Low Energy Electromagnetic Physics - Geant4 - CERN
Low Energy Electromagnetic Physics - Geant4 - CERN
Low Energy Electromagnetic Physics - Geant4 - CERN
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
<strong>Low</strong> <strong>Energy</strong> <strong>Electromagnetic</strong> <strong>Physics</strong><br />
Maria Grazia Pia, INFN Genova<br />
on behalf of the <strong>Low</strong>E WG<br />
http://www.ge.infn.it/geant4/lowE/index.html<br />
<strong>Geant4</strong> Workshop and <strong>Geant4</strong> ∆ Review, <strong>CERN</strong>, October 2002<br />
Maria Grazia Pia, INFN Genova
The process in a nutshell<br />
We have and maintain a URD<br />
– Regular contacts with users<br />
We have a process for requirements<br />
management<br />
– But we would like to have a tool for it!<br />
We do analysis and design<br />
– We validate our designs against use cases<br />
We do design and code reviews<br />
– not enough, however…<br />
– main problem: geographical spread<br />
Unit, package integration, system tests<br />
+ validation (acceptance)<br />
– we do a lot… but we would like to do more<br />
– Limited by availability of resources for core<br />
testing<br />
– Need a more systematic approach and better<br />
toolsè Test & Analysis Project<br />
– Close collaboration with users<br />
Ample requirements traceability<br />
– Still improving it: added documentation<br />
and validation results as traceability items<br />
– in progress: traceability documentation<br />
from simple matrix to Rose model<br />
We regularly hold WG meetings to<br />
discuss and agree together our project<br />
planning (GDPM approach)<br />
We have a SPI process<br />
– With some spells of SPD sometimes…<br />
– Collaboration with Anaphe for a common<br />
(tailored) process<br />
We keep everything in CVS<br />
(not in our head…)<br />
– Code, designs, tests, documents etc.<br />
We maintain a web site<br />
– <strong>Low</strong>E, advanced examples, WG projects<br />
More details: see talk on Software Process in <strong>Physics</strong>, <strong>Geant4</strong> Review 2001<br />
Maria Grazia Pia, INFN Genova
Recent physics activities<br />
Electron processes<br />
– New parameterisations of LLNL data<br />
– Various bug fixes<br />
– Tests against NIST database (range)<br />
– Tests against Sandia database<br />
Photon processes<br />
– Rather stable<br />
– Tests of angular distributions in<br />
progress<br />
Polarisation<br />
– Improvement of Compton<br />
– γ conversion in progress<br />
– Contacts with experiments for<br />
common validation tests<br />
Auger effect<br />
– New<br />
Fluorescence<br />
– Small fixes and improvements while reimplementing<br />
in a design iteration<br />
– Test beam validation in collaboration with<br />
ESA Science Payload Division<br />
PIXE<br />
– Toy model<br />
– Established contacts for databases, plans for<br />
new model<br />
Protons, ions<br />
– Stable, minor improvements<br />
– Bragg peak tests in progress<br />
Antiprotons<br />
– Paper in progress, very close to submission<br />
Maria Grazia Pia, INFN Genova
Photons: mass attenuation coefficient<br />
Comparison against NIST data<br />
Tests by IST - Natl. Inst. for Cancer<br />
Research, Genova (F. Foppiano et al.)<br />
<strong>Low</strong>E accuracy ~ 1%<br />
E (%)<br />
UR 1.1<br />
18<br />
16<br />
14<br />
12<br />
10<br />
8<br />
6<br />
4<br />
2<br />
0<br />
-2<br />
-4<br />
-6<br />
-8<br />
-10<br />
-12<br />
-14<br />
-16<br />
-18<br />
E = (NIST-G4EMStandard)/NIST<br />
E = (NIST-G4<strong>Low</strong>En)/NIST<br />
0.01 0.1 1 10<br />
Photon <strong>Energy</strong> (MeV)<br />
Fe<br />
This test will be introduced into the Test & Analysis project<br />
for a systematic verification<br />
Also water, Pb<br />
Maria Grazia Pia, INFN Genova
µ /ρ (cm 2 /g) in water<br />
10<br />
1<br />
0.1<br />
Photon attenuation: <strong>Geant4</strong> vs. NIST data<br />
Test and validation by IST - Natl. Inst. for Cancer Research, Genova<br />
<strong>Geant4</strong> <strong>Low</strong>En<br />
NIST<br />
1000<br />
100<br />
100<br />
water Fe Pb<br />
10<br />
µ /ρ (cm 2 /g) in iron<br />
10<br />
1<br />
0.1<br />
UR 1.1<br />
<strong>Geant4</strong> <strong>Low</strong>En<br />
NIST<br />
µ/ρ (cm 2 / g in lead<br />
1<br />
0.1<br />
0.01<br />
<strong>Geant4</strong> <strong>Low</strong>En<br />
NIST<br />
0.01 0.1 1 10<br />
Photon <strong>Energy</strong> (MeV)<br />
0.01<br />
0.01 0.1 1 10<br />
Photon <strong>Energy</strong> (MeV)<br />
0.01 0.1 1<br />
Photon energy (MeV)<br />
Delta (%)<br />
16<br />
14<br />
12<br />
10<br />
8<br />
6<br />
4<br />
2<br />
0<br />
-2<br />
-4<br />
-6<br />
-8<br />
-10<br />
-12<br />
-14<br />
-16<br />
Delta = (NIST-G4EMStand) / NIST<br />
Delta = (NIST-G4<strong>Low</strong>En) / NIST<br />
0.01 0.1 1 10<br />
Photon <strong>Energy</strong> (MeV)<br />
E (%)<br />
18<br />
16<br />
14<br />
12<br />
10<br />
8<br />
6<br />
4<br />
2<br />
0<br />
-2<br />
-4<br />
-6<br />
-8<br />
-10<br />
-12<br />
-14<br />
-16<br />
-18<br />
• <strong>Low</strong> <strong>Energy</strong> EM<br />
• Standard EM<br />
w.r.t. NIST data<br />
E = (NIST-G4EMStandard)/NIST<br />
E = (NIST-G4<strong>Low</strong>En)/NIST<br />
accuracy within 1%<br />
0.01 0.1 1 10<br />
Photon <strong>Energy</strong> (MeV)<br />
E (%)<br />
10<br />
8<br />
6<br />
4<br />
2<br />
0<br />
-2<br />
-4<br />
-6<br />
-8<br />
-10<br />
E = (NIST - G4EM Standard)/NIST<br />
E = (NIST- G4<strong>Low</strong>En)/NIST<br />
0.01 0.1 1<br />
Photon <strong>Energy</strong> (MeV)<br />
Maria Grazia Pia, INFN Genova
Photons: angular distributions<br />
UR 1.1<br />
Maria Grazia Pia, INFN Genova<br />
Rayleigh scattering: <strong>Geant4</strong>-<strong>Low</strong>E and expected distribution<br />
(more work in progress)
Photons, evidence of shell effects<br />
UR 1.1<br />
Photon transmission, 1 µm Pb<br />
Photon transmission, 1 µm Al<br />
Maria Grazia Pia, INFN Genova
Electron Bremsstrahlung<br />
UR 1.1<br />
New parameterisations of<br />
EEDL data library<br />
– in response to problem reports<br />
from various users<br />
– precision is now ~ 1.5 %<br />
Plans<br />
– Systematic verification over Z<br />
and energy<br />
– Need Test & Analysis Project<br />
for automated verification<br />
Maria Grazia Pia, INFN Genova
Electron ionisation<br />
UR 1.1<br />
New parameterisations<br />
of EEDL data library<br />
– in response to problem<br />
reports from various users<br />
– precision is now better than<br />
5 % for ~ 50% of the shells,<br />
poorer for the 50% left<br />
Plans<br />
– Systematic verification over<br />
shell, Z and energy<br />
– Need Test & Analysis Project<br />
for automated verification<br />
(all shells, 99 elements!)<br />
Maria Grazia Pia, INFN Genova
Electrons: range<br />
UR 1.1<br />
Range in various simple and<br />
composite materials<br />
Compared to NIST database<br />
Al<br />
Also Be, Fe, Au, Pb, Ur, air,<br />
water, bone, muscle, soft tissue<br />
Testbed for<br />
Test&Analysis prototype<br />
Maria Grazia Pia, INFN Genova
Electrons: dE/dx<br />
UR 1.1<br />
Ionisation energy loss in<br />
various materials<br />
Compared to Sandia database<br />
More systematic verification<br />
planned (for publication)<br />
Maria Grazia Pia, INFN Genova<br />
Also Fe, Ur
Electrons, transmitted<br />
20 keV electrons, 0.32 and 1.04 µm Al<br />
UR 1.1<br />
Maria Grazia Pia, INFN Genova
UR 2.1<br />
Protons<br />
Stopping power<br />
Z dependence for various energies<br />
Ziegler and ICRU models Ziegler and ICRU, Fe Ziegler and ICRU, Si<br />
Straggling<br />
UR 2.5<br />
Nuclear stopping power<br />
Maria Grazia Pia, INFN Genova<br />
Bragg peak (with hadronic interactions)
Antiprotons<br />
UR 2.3<br />
New: comparison with another<br />
theoretical model<br />
– Non-linear calculation by Arista<br />
and Lifschitz<br />
Dashed<br />
– <strong>Geant4</strong> <strong>Low</strong>E proton<br />
Solid<br />
– <strong>Geant4</strong> <strong>Low</strong>E Quantal Harmonic<br />
Oscillator model<br />
Dotted-dashed<br />
– Calculation by Arista and Lifschitz<br />
Points<br />
– Data from ASACUSA<br />
Maria Grazia Pia, INFN Genova
Ions<br />
Deuterons<br />
UR 2.2<br />
Ar and C ions<br />
Maria Grazia Pia, INFN Genova
Polarisation<br />
x<br />
250 eV -100 GeV<br />
ξ φ<br />
hν<br />
hν<br />
ε A<br />
0 θ<br />
O α<br />
C<br />
Cross section:<br />
UR 4.1, D.1<br />
z<br />
d<br />
dΩ<br />
σ 1<br />
2<br />
=<br />
' ⎛<br />
ε||<br />
= ⎜Nî−<br />
⎝<br />
θ Polar angle<br />
φ Azimuthal angle<br />
ε Polarization vector<br />
2<br />
2 hν<br />
⎡hν0<br />
hν<br />
2<br />
r0 ⎢ + − 2sin θ cos<br />
2<br />
2 hν0<br />
⎣ hν<br />
hν0<br />
1<br />
N<br />
cosξ = sinθcosφ<br />
Scattered Photon Polarization<br />
'<br />
ε ⊥<br />
=<br />
⇒<br />
1<br />
N<br />
2<br />
sin θ sinφ<br />
cosφĵ−<br />
1<br />
N<br />
sinξ =<br />
⎤<br />
φ⎥<br />
⎦<br />
2 2<br />
1−sin<br />
θcos<br />
φ = N<br />
( cosθ<br />
ĵ − sin θsin<br />
φ kˆ ) sinβ<br />
⎞<br />
sinθ<br />
cosθ<br />
cosφkˆ<br />
⎟cosβ<br />
⎠<br />
<strong>Low</strong> <strong>Energy</strong><br />
Polarised Compton<br />
y<br />
100 keV<br />
1 MeV<br />
10 MeV<br />
small ϑ<br />
small ϑ<br />
More details: talk on<br />
small ϑ<br />
<strong>Geant4</strong> <strong>Low</strong> <strong>Energy</strong><br />
<strong>Electromagnetic</strong> <strong>Physics</strong><br />
large ϑ<br />
large ϑ<br />
large ϑ<br />
Maria Grazia Pia, INFN Genova<br />
Other polarised processes under development
Fluorescence<br />
Microscopic validation:<br />
against reference data<br />
UR 3.1<br />
Experimental validation:<br />
test beam data, in collaboration with<br />
ESA Science Payload Division<br />
Fe lines<br />
Spectrum from<br />
a Mars-simulant<br />
rock sample<br />
GaAs lines<br />
Scattered<br />
photons<br />
Maria Grazia Pia, INFN Genova
Auger effect<br />
UR 3.1<br />
New process,<br />
validation in progress<br />
Auger electron emission<br />
from various materials<br />
Sn, 3 keV photon beam,<br />
electron lines w.r.t. published<br />
experimental results<br />
Maria Grazia Pia, INFN Genova
Contribution from users<br />
Many valuable contributions to the validation of <strong>Low</strong>E<br />
physics from users all over the world<br />
– excellent relationship with our user community<br />
User comparisons with data usually involve the effect<br />
of several physics processes of the <strong>Low</strong>E package<br />
A small sample in the next slides<br />
– no time to show all!<br />
Maria Grazia Pia, INFN Genova
GEANT4 Workshop, 2002<br />
30 September – 4 October<br />
GEANT4 Medical Applications at LIP<br />
P. Rodrigues, A. Trindade, L.Peralta, J. Varela<br />
LIP – Lisbon<br />
Maria Grazia Pia, INFN Genova
Homogeneous Phantom<br />
P. Rodrigues, A. Trindade, L.Peralta, J. Varela, LIP<br />
• Simulation of photon beams produced by a Siemens<br />
Mevatron KD2 clinical linear accelerator<br />
• Phase-space distributions interface with GEANT4<br />
• Validation against experimental data: depth dose and<br />
profile curves<br />
Differences<br />
LIP – Lisbon<br />
10x10 cm 2<br />
15x15 cm 2<br />
10x10 cm 2 15x15 cm 2<br />
Maria Grazia Pia, INFN Genova
Electron Transport at <strong>Low</strong> Energies<br />
P. Rodrigues, A. Trindade, L.Peralta, J. Varela, LIP<br />
• Evaluation of electron range for different GEANT4 GEANT4 releases (<strong>Low</strong>+Std)<br />
Styrophoam<br />
Lead<br />
Maria Grazia Pia, INFN Genova
Dose Calculations with 12 12 C<br />
P. Rodrigues, A. Trindade, L.Peralta, J. Varela, LIP<br />
• Bragg peak localization calculated with GEANT4 (stopping powers<br />
from ICRU49 and Ziegler85) and GEANT3 in a water phantom<br />
• Comparison with GSI data<br />
Maria Grazia Pia, INFN Genova
<strong>Geant4</strong> low energy validation<br />
Jean-Francois Carrier, Louis Archambault, Rene Roy and Luc Beaulieu<br />
Service de radio-oncologie, Hotel-Dieu de Quebec, Quebec, Canada<br />
Departement de physique, Universite Laval, Quebec, Canada<br />
The following results will be published soon. They are part<br />
of a general <strong>Geant4</strong> low energy validation project.<br />
Maria Grazia Pia, INFN Genova
• Using <strong>Geant4</strong>, we calculated depth-dose curves for many<br />
different electron or photon sources:<br />
•Beams<br />
•monoenergetic beam<br />
•realistic clinical accelerator beam<br />
•Point sources<br />
•monoenergetic source<br />
•source with real nuclide energy spectra<br />
•and different irradiated media:<br />
•Homogeneous<br />
•water, Be, Mo or U<br />
•Heterogeneous<br />
•water/Al/lung/water<br />
•water/air/steel/air/water<br />
Maria Grazia Pia, INFN Genova<br />
Jean-Francois Carrier, Louis Archambault, Rene Roy and Luc Beaulieu
Uranium irradiated by electron beam<br />
Jean-Francois Carrier, Louis Archambault, Rene Roy and Luc Beaulieu<br />
Fig 1. Depth-dose curve for a semi-infinite uranium slab irradiated by a 0.5<br />
MeV broad parallel electron beam<br />
Maria Grazia Pia, INFN Genova<br />
1 Chibani O and Li X A, Med. Phys. 29 (5), May 2002
Multi-slab medium irradiated by photons<br />
Jean-Francois Carrier, Louis Archambault, Rene Roy and Luc Beaulieu<br />
Fig 2. Depth-dose curve for a multi-slab medium irradiated by a 18 MV<br />
realistic clinical accelerator photon beam<br />
2 Rogers D W O and Mohan<br />
R,http://www.irs.inms.nrc.ca/inms/irs/papers/iccr00/iccr00.html<br />
Maria Grazia Pia, INFN Genova
Water phantom irradiated by clinac beam<br />
Jean-Francois Carrier, Louis Archambault, Rene Roy and Luc Beaulieu<br />
Fig 3. Relative dose distribution for a water phantom irradiated by a 6<br />
MeV Clinac 2100C electron beam<br />
Maria Grazia Pia, INFN Genova<br />
3 Ding G X and Rogers D W O<br />
http://gold.sao.nrc.ca/inms/papers/PIRS439/pirs439.html
Ions<br />
Independent validation at<br />
Univ. of Linz (H. Paul et al.)<br />
<strong>Geant4</strong>-<strong>Low</strong>E reproduces the right<br />
side of the distribution precisely,<br />
but about 10-20% discrepancy is<br />
observed at lower energies<br />
Maria Grazia Pia, INFN Genova
Dose distribution: TG 43 protocol,<br />
experimental data (S. Paolo Hospital, Savona), G4-<strong>Low</strong>E<br />
o Protocol<br />
ê Data (SV)<br />
m G4-<strong>Low</strong>E<br />
Maria Grazia Pia, INFN Genova<br />
S. Guatelli’s thesis
Application<br />
Cosmic rays,<br />
jovian electrons<br />
Solar X-rays, e, p<br />
and more!<br />
Courtesy SOHO EIT<br />
Maria Grazia Pia, INFN Genova<br />
Courtesy of S. Magni, Borexino<br />
Not only<br />
“space and medical”!
Team work!<br />
<strong>Geant4</strong> <strong>Low</strong> <strong>Energy</strong> <strong>Electromagnetic</strong> Working Group<br />
+<br />
users all over the world<br />
The validation plots in this presentation<br />
have been contributed by<br />
19 people from 9 countries<br />
Thanks to all!<br />
Students<br />
Jean-Francois Carrier<br />
Stephane Chauvie<br />
Elena Guardincerri<br />
Susanna Guatelli<br />
Alfonso Mantero<br />
Pedro Rodrigues<br />
Andreia Trindade<br />
Matteo Tropeano<br />
Maria Grazia Pia, INFN Genova
Further physics improvements and extensions<br />
Various projects in progress<br />
– all motivated by requirements in the URD<br />
Some examples in the following slides<br />
– no time to show all!<br />
Maria Grazia Pia, INFN Genova
Bremsstrahlung Models<br />
UR A.5<br />
• Current bremstrahlung polar angle generation scheme is independent<br />
of both atomic number, Z, and emitted photon momentum, k<br />
• Does not account variations due to the screening of the nucleus by<br />
the atomic electrons<br />
• At generator level, for 50 keV incident electrons with k/T=0.7 in Ag<br />
New model (2BN) to be<br />
implemented by LIP group<br />
Maria Grazia Pia, INFN Genova
Polarisation<br />
UR 1.4, 4.1<br />
theory<br />
500 million events<br />
simulation<br />
Polarisation of a non-polarised photon<br />
beam, simulation and theory<br />
Maria Grazia Pia, INFN Genova<br />
Ratio between intensity with perpendicular and parallel polarisation<br />
vector w.r.t. scattering plane, linearly polarised photons
Ongoing significant effort in OOAD<br />
Maria Grazia Pia, INFN Genova
Other activities in the WG<br />
Advanced examples<br />
Simulation + analysis in a distributed computing environment<br />
Test & Analysis<br />
Technology transfer<br />
Training<br />
Maria Grazia Pia, INFN Genova
Technology transfer<br />
Particle physics<br />
software aids space<br />
and medicine<br />
M.G. Pia and J. Knobloch<br />
<strong>Geant4</strong> is a showcase example of<br />
technology transfer from particle<br />
physics to other fields such as<br />
space and medical science […].<br />
<strong>CERN</strong> Courier, June 2002<br />
Maria Grazia Pia, INFN Genova
Talks<br />
since last<br />
workshop<br />
in WG web<br />
1. The <strong>Geant4</strong> Toolkit: simulation capabilities and application results<br />
M.G. Pia et al., 8th Topical Seminar on Innovative Particle and Radiation Detectors, Siena, 2002<br />
2. <strong>Geant4</strong>: a powerful tool for medical physics<br />
E.Lamanna et al., 8th Topical Seminar on Innovative Particle and Radiation Detectors, Siena, 2002<br />
3. Dose calculation for radiotherapic treatment on a distributed computing environment<br />
S.Chauvie et al., 8th Topical Seminar on Innovative Particle and Radiation Detectors, Siena, 2002<br />
4. Parallel <strong>Geant4</strong> simulation in medical and space science applications<br />
J. Moscicki et al., 8th Topical Seminar on Innovative Particle and Radiation Detectors, Siena, 2002<br />
5. Simulation and analysis for astroparticle experiments<br />
A. Howard et al., 8th Topical Seminar on Innovative Particle and Radiation Detectors, Siena, 2002<br />
6. Leipzig applicators Montecarlo simulations: results and comparison with experimental and manufacturer's data<br />
M. Tropeano et al., 21st ESTRO Meeting, Prague, 2002<br />
7. Tools for simulation and analysis<br />
A. Pfeiffer and M.G. Pia (for the <strong>Geant4</strong> and Anaphe Collaborations), ICHEP02, Amsterdam, 2002<br />
8. The <strong>Geant4</strong> Simulation Toolkit and Its <strong>Low</strong> <strong>Energy</strong> <strong>Electromagnetic</strong> <strong>Physics</strong> Package<br />
S.Chauvie et al., 44th Annual Meeting of the American Ass. of Physicists in Medicine, Montreal, 2002<br />
9. The <strong>Geant4</strong> Toolkit: Overview<br />
M. G. Pia, Invited lecture at the MCNEG Workshop, Stoke-on-Trent, UK, 2002<br />
10. Medical applications of the <strong>Geant4</strong> Simulation Toolkit<br />
M. G. Pia, Invited lecture at the MCNEG Workshop, Stoke-on-Trent, UK, 2002<br />
11. Simulation software: applications and results in the bio-medical domain<br />
M. G. Pia et al., VII International Conference on Advanced Technologies and Particle <strong>Physics</strong>, Como, 2001<br />
12. From HEP computing to bio-medical research and vice-versa: technology transfer and application results<br />
M. G. Pia et al., Plenary talk at CHEP 2001, Beijing, China, 2001<br />
13. Architecture of Collaborating Frameworks<br />
A.Pfeiffer et al., CHEP2001, Beijing, China, 2001<br />
14. Simulation For Astroparticle Experiments And Planetary Explorations<br />
A.Brunengo (for the <strong>Geant4</strong> <strong>Low</strong> <strong>Energy</strong> <strong>Electromagnetic</strong> Group), CHEP2001, Beijing, China, 2001<br />
15. <strong>Geant4</strong> <strong>Low</strong> <strong>Energy</strong> <strong>Electromagnetic</strong> <strong>Physics</strong><br />
M. G. Pia (for the <strong>Geant4</strong> <strong>Low</strong> <strong>Energy</strong> <strong>Electromagnetic</strong> Group), CHEP2001, Beijing, China, 2001<br />
16. The GEANT4 simulation toolkit<br />
G. Santin, Monte Carlo Workshop for Nuclear Medicine applications, July 2001<br />
17. <strong>Geant4</strong>: simulation capabilities and application results<br />
M.G. Pia (for the <strong>Geant4</strong> Collaboration), EPS-HEP Conference, Budapest, July 2001<br />
Maria Grazia Pia, INFN Genova
Training<br />
National School on Detector Technologies, Torino, Feb. 2002<br />
– Lectures + “<strong>Geant4</strong> through an example”<br />
<strong>Geant4</strong> & Anaphe mini-workshop, Gran Sasso Lab, July 2002<br />
– Tutorials + “<strong>Geant4</strong> through an example” +demo<br />
<strong>Geant4</strong> User Workshop, Salamanca, July 2002<br />
– Lectures + exercises<br />
<strong>Geant4</strong> & Anaphe mini-workshop, INFN-LNS Lab, November 2002<br />
– Tutorials + + “<strong>Geant4</strong> through an example” +demo “<strong>Geant4</strong> through an<br />
example” +demo<br />
User-centric approach:<br />
– Introduction to “advanced” software engineering concepts<br />
– Complete (from the user’s view) training: simulation + analysis<br />
Maria Grazia Pia, INFN Genova
Resources<br />
New collaborators:<br />
– Pablo Cirrone (INFN-LNS)<br />
– Luis Peralta, Pedro Rodrigues, Andreia Trindade (LIP, Lisbon)<br />
– Interest expressed by small group at INFN-Gran Sasso Lab<br />
Status on 1 September 2002<br />
Maria Grazia Pia, INFN Genova
We do a lot of work<br />
– and we do our best to do it well…<br />
– a rigorous software process, continuous SPI<br />
Conclusions<br />
– very effective team-work<br />
work, several brilliant and motivated young collaborators<br />
We have plenty of interesting physics results in a new (and difficult)<br />
simulation domain<br />
– significant progress in the last year in a few problematic areas<br />
– don’t forget in what status we inherited the package, when the WG was created!<br />
A huge user community worldwide<br />
– excellent, constructive relationship between users and developers<br />
– more support for our activities outside the Collaboration than inside<br />
Many projects in the WG, not only physics<br />
– Testing system, analysis, advanced examples, general electromagnetic OOAD,<br />
distributed computing, technology transfer<br />
More information in http://www.ge<br />
ge.infn.it/geant4/<br />
.it/geant4/lowE<br />
Maria Grazia Pia, INFN Genova