Group Meeting at Mainz 26th April 2012
Y. Ma
: Future Plan
Meeting minutes
Christine
:
Chiller don't arrive to -25°C due to the compressor
It is the possibility to buy a new one or a chiller on exposition for half price.
Vacuum workshop find a chiller which arrive to -40°C.
Pascal
:
Flash ADC read by the Data acquisition system and merge on the root file.
External trigger for a cosmic muon is under construction.
Iris
:
Macro for the pion, muon production in the Himster, 1M event in production.
Dexu:
:
Start
GiBUU
code on the Himster
two kaon decay are not back to back produce. Dexu try to understand this.
Cristina
:
Background signal studies (
BesIII
on e+e- collider)
Install simulation in Himster
Yue Ask about the resolution difference between PANDA and
BesIII
?
Studies make by Dmitry on the Form factors show is better determine for PANDA (statistical error low than
BesIII
).
Only the Luminosity make the difference.
Keith
:
Preparing a proposal on strange Barion, Omega(3s) and sigma(2s).
Analysis on the EMC effect in Deuteron.
Keith explain the EMC effect and the difference between the strong and the weak interaction.
Dmitry
:
install new macro in Himster for studie radiative correction e+e-
Put this radiative correction on the event generator is the goal of this studies.
Mamen
:
Waiting for the correction.
Manuel
:
preparing the code to calculate the pbarp going to pi+pi-
Cross section is need for the determination of the suppression factor.
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Topic revision:
2012-05-03,
RobertoPerezBenito
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