A 8 GeV electrons beam (composed by 1.1e+4 particles) impinge on a <111> oriented tungsten crystal of 1mm thickness.
Particles at the exit of the crystal
For display reason a cut is apply on px and py value (abs(px&&py)<20 MeV/c).
First case a transverse distribution of sigma=1mm is added to the particles transverse distribution
Electrons phase space at the exit of the crystal
Photons phase space at the exit of the crystal
Positrons phase space at the exit of the crystal
Second case a transverse distribution of sigma=2.5mm is added to the particles transverse distribution
Electrons phase space at the exit of the crystal
Photons phase space at the exit of the crystal
Positrons phase space at the exit of the crystal
Particles at the exit of the amorphous
The photons at the exit of the crystal is use to impinge on 8mm amorphous tungsten
(for 2.5mm rms value)
After the amorphous px,py and pz are defined by the following
Photons phase space at the exit of the amorphous
Electrons phase space at the exit of the amorphous
Positrons phase space at the exit of the amorphous
A 10GeV mono energetic electron beam (with au gaussian distribution in x and y
-in root : gRandom->Gaus(0,2.5e-3)/sqrt(2.)-) impinging on 0.1 cm amorphous tungsten produced gamma with this phase space (yield=#gamma/#e-=138966/50000~2.78)
Gamma energy distribution
X distribution
Y distribution
Those gamma are using to produce positron by impinging on 0.8 cm of amorphous tungsten
(distance between the two amophous target is 2m).
Positron phase space distribution(yield=#positron/#electron=143443/50000 ~2.86)
(initial particles impinging on the crystal = 5000 macro e-)
Photons energy spectrum
Positrons phase space after the amorphous target
Energy (no energy cut)
Energy (below 400 MeV):
X:
Y:
Px:
Py:
Positrons spatial distribution after capture section (AMD)
AMD caracteristics
AMD length: 50 cm
B = B0/(1+alpha*z) with B0=6 Tesla and alpha=22/m
Transverse phase space of the positrons from the target.
We apply a cut in the radius, r<20mm corresponding to the aperture of the
pre-accelerating cavities.
In blue after the amorphous and in red after the AMD
Angle distribution
Electron beam energy : 5GeV
Crystal thickness : 0.14 cm
Distance between amorphous and amorphous : 2m
Amorphous thickness : 1 cm
(initial particles impinging on the crystal = 6000 macro e-)
Photons energy spectrum
Positrons phase space after the amorphous target
Energy (no energy cut):
Energy (below 200 MeV):
X:
Y:
Px:
Py:
Positrons spatial distribution after capture section (AMD)
AMD caracteristics
AMD length: 50 cm
B = B0/(1+alpha*z) with B0=6 Tesla and alpha=22/m
Transverse phase space of the positrons from the target.
We apply a cut in the radius, r<20mm corresponding to the aperture of the
pre-accelerating cavities.
In blue after the amorphous and in red after the AMD
Angle distribution
EXTRA …
(thanks to Laurent Garnier Qt implementation see http://users.lal.in2p3.fr/garnier/G4QtTutorial.html#interface)
Tungsten target of 1×X0 = 3.5 mm (Z=74, ρ = 19.3 g/cm3)
Positron Yield = Ne+/Ne- ~ 15 %
Energy deposited in the tungsten target per initial incident electron ~ 14 MeV
Mean positron polarisation : Sz ~ 30 %
Modification of the positron yield, positron polarisation considering differents target thickness and
two differents inital electron energy (50 MeV and 80 MeV)
Initial electron energy 50 MeV
Positron Yield versus target thickness (different energy selection are shown)
Mean positron energy versus target thickness (different energy selection are shown)
Positron polarisation versus target thickness (different energy selection are shown)
Initial electron energy 80 MeV
Positron yield versus target thickness (different energy selection are shown)
Mean positron energy versus target thickness (different energy selection are shown)
Positron polarisation versus target thickness (different energy selection are shown)
J’ai cherché désespérément ces informations pour cross checker ma simulation Geant4:
Nombre particules secondaires créées et leur pertes d’énergie dans la cible.
Taille de la cible de Tungsten(G4_W densité 19.3 g/cm3) 3.5mm (*20cm*20cm)
Uniquement les processus EM pris en compte pas de flag hadronique i.e pas de création de neutrons
1) Run 10000 gamma de 100 MeV
Gamma
Mean Number per Event : 3.127400
Mean Kinetic Energy : 22.142556 MeV +- 37.196105 MeV
Energy deposited in the target per incident particles 0.133872 MeV
Electrons
Mean Number per Event : 0.406800
Mean Kinetic Energy : 30.026098 MeV +- 24.451613 MeV
Energy deposited in the target per incident particles 3.404414 MeV
Positron
Mean Number per Event : 0.366600
Mean Kinetic Energy : 33.335758 MeV +- 23.974807 MeV
Energy deposited in the target per incident particles 2.190985 MeV
Soit 5.73 MeV déposée dans la cible de tungstène par gamma incident
2) Run 10000 e- de 100 MeV
Gamma
Mean Number per Event : 6.670000
Mean Kinetic Energy : 7.301013 MeV +- 13.162204 MeV
Energy deposited in the target per incident particles 0.345439 MeV
Electrons
Mean Number per Event : 1.068500
Mean Kinetic Energy : 31.868788 MeV +- 24.521092 MeV
Mean Polarization :0.000000 +- 0.000000
Energy deposited in the target per incident particles 12.372011 MeV
Positron
Mean Number per Event : 0.183000
Mean Kinetic Energy : 14.930346 MeV +- 13.545201 MeV
Energy deposited in the target per incident particles 1.234059 MeV
Soit 14 MeV déposée dans la cible de tungstène par e- incident
Improved 2mrad crossing angle layout for the International Linear Collider
Philip Bambade, S. Cavalier, O. Dadoun (Orsay, LAL) , D.A.K. Angal-Kalinin (Daresbury) , Robert Barrie Appleby, D. Toprek (Manchester U.) . PAC07-THPMN077, Jun 2007.
In the Proceedings of Particle Accelerator Conference (PAC 07), Albuquerque, New Mexico, 25-29 Jun 2007, pp 2883
GUINEA PIG++ : An Upgraded Version of the Linear Collider Beam Beam Interaction Simulation Code GUINEA PIG
D. Schulte (CERN) , M. Alabau (Valencia U., IFIC) , Philip Bambade, O. Dadoun, G. Le Meur, C. Rimbault, F. Touze (Orsay, LAL) . PAC07-THPMN010, Jun 2007.
In the Proceedings of Particle Accelerator Conference (PAC 07), Albuquerque, New Mexico, 25-29 Jun 2007, pp 2728.
Backscattering of Secondary Particles into the ILC Detectors from Beam Losses Along the Extraction Lines
Philip Bambade, O. Dadoun (Orsay, LAL) . PAC07-THPMN009, Jun 2007.In the Proceedings of Particle Accelerator Conference (PAC 07), Albuquerque, New Mexico, 25-29 Jun 2007, pp 2725.
Technical Challenges for Head On Collisions and Extraction at the ILC
O. Delferriere et al. PAC07-THPMN005, Jun 2007.
In the Proceedings of Particle Accelerator Conference (PAC 07), Albuquerque, New Mexico, 25-29 Jun 2007, pp 2716
Design of the Beam Delivery System for the International Linear Collider
A. Seryi et al. FERMILAB-CONF-07-473, SLAC-PUB-12743, Aug 14, 2007. 3pp.
Presented at Particle Accelerator Conference (PAC 07), Albuquerque, New Mexico, 25-29 Jun 2007.
Published in *Albuquerque 2007, Particle accelerator* 1985-1987
Evaluation of luminosity reduction in the ILC head-on scheme from parasitic collisions
J. Brossard, P. Bambade, O. Dadoun, T. Derrien (Orsay, LAL) , M.C. Alabau-Pons (Orsay, LAL and Valencia U.) , O. Napoly, J. Payet (Saclay) , D. Angal-Kalinin (Daresbury) . EUROTEV-REPORT-2007-052, Jul 2007. 4pp.
Prepared for Particle Accelerator Conference (PAC 07), Albuquerque, New Mexico, 25-29 Jun 2007.
Technical challenges for head-on collisions and extraction at the ILC
O. Napoly et al. SLAC-PUB-12744, EUROTEV-REPORT-2007-043, Jun 2007. 3pp.
Prepared for Particle Accelerator Conference (PAC 07), Albuquerque, New Mexico, 25-29 Jun 2007.
Improved 2-mrad crossing angle layout for the International Linear Collider.
R. Appleby, D. Toprek (Manchester U. & Cockcroft Inst. Accel. Sci. Tech.) , D. Angal-Kalinin (Cockcroft Inst. Accel. Sci. Tech.) , P. Bambade, S. Cavalier, O. Dadoun (Orsay, LAL) . EUROTEV-REPORT-2007-022, Jun 2007. 3pp.
Prepared for Particle Accelerator Conference (PAC 07), Albuquerque, New Mexico, 25-29 Jun 2007.
Published in *Albuquerque 2007, Particle accelerator* 2883-2885
BDSIM: Beamline simulation toolkit based on GEANT4.
I. Agapov, J. Carter, G.A. Blair (Royal Holloway, U. of London) , O. Dadoun (Orsay, LAL) . EUROTEV-REPORT-2006-035, 2006. 3pp.
Prepared for European Particle Accelerator Conference (EPAC 06), Edinburgh, Scotland, 26-30 Jun 2006.
Response to the critics of Borexino result in »A New experimental limit for the stability of the electron » by H.V. Klapdor-Kleingrothaus, I.V. Krivosheina and I.V. Titkov
By Borexino Collaboration (H.O. Back et al.). Mar 2007. 5pp.
e-Print: hep-ex/0703044
BDSIM: Beamline simulation toolkit based on GEANT4.
I. Agapov, J. Carter, G.A. Blair (Royal Holloway, U. of London) , O. Dadoun (Orsay, LAL) . EUROTEV-REPORT-2006-035, 2006. 3pp.
Prepared for European Particle Accelerator Conference (EPAC 06), Edinburgh, Scotland, 26-30 Jun 2006.
Published in *Edinburgh 2006, EPAC* 2209-2211
The BDSIM toolkit.
I. Agapov, G.A. Blair, J. Carter (Royal Holloway, U. of London) , O. Dadoun (Orsay, LAL) . EUROTEV-REPORT-2006-014, Mar 2006. 33pp.
DESY Document Server
Design of an interaction region with head-on collisions for the ILC.
R. Appleby et al. SLAC-PUB-11950, LAL-RT-06-09, EUROTEV-REPORT-2006-083, Jun 2006. 4pp.
Presented at European Particle Accelerator Conference (EPAC 06), Edinburgh, Scotland, 26-30 Jun 2006.
e-Print Archive: physics/0609248
Optimization of the e- e- option for the ILC.
M. Alabau Pons, P. Bambade, O. Dadoun (Orsay, LAL) , R. Appleby (Manchester U.) , A. Faus-Golfe (Valencia U., IFIC) . LAL-RT-06-08, EUROTEV-REPORT-2006-067, CARE-ELAN-2006-007, Jun 2006. 4pp.
e-Print Archive: physics/0609043
Benchmarking of Tracking Codes (BDSIM/DIMAD) using the ILC Extraction Lines.
R. Appleby (Manchester U.) , P. Bambade, O. Dadoun (Orsay, LAL) , A. Ferrari (Uppsala U.) . LAL-RT-06-06, EUROTEV-REPORT-2006-038, Jun 2006. 4pp.
Contributed to European Particle Accelerator Conference (EPAC 06), Edinburgh, Scotland, 26-30 Jun 2006.
e-Print Archive: physics/0607165
Particle tracking in the ILC extraction lines with DIMAD and BDSIM.
R. Appleby (Manchester U.) , P. Bambade, O. Dadoun (Orsay, LAL) , A. Ferrari (Uppsala U.) . LAL-RT-06-05, EUROTEV-REPORT-2005-026, Jun 2006. 11pp.
e-Print Archive: physics/0607163
Design of an Interaction Region with Head-On Collisions for the ILC.
J. Payet et al. SLAC-PUB-11950, Jul 12, 2006. 4pp.
Presented at European Particle Accelerator Conference (EPAC 06), Edinburgh, Scotland, 26-30 Jun 2006.
The 2mrad Crossing Angle Interaction Region and Extraction Line.
R. Appleby et al. SLAC-PUB-11952, Jul 12, 2006. 4pp.
Presented at European Particle Accelerator Conference (EPAC 06), Edinburgh, Scotland, 26-30 Jun 2006.
ATF2 Proposal Vol.2.
B.I. Grishanov et al.. DESY-06-001, CERN-AB-2006-004, ILC-ASIA-2005-26,
JAI-2006-001, KEK-REPORT-2005-9, SLAC-R-796, UT-ICEPP-05-04, Feb 2006. 43pp.
PHENYLXYLYLETHANE (PXE): a high-density, high-flashpoint organic liquid scintillator for applications in low-energy particle and astrophysics experiments.
By Borexino Collaboration (H.O. Back et al.). MPIK-2003-059, Aug 2004. 45pp.
Submitted to Nucl.Instrum.Meth.A
e-Print Archive: physics/0408032
New experimental limits on violations of the pauli exclusion principle obtained with the BOREXINO Counting Test Facility.
By Borexino Collaboration (H.O. Back et al.). Jun 2004. 10pp.
Published in Eur.Phys.J.C37:421-431,2004
e-Print Archive: hep-ph/0406252
White paper report on using nuclear reactors to search for a value of theta(13).
K. Anderson et al. FERMILAB-PUB-04-180, Jan 2004. 167pp.
e-Print Archive: hep-ex/0402041
New experimental limits on heavy neutrino mixing in B-8 decay obtained with the BOREXINO Counting Test Facility.
Published in JETP Lett.78:261-266,2003, Pisma Zh.Eksp.Teor.Fiz.78:707-712,200300
New limits on nucleon decays into invisible channels with the BOREXINO Counting Test Facility.
By Borexino Collaboration (H.O. Back et al.). Feb 2003. 22pp.
Published in Phys.Lett.B563:23-34,2003
e-Print Archive: hep-ex/0302002
Study of the neutrino electromagnetic properties with prototype of borexino detector.
H.O. Back et al. JINR-E1-2002-29, Apr 2002. 17pp.
BOREXINO.
By Borexino Collaboration (G. Ranucci et al.). Jul 2001.
Prepared for NO-VE International Workshop on Neutrino Oscillations in Venice, Venice, Italy, 24-26 Jul 2001.
Published in *Venice 2001, Neutrino oscillations* 105-116 Also in *Tokyo 2000, Low energy solar neutrino detection*47-56
Search for electron decay mode e –> gamma + nu with prototype of BOREXINO detector.H.O. Back et al.. JINR-E1-2002-30, 2002. 19pp.
Published in Phys.Lett.B525:29-40,2002
Measurements of extremely low radioactivity levels in BOREXINO.
By BOREXINO Collaboration (C. Arpesella et al.). Sep 2001. 27pp.
Published in Astropart.Phys.18:1-25,2002
e-Print Archive: hep-ex/0109031
Borexino est l’expérience grâce à laquelle la « détection en temps réel » des neutrinos solaires de la raie de 7Be à 862 keV se fois. Rappelons que toutes les expériences de neutrinos solaires menées jusqu’à présent, n’offraient pas la possibilité d’effectuer conjointement une mesure du taux de neutrinos de basse énergie et une étude de sa variation temporelle. Qui plus est, le taux journalier attendu de neutrinos du 7Be est élevé, assurant ainsi une grande statistique : on attend environ 45 événements par jour dans le cadre du Modèle Standard du Soleil, à 12 événements par jour dans le cas d’une conversion complète de neutrinos.
L’expérience Borexino, ainsi que son prototype CTF, se situent au LNGS (Gran Sasso INFN Italie) dans le Hall C du laboratoire souterrain. J’ai participé durant mes années de thèse à l’implantation de l’électronique, au programme d’acquisition et j’ai travaillé sur la « Mesure des neutrinos de réacteurs nucléaires dans l’expérience Borexino » (j’ai mis une limite sur le bruit de fond attendu pour cette mesure au travers d’une analyse de données du prototype CTF). Ce travail fût l’objet de ma thèse.