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1. Status of GRETINA
2. Status of GRETINA
5. GRETINA - People Contractor Project Manager: I-Yang Lee (LBNL)?
GRETINA Advisory Committee (GAC):
Con Beausang (U. of Richmond)?
Doug Cline (U. of Rochester)?
Thomas Glasmacher (MSU / NSCL)?
Kim Lister (ANL)?
Augusto Macchiavelli (LBNL)
David Radford (ORNL) (Chair)?
Mark Riley (Florida State U.)?
Demetrios Sarantites (Washington U.)?
Kai Vetter (LLNL)?
Working Groups and chairs
Physics M. A. Riley (FSU)?
Detectors A. O. Macchiavelli (LBNL)?
Electronics D. C. Radford (ORNL)?
Software M. Cromaz (LBNL)?
Aux. Detectors D.G. Sarantites (WUSTL)?
7. First Quadruple Cluster (Q1)?
8. Second Quadruple Cluster (Q2)?
10. Electronics
11. Computing System
13. Examples of calculated signals: Sensitivity to position
14. Current algorithm is a hybrid: AGS + SQP
Pair-wise Adaptive Grid Search
~200,000 two-par. least-squares fits per segment (for energies)? in ~2 ms
Non-linear Least-Squares (a.k.a. SQP)?
Have also been developing Singular Value Decomposition
Collaboration with Tech-X Corp., funded under DOE SBIR
Developed SVD + SQP hybrid algorithm
- SVD on a coarse grid, with 250 eigenvalues
- Localize interaction regions
- Estimate number of interactions in each segment
Approx. 25% faster, but slightly poorer fits; further work planned
Also demonstrated speed-up of SVD algorithm by factor 30 to 40 using Graphics Processing Units (GPUs) rather than CPUs.
CPU time required : AGS ~ O(500n)?
SQP ~ O(n + ?n2)? for n interactions
SVD ~ O(n)?
Signal Decomposition Algorithm
15. Status of Signal Decomposition Algorithm
Three orders of magnitude improvement in CPU time; now meets timing requirements
Developed new optimized, irregular grid for the basis signals
Developed method to accurately correct calculated signals for preamplifier response and for two types of cross talk
Incorporated fitting of signal start time t0
Much improved fits (?2 values)?
Can handle any number of hit detector segments, each with up to two interactions
Although some work remains to be done, we have demonstrated that the problem of signal decomposition for GRETINA is solved
18. Collimated Cs-source test
19. Scanning-table coincident-data test
20. Workshop in Oct 2007, organized by the GAC
Plan for optimizing physics impact of GRETINA following completion in March 2011
Participation and presentation by Prof. Shimoura, U. of Tokyo; expressed interest in hosting GRETINA at RIKEN
Report prepared by GAC, submitted to DOE
Unanimous agreement on a plan for the first physics campaigns
Commissioning runs at LBNL, starting March 2001, coupled to BGS
Then rotate to other national laboratories, ~ 6 month campaigns
Suggested sequence for the first cycle:
MSU - NSCL
ORNL - HRIBF
ANL - ATLAS
“We look forward to further discussions with our Japanese colleagues and are excited about the possibility of future collaborations.”
Unique opportunities at RIKEN: Beams, auxiliary instruments, expertise
Siting
21.
Construction is proceeding, on schedule, on budget
Received CD2B / 3B approval Oct 2007
Signal decomposition problem is solved
Scheduled completion date: 2 March 2011 (Wed)?
We have proposed a plan for the first round of physics campaigns
Next stage: Full 4? steradians
GRETA received strong community support in LRP
“… construction of GRETA should begin upon successful completion of GRETINA” Summary
22. LBNL:
I-Yang Lee
Overall project manager and source of all wisdom!
A. Machiavelli, M. Cromaz, P. Fallon, M. Descovich, J. Pavan, many others
Detectors, DAQ, in-beam data analysis, simulations, electric field calc'ns, etc.
Sergio Zimmermann, John Joseph, Carl Lionberger, many others
Electronics, engineering, computing, etc.
GRETINA Advisory Committee and Working Group Leaders
Endless proposal writing, review preparation, working group meetings, conference calls, ...
John Anderson (ANL)?
Trigger system
Karin Lagergren (ORNL / UTK)?
Signal calculation code in C, Optimized pseudo-cylindrical grid
Tech-X Corp, especially Isidoros Doxas
SVD development
23. Backup Slides
25. In-Beam test at LBNL
26. In-Beam test at MSU
27. ORNL Installation
28. Cross-talk Differential cross talk arises from capacitive coupling between the inputs to the preamplifiers (some due to physical capacitance of the detector)
Can be modelled well in SPICE, but needs to be carefully characterized in reality
29. Fitting to Extract Cross-Talk Parameters
30. Why is it hard?
31. Comparison – Old Basis and Code vs. New
34. Singular Value Decomposition
35. Singular Value Decomposition
36. Singular Value Decomposition
37. 1? ? 4? coverage, 28 ? 120 detectors
38. How do extreme proton-to-neutron asymmetries affect nuclear properties, such as shell structure and collectivity?
What are the properties of nuclei at the limits of mass and charge?
What are the properties of nuclei at the limits of angular momentum?
Nuclear astrophysics, fundamental interactions and rare processes
39. Gamma-Ray Tracking
“… The construction of GRETA should begin upon successful completion of GRETINA. This gamma-ray energy tracking array will enable full exploitation of compelling science opportunities in nuclear structure, nuclear astrophysics, and weak interactions.” GRETA in the 2007 NSAC Long Range Plan
40. GRETA Cost and Schedule