Implementation of the Implementation of the concept: AGATA/GRETA concept: AGATA/GRETA
- Specs
- Configurations of 4π Arrays
- Monte Carlo simulations
- The detectors
- Status
Implementation of the Implementation of the concept: AGATA/GRETA - - PowerPoint PPT Presentation
Implementation of the Implementation of the concept: AGATA/GRETA concept: AGATA/GRETA Specs Configurations of 4 Arrays Monte Carlo simulations The detectors Status Requirements for a Gamma Tracking Array Requirements
efficiency, energy resolution, dynamic range, angular resolution, timing, counting rate, modularity, angular coverage, inner space Quantity Target Value Specified for
50 % 25 % 10 % 60 - 70 % 40 - 50 % better than 1° 3 MHz 300 kHz > 34 cm Photo-peak efficiency (εph) Eγ = 1 MeV, Mγ = 1, β < 0.5 Eγ = 1 MeV, Mγ =30, β < 0.5 Eγ =10 MeV, Mγ = 1 Peak-to-total ratio (P/T) Eγ = 1 MeV, Mγ = 1 Eγ = 1 MeV, Mγ = 30 Angular resolution (Δθγ) for ΔE/E < 1% at large β Maximum event rates Mγ = 1 Mγ = 30 Inner diameter for ancillary detectors
Start with a platonic solid e.g. an icosahedron On its faces, draw a regular pattern of triangles grouped as hexagons and pentagons. E.g. with 110 hexagons and (always) 12 pentagons Project the faces
sphere; flatten the hexagons.
Space for encapsulation and canning obtained cutting the
crystals form a triple cluster Add encapsulation and part of the cryostats for realistic MC simulations Al capsules 0.4 mm spacing 0.8 mm thick Al canning 2.0 mm spacing 1.0 mm thick A radial projection of the spherical tiling generates the shapes of the detectors. Ball with 180 hexagons.
120 hexagonal crystals 2 shapes 30 quadruple-clusters all equal Inner radius (Ge) 18.5 cm Amount of germanium 237 kg Solid angle coverage 81 % 4320 segments Efficiency: 41% (Mγ=1) 25% (Mγ=30) Peak/Total: 57% (Mγ=1) 47% (Mγ=30)
Ge crystals size: Length 90 mm Diameter 80 mm
180 hexagonal crystals 3 shapes 60 triple-clusters all equal Inner radius (Ge) 23.5 cm Amount of germanium 362 kg Solid angle coverage 82 % 6480 segments Efficiency: 43% (Mγ=1) 28% (Mγ=30) Peak/Total: 58% (Mγ=1) 49% (Mγ=30)
Response function Absolute efficiency value includes the effects of the tracking algorithms! Values calculated for a source at rest.
5 asymmetric triple-clusters 36-fold segmented crystals 555 digital-channels
Full EDAQ with on line PSA and γ-ray tracking In beam Commissioning First installation site: LNL
Main issue is Doppler correction capability → coupling to beam and recoil tracking devices
INFN - LNL
INFN - LNL 195 MeV 195 MeV 36
36S +
S + 208
208Pb,
Pb, θ θlab
lab = 80
= 80o
E (a.u a.u.) .) Δ ΔE ( E (a.u a.u.) .)
Z=16 Z=16 Z=28 Z=28
X Y X position X position Y position Y position
Δ ΔE/E < 2% E/E < 2% Z/ Z/Δ ΔZ ~ 60 for Z=20 Z ~ 60 for Z=20 Δ Δt t < 500 < 500 ps ps Δ ΔX = 1 mm X = 1 mm Δ ΔY = 2 mm Y = 2 mm Δ Δt t ~ 350 ~ 350 ps ps, , Δ ΔX = 1 mm X = 1 mm Δ ΔY = 1 mm Y = 1 mm
First installation site for the Demonstrator: the PRISMA spectrometer at LNL
AGATA Demonstrator
MCP
Quadrupole Dipole MWPPAC Ion Chamber
β=20% The comparison between spectra
the event-by-event velocity vector shows that additional information will be essential to fully exploit the concept of tracking β (%) 5 20 50 δs(cm) 1.5 0.5 0.3
σdir(degrees)
2 0.6 0.3 Δβ (%) 2.4 0.7 0.3
Uncertainty on the recoil direction (degrees)
90Zr recoils with E~350 MeV (with 10% dispersion) assumed.
Agata Geant4 code + PRISMA simulation
Photopeak efficiency P/T Ratio
1 MeV photons, point source at rest. Tracking is performed.
~14cm: Possible target-detector distance for the Demonstrator on PRISMA
Peak FWHM Photopeak efficiency
Typical values for reaction products at PRISMA
2010 LNL 5TC 2012 GSI/FRS ≥8TC 2014 GANIL/SPIRAL2 ~15TC
AGATA D.+PRISMA
AGATA D. + VAMOS + EXOGAM
AGATA D. @ FRS
Total Eff. > 10%
Total Eff. > 20% Total Eff. ~6%
Cost 17 M$ (full project including man-power and contingency) 30 36-fold segmented detectors 10 triple-clusters Start construction 2007 Start operation 2010
Courtesy Canberra-Eurisys
Pulse Shape Simulations
A.Wiens et al. NIMA 618 (2010) 223 E.Farnea et al. NIMA 621 (2010)331
Implementation in GEANT4
Courtesy I-Yang Lee, LBNL Courtesy J.Eberth, IKP Cologne
Challenges:
spectroscopy channels
B-type A-type
TRACKING Control, Storage… EVENT BUILDER PSA FARM Core + 36 seg.
GL Trigger Clock 100 MHz T-Stamp
Other detectors
Fast 1st Level Trigger
interface to GTS, merge time-stamped data into event builder, prompt local trigger from digitisers
Other Detectors GTS DIGITIZER PREAMPL. ATCA Carrier GTS
Global Level
DAQ-NARVAL RUN- & SLOW-Control
HIGH THROUGHTPUT PRE- PROCESSING CARRIER / MEZZANINES
Other detectors Digital preamplifier concept
100MB/s/ detector
200MB/s/ segment
(300 kHz of M (300 kHz of Mγ
γ = 30
= 30 50 kHz singles) 50 kHz singles)
100 B/ev 5 MB/s 200 MB/s 1.5 ··· 7.5 kB/ev ~ 100 MB/s
36+1 7.5 kB/event
380 MB/s ~ 200 B/segment ~ 10 MB/s 100 Ms/s 14 bits
Pulse Shape Analysis Event Builder γ-ray Tracking HL-Trigger, Storage On Line Analysis
< 100 MB/s
SEGMENT GLOBAL Energy & Classification
5*n max. 900 MB/s
save 600 ns of
pulse rise time
E, t, x, y, z,...
DETECTOR
LL-Trigger Suppression / Compression ADC
+
GL-Trigger to reduce event rate to whatever value PSA will be able to manage 20 μs/event
F.Zocca, A.Pullia, G.Pascovici INFN-Milano, GANIL, IKP-Köln
ADC overflow voltage level
Saturated
pulsed-reset Ideal non-saturated
pulsed-reset Preamplifier output with continuous-reset (50μs decay time constant) Output with pulsed-reset
An ADC overflow condition would saturate the system for a long while A pulsed-reset mechanism allows a fast recovery of the output quiescent value, so minimizing the system dead time
F.Zocca, A.Pullia, G.Pascovici INFN-Milano, GANIL, IKP-Köln
O
2 1 1 2 2 1
E = energy of the large signal T = reset time
contribution of the tail due to previous events
V1 , V2 = pre-pulse and post-pulse baselines b1 , b2 , k1 , E0 = fitting parameters
second-order time-energy relation
Within ADC range standard “pulse-height mode” spectroscopy Beyond ADC range new “reset mode” spectroscopy F.Zocca, A.Pullia, G.Pascovici
Energy Resolution (fwhm) in pulse-height mode Resolution (fwhm) in reset mode 4.440 MeV (12C) 104 keV 2.34 % 104 keV 2.34 % ~5.6 MeV 10.5 keV 0.14 % 18.8 keV 0.34 % ~6.1 MeV 15.1 keV 0.17 % 17.1 keV 0.28 % 7.6312 MeV (Fe) 11 keV 0.14 % 7.6456 MeV (Fe) 11 keV 0.14 % 18.8 keV (29.4 keV for the double- peak) 0.25 % (0.38 % for the double- peak) 8.9984 MeV (Ni) 15 keV 0.17 % 18.9 keV 0.21 %
F.Zocca, A.Pullia, G.Pascovici
triple cluster)
purpose trigger (e.g. Fast trigger complementary detectors conventional electronics )
Excellent Performance: SNR average value 75.45 dB. ENOB average value 12.24 bits IPHC Strasbourg, The University of Liverpool, STFC-Daresbury
SEGMENT mezzanine (also Core mezzanine) 6 channels GTS mezzanine
The Pre-Processing is the first level that can interact with the Global Trigger through the GTS mezzannine. It receives, and send to the Digitizer, the Global clock synchronizing the system.
1 crystal needs : 2 ATCA carriers, 1 TCLK, 1 GTS, 7 segment mezzanines
Detector (Germanium) Detector (Germanium) Shaping Amplifier Shaping Amplifier CFD CFD DAQ E t FADC FADC MWD DCFD Filters DAQ E t ADC ADC TDC TDC PSA Tracking E t x,y,z E t
Segment Detector Array Detector (Germanium) Detector (Germanium)
Actual filter is trapezoidal
Moving Window
Moving Window Deconvolution (MWD) A.Georgiev and W. Gast, IEEE Trans. Nucl. Sci., 40(1993)770 V.T.Jordanov and G.F.Knoll, Nucl.Instr.Meth., A353(1994)261
Slope Condition Counting (SSC) Normalized Step Response (NSR) W.Gast et al, IEEE Trans.Nucl.Sci., 48(2001)2380
1 ms, 100 Ms/s
@ 40 kHz 28 events 5 pileups
Max capacity of 2 levels: 9 GTS 6 triple clusters + 2 ancillaries (AGAVA)
To the trigger A ternary tree for collecting the trigger requests, and distributing back the validations/rejections to GTS leaves
PCIe eval. board with a Virtex4 FX100 Partly in firmware (partitions, sumbuses) Partly in software running on the PPC Implemented by Luciano Berti (LNL) Present version: 48 inputs in 2 partitions Each partition has 4 multiplicity thresholds The two partitions can be in coincidence Typically: P1 with the Ge crystals P2 with the ancillary Trig1 P1 >=1 & P2 = 1 Trig2 P1 >=2
Root GUI for analysis NARVAL Producer
Front End Electronics
NARVAL Producer
Front End Electronics
Pre Processing Pre Processing Pulse Shape Analysis Pulse Shape Analysis Event Building Event Building Tracking Tracking Consumer Consumer
AGATA Crystal AGATA Crystal NARVAL Producer
Complementary detectors
NARVAL Producer
Complementary detectors
RUN GUI
30Si(70MeV)+12C reaction
RED 1785 1790 1795 1800 1805 1810 5 10 15 20 25 30 35 40 GREEN 1795 1800 1805 1810 1815 1820 5 10 15 20 25 30 35 40 BLUE 1808 1813 1818 1823 1828 1833 5 10 15 20 25 30 35 40
40K
1823 keV
40K
2333 keV
– (Similar to the 56Fe on 208Pb performed in 2001 with MARS)
Position of interactions in Dante 547 keV (197Au) 847 keV ( 56Fe) Dante+PSA 4.6 keV Original ~30 keV
Structure of the Doppler shift for the 847 keV peak as a function of the position in Dante 56Fe 197Au
Dante+PSA 2.6 keV Original ~10 keV
Optimized result: 3.2 keV Optimized result: 3.2 keV
Projection of γγ matrix Most intense channel:
138Sm
138Sm ground-state band (sum of gates)
Neutron drip-line Proton drip-line
Spectroscopy and lifetimes in the new region of deformation n-rich A~60, N~40 nuclei
n-rich nuclei
Lifetimes in neutron-rich Ca isotopes N=50 shell gap: lifetime, and excited states Quenching of the N=82 shell gap in n-rich nuclei
More than 20 LoI:
Highly Excited Collective Modes. Proton-rich mirror nuclei. Superdeformed states in A~40 proton-rich region. Order-Chaos transition in warm rotating nuclei. etc...
Evolution of collectivity and Dynamical Symmetries in the rare earths Mix-symmetry states Lifetimes in the region
(A.Maj, F.Azaiez, P.Napiórkowski)
to the region of the Giant Quadrupole Resonance (R.Nicolini)
(E.Sahin, M.Doncel, A.Görgen)
(J.J.Valiente-Dobón)