fluka energy deposition study : early separation scheme with dipole d0 first results
DESCRIPTION
FLUKA Energy deposition study : Early separation scheme with Dipole D0 First Results. Christine HOA (AT-MAS-MA), Guido STERBINI (AT-MAS-MA),. Outline. LHC Upgrade configuration with D0 FLUKA energy deposition calculations Monte Carlo code Modeling parameters - PowerPoint PPT PresentationTRANSCRIPT
Section meeting 22/08/06
Energy deposition study on D0 1
FLUKA Energy deposition study :
Early separation scheme with Dipole D0
First ResultsChristine HOA (AT-MAS-MA), Guido STERBINI (AT-MAS-MA),
Section meeting 22/08/06
Energy deposition study on D0 2
Outline
LHC Upgrade configuration with D0 FLUKA energy deposition calculations
Monte Carlo code Modeling parameters D0 results for energy deposition
Investigations: P-P collisions Next steps Conclusions
Section meeting 22/08/06
Energy deposition study on D0 3
LHC Upgrade configuration with D0 Early scheme D0 dipole
Q1 Q2 Q3Q2Q3
IP
D0D0
Q1
Upgrade luminosity: 10 35cm-2 s-1
Total power: 18 kWQuestion: Energy deposition in the dipole?… in the IR quads?
Section meeting 22/08/06
Energy deposition study on D0 4
FLUKA: Monte Carlo code
Multi-particle transport code CERN/INFN development
A. Ferrari, P.R Sala, A. Fassò, J.Ranft
Fluka team with technical support at CERN
Version 2006, not yet released Including DPMJET
Event Generator
for the p-p collisions
DPMJET
FLUKAParticles trackingInteractions/ TransportEnergy deposition
GEOMETRY Magnetic field
Post-treatmentsFlukaplot.r, Simplegeo, fluka Gui, MATLAB, Mathematica
Source particles
Simplegeo V.2,DTUJET, DPMJET ROXIE, …
Section meeting 22/08/06
Energy deposition study on D0 5
FLUKA: Modeling parameters
Section meeting 22/08/06
Energy deposition study on D0 6
FLUKA: Modeling parameters
Beam parameters
p-p collision DPMJET event generator
Crossing angle 0
x (m) 11.81E-6
y (m) 11.81E-6
z (m) 7.55E-2
L, Luminosity 1035
A, Cross section (mbarn) 80
Section meeting 22/08/06
Energy deposition study on D0 7
FLUKA: Modeling parameters
Meshing Cartesian mesh: 0.2*0.2*2 cm Physical meaning with
respect to quench limitrelated to minimum cable dimension (width of 1-2 mm)
(discussion with D. Tommasini)
Computing parameters Nb of particles for good
statistics: 3*1000 particles (CPU time 16 hours)
Cut-off parameters
Number of primary particles
3000
CPU time 16 h
Cut off energy for e-/+e-
<30 keV in the dipole and beam pipe<2 MeV in the Air cylinder region
Cut off energy for photons < 3 keV in the dipole and beam pipe< 200keV in the Air cylinder region
Cut off energy for Hadrons/ Muons
<100 keV
Cut off for high energy neutrons
< 19.6 Mev
Cut off for low energy neutrons
thermal energies
Section meeting 22/08/06
Energy deposition study on D0 8
FLUKA: D0 results Without magnetic field
1st slide of the dipoleZ=[0,2] cm
Section meeting 22/08/06
Energy deposition study on D0 9
FLUKA: D0 results Without magnetic field
36 mW/cm3
12 mW/cm3
Section meeting 22/08/06
Energy deposition study on D0 10
FLUKA: D0 results
With a constant magnetic field of 6 T
Section meeting 22/08/06
Energy deposition study on D0 11
FLUKA: D0 results
With a constant magnetic field of 6 T
Section meeting 22/08/06
Energy deposition study on D0 12
FLUKA: D0 results
Comparing results: deposited power in D0
Total heat deposition
(W)for L=1035 and A=80
mbarn
Averagedheat
depositiondensity
(mW/cm3)
Maximun heat depositiondensity(mW/cm3)
Quench limit
IR in quadsNb Ti
(mW/cm3)
Quench limit
Nb3Sn quads
(mW/cm3)
Without magnetic field
33.4 8.3 48.3 12[Mokhov]
36[Mokhov]
With magnetic field of 6 T
34.3 8.6 49.7 12[Mokhov]
36[Mokhov]
[Mokhov]: “Beam induce energy deposition studies in IR Magnets”, April 2006, WAMDO workshop
Section meeting 22/08/06
Energy deposition study on D0 13
FLUKA: D0 results
Summary 34 W deposited power in the dipole no influence of the magnetic field
Opening questions Why such a small value?
Investigation on the p-p collision:
Spatial distribution and energy range
Section meeting 22/08/06
Energy deposition study on D0 14
P-P collisions analyses
Aim: Distribution of secondaries w.r.t of energy range and space
Y
p-p collision at 14 TevUpgrade Luminosity 1035 cm-2.s -1 18kW
Polar distribution: from 0 to 180
Sphere: 180 ring regions
Z
X
Section meeting 22/08/06
Energy deposition study on D0 15
P-P collisions analyses
Far field region of the interaction at R>3.5m
Section meeting 22/08/06
Energy deposition study on D0 16
P-P collisions analyses Spatial distribution (no crossing angle)
IP
D0 dipoleIR=3.5 cmOR=5 cm
=0.75=0.35
1 m3.5 m
Section meeting 22/08/06
Energy deposition study on D0 17
P-P collisions analyses
Scaling law for aperture radius
Section meeting 22/08/06
Energy deposition study on D0 18
P-P collisions analyses
Power spectrum in D0 dipole
1 Gev-100 Gev : narrow power spectrum
62% Charged particles38% Neutral particles30% Photons
Section meeting 22/08/06
Energy deposition study on D0 19
P-P collisions analyses
Power spectrum in D0 dipole
Photon total energy in D0: 44 Wmost of this energy is deposited in D0
Section meeting 22/08/06
Energy deposition study on D0 20
Next steps
Origins of the energy deposition More details on charged particles?
To take into account Crossing angle : small effects expected?
Magnetic field of the Solenoid: small effects expected?
Section meeting 22/08/06
Energy deposition study on D0 21
Conclusions
FLUKA results: 34 W of power deposition
Good surprise! Understanding of this result
Z> 3.5 m :far field region of the p-p interactions High energetic particles channeled in the beam pipe Impinging energy in the dipole at 3.5 m: 144 W
Solutions to decrease the energy deposition: Increase the aperture of D0 front absorber
%d0%a4%d0%93%d0%9e%d0%a1%203 %20%d0%9b%d0%b5%d1%87%d0%b5%d0%b1%d0%bd%d0%be%d0%b5%20%d0%b4%d0%b5%d0%b
%d0%92%d1%96%d0%b4%d0%bf%d0%be%d0%b2%d1%96%d0%b4%d1%8c %d0%9e%d0%b1%d1%83%d1%85%d1%96%d0%b2 %d0%bf%d
%d0%9f%d0%be%d0%bb%d0%be%d0%b6%d0%b5%d0%bd%d0%b8%d0%b5 %d0%9f%d0%be%d1%81%d0%bb%d1%8b%20%d0%9f%d0%be
1060204 %d0%bb%d0%b8%d1%81%d1%82%d0%be%d0%b2%d0%ba%d0%b0 %d0%bf%d0%be %d1%82%d0%b5%d0%bf%d0%bb%d0%be