Minutes of the E89044 group meeting, July 21, 1999, at Jefferson Lab


List of participants:
Konrad Aniol
Zhengwei Chai
George Chang
Salvatore Frullani
Shalev Gilad
Sabine Jeschonnek
Jim Kelly
Michael Kuss
John LeRose
Richard Lindgren
Dimitri Margaziotis
Charles Perdrisat
Vina Punjabi
Marat Rvachev
Arun Saha
Adam Sarty
Jeffrey Templon
Luminita Todor
Larry Weinstein

Adam Sarty and Jeff Templon ...
... spoke about the gory details in unfolding the radiative tail. The talk was identical (as requested) to the one given in the June 25, 1999 JLab User Group Workshop. Please check the transparancies of Adams and Jeffs talks and their preprint nucl-ex/9906008 for detailed information. Main messages were that going to high Emiss one has to be careful which other kinematical regions may radiate into the region of interest, and eventually also span those region to be able to unfold the effects. Also, the standard two-dimensional unfolding seems not to work all the time, and one may have to go up to 5 or 6 dimensions. Jeff pointed out that not the data have to be "corrected" but the theory has to contain radiative effects. Alternatively, one can take the theory and radiate it till the result fits the experimental data.

George Chang ...
... presented GEANT simulations for collimator punch-through for extended targets. The studies are motivated by the fact that punch-through may pollute the higher Emiss region with additional counts. He showed that the electrons deposit almost all their energy and thus don't cause problems. However, protons loose less energy and moreover, just grazing the collimator, may fill the entire range between the nominal energy and the maximum energy loss. He also showed simulations that showed that those events may be identified by using selected cuts. Transparancies will follow.

Luminita Todor ...
... demonstrated for the E93050 (VCS) experiment that those cuts to reduce the background from punch-through really work. She favors two-dimensional cuts which were able to reduce the background dramatically. Transparancies will follow.

Nilanga Liyanage ...
... presented the run plan for optics studies at 4 GeV. He pointed out that it is uncertain when to run because it needs 4.8 GeV beam energy. However, the optics should not to be too different from at 3.5 GeV, so the current matrizes are good for online analysis and it is an option to perform the studies even during or after the experiment. Arun showed that one possible slot is February 2000 when we are running at 4.75 GeV. Eventually the spectrometer constant may be different, which will show up in shifted missing mass peaks.

Konrad Aniol ...
... spoke about luminosity monitoring. A discussion on this topic you can find here and there.

Discussion: