely dismount the crystals and phototubes
8 GALILEO Holding Structure Design by C.Fanin
9 GALILEO Holding Structure
10 GALILEO Location Experimental Hall II replacing GASP PISOLO 8piLP RMS July 2012 alignment of the beam line with beam
11 GALILEO Electronics & DAQ New electronics is being built in close synergy with AGATA low noise, fast, low power consumption * use solutions already developed for AGATA core type preamplifiers done GTS done AGAVA interface with the VME electronics (collab. with Kracow) o new developments for AGATA and GALILEO low power digitizers prototype test readout and preprocessing on PCI express boards prototype test o anti Compton shields signal readout digital (similar to the Ge detectors)
12 GALILEO Electronics a fast low noise charge sensitive preamplifier based on the core type AGATA preamplifier used for both tapered and triple cluster detectors 80 preamplifiers already available! Digi-opt12: 12-channel 14/16-bit 100/125-MS/s digitizer with optical output for GALILEO/AGATA power consumption < 10 W / board prototypes (5) under test new low power and low cost readout and preprocessing PCI express boards developed for GALILEO and AGATA prototypes (3) under test
13 GALILEO Electronics & DAQ Fully synchronous system with global" 100 MHz clock and time-stamp distribution New AGATA core like preamplifiers differential output, one 10 MeV range - done GTS clk Detector Ge Preamps Detector AC Preamps New Digitizers: 100 Ms/s, 14 bit prototype ready Optical fiber read-out of full data" stream to pre-processing electronics Digitizers Digitizers 0.2 GB/s/det New local processing: determine energy, time and isolate ~ 600 ns of signal around rise-time First prototype fully operational 38 channels Buffers of time-stamped local events sent" to PSA if needed neutron damage correction XDAQ PCI Express board Local processing Local processing khz trigger 15 MB/s/det PSA PSA 2.5 MB/s/det Global event builder and software trigger Event Builder Control and storage, On line Storage
14 GALILEO Ancillary Detectors Study of weak reaction channels or weakly populated structures LoI letters of intent (30 institutes, 11 countries) high efficiency + high resolving power Light charged particles detectors Neutron detectors Binary reactions fragment detectors Lifetime measurement Recoil detectors High energy g ray detectors Fast timing detectors HECTOR HECTOR+ PARIS Prototype
15 GALILEO RFD & N Wall 3D Model RFD Kracow N Wall
16 Summary R&D for improving detectors and electronics " higher detector granularity " improved efficiency at high energies (composite configuration) " low noise, fast electronics " digital treatment of the signals The building of GALILEO proceeds " the holding structure " triple cluster cryostats " triple cluster anti Compton shields " LN 2 filling system Integration of ancillary detectors " RFD and N Wall in advanced stage " others EUCLIDES, TRACE, SPIDER, LUSIA Expected to start the physics campaign in summer 2013
17 Satellite workshop to INPC2013 Symposyum on Nuclear Structure with Large Gamma Ray Arrays NSP 2013 Padova, June 10 12, 2013
18 GALILEO Triple cryostat GASP Rel. Efficiency cluster addback 7-cluster addback Rel. Efficiency [a.u.] GASP 7-cluster/7 3-cluster/ Energy [MeV] GEANT4 Simulations by E.Farnea
19 GALILEO Beam line design 82 Se 450 MeV M.Comunian Ion optics calculations performed by the accelerator division at LNL beam envelope in X (top) and Y (bottom) directions GALILEO target position
20 GALILEO LN 2 Filling System same logic flow as for GASP and EUROBALL based on NI CompactRio architecture Under construction at the electronics lab. of INFN Padova
21 AC shields for the triple TC detectors q moved one EB cluster AC shield to Legnaro demonstrate the possibility of safely dismounting the crystals and phototubes
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