Aucun titre de diapositive - PowerPoint PPT Presentation

About This Presentation
Title:

Aucun titre de diapositive

Description:

... energy range 0.2-1000 GeV and for zenith angles greater than 70 degrees (10 h CPU time) ... 0.2-10 GeV but for all zenith angles (more than 20 h CPU time) ... – PowerPoint PPT presentation

Number of Views:10
Avg rating:3.0/5.0
Slides: 26
Provided by: lakt
Category:

less

Transcript and Presenter's Notes

Title: Aucun titre de diapositive


1
TEST BEAM EXPERIMENT
OPERETTE
C. HERITIER on behalf of operette working group
2
  • OPERETTE
  • WHY?
  • The main aim of Operette is to prepare OPERA
    for what concerns the scanning of emulsion films
    with neutrino events.
  • to check and improve on vertex finding
    efficiency.
  • to check the validity of the brick finding
    efficiency
  • to check the back scattering contribution.
  • USING FREE NEUTRINO BEAM

3
The beam layout
  • 400 GeV p SPS cycle16.8s/Slow spill 5.2 s
  • p(K) beam 9.6 mrad upwards/0.3 mrad spread
  • Muons at EHN2 2x108 /1013 pot(cycle)
  • Neutrinos 2x109/cycle
  • Narrow radial distribution gt small size detector
  • Strong correlation between neutrino energy and
    radial position (CC/NC)

4
Predicted energy from radius vs true energy
Mean Energy vs Radius
5
shielding
beam
1 m
emulsion bricks
TT
dummy bricks
SFT
RPC
6
SFT
7
Neutrinos
1020 m
On-axis
GeV
4 events/brick/month
8
  • Physics Strategy
  • Run during 1-2 months with bricks kept in place
  • Events triggered are recorded from both TT and
    SFT
  • SFT will be used to estimate the brick finding
    efficiency
  • based on TT information
  • (information from SFT seems enough to locate, at
    very high efficiency, the brick)
  • SFT will be used to estimate the back-scattering
  • After the run ? develop and scan all the bricks
  • ? compare with TT, SFT

9
BRICK FINDING EFFICIENCY WITH SFT
  • We are developping an algorithm using
    information
  • of SFT detectors to find the brick. This
    algorithm uses a
  • barycentric method (possible reconstruction of
    particles
  • direction using the 2 doublets of each station).
  • For the Charged Current events, we have a
    resolution
  • about 95 and for the Neutral Current events, 92.

10
BACKGROUND
  • muons produced by neutrino interactions in
  • the earth in front of the detector. The first two
  • RPC stations and the first plane of scintillators
  • allow to improve the rejection efficiency of
  • those muons.
  • cosmics some preliminary results concerning
    this point (Trigger study).

11
Rock Muons Produced by neutrino interaction in
the rock
GeV
6 105 muons/month
12
  • TRIGGER
  • Rock muons
  • Using the veto system (2 RPC stations first TT)
  • 6.105 muons/month ? 2 muons escaping
    detection for 1 month.
  • Cosmics
  • A complete trigger scheme is under study using
    TT RPC informations (at present only the TT
    information is used)
  • Furthermore the use of the SFT requires a fast
    hard trigger (due to the acquisition rate of the
    CCD reading out the SFT 30 fps)

13
COSMICS
  • The experimental set-up was simulated in the
    Geant3 code.
  • We used the same neutrino events generator as
    for OPERA to produce 10000 ??CC events with the
    expected energy spectrum given by the halo code.
  • For the generation of cosmics muons, we use a
    generator provided by M. Sioli.
  • data1 1 minute of cosmics flux in the energy
    range 0.2-1000 GeV and for zenith angles greater
    than 70 degrees (10 h CPU time)
  • data2 10 seconds of cosmics flux in the
    energy range 0.2-10 GeV but for all zenith angles
    (more than 20 h CPU time)

14
?
15
Energy spectrum of cosmics muons.
data1
data2
16
Energy spectrum of neutrino events generated(CC)
? from ?? interaction
The interaction vertex are distributed randomly
inside the emulsion bricks.
17
Number of scintillator planes per event
cosmics
neutrinos
18
Number of strips per event
muons
neutrinos
19
Number of photoelectrons per event
cosmics
neutrinos
The digitization takes into acount the response
of PM.
20
Number of RPC stations per event
Station 1
Station 2
Station 3
Station 4
21
FIRST RESULTS
  • Using a cut at 25 strips per event
  • we have 98 of rejection for cosmics and 90 of
  • efficiency for neutrino events.
  • BUT we can improve by
  • using information from RPC stations
    in front of the detector
  • using the information on the number of
    photoelectrons.

22
CONCLUSION
  • Operette can be a real test for different
    sub-detectors
  • Emulsion, Scintillators, RPC, Electronics ,
    Scanning.
  • Acquisition (electronics, scanning) can be
    tested and
  • strategies can be decided accordingly.
  • Many studies are done and an OPERA note will be
    soon
  • available
  • Expected time to start in 2004

23
  • Installation Strategy
  • TT planes with endcaps and electronic readout
  • should be assembled in one lab.
  • Bricks should be prepared and put in their walls
  • at CERN (aleph pit?)
  • The set-up should then be completed quickly
  • on the detector place before the run
  • It is possible to run one month with only fake
    bricks to test electonics

24
  • Needs List
  • Mechanical structure 2 men during 1
    month
  • TT planes construction 3 men during 1
    month
  • Bricks 4 man
    during 15 days
  • installation 2-4 man
    during 1 week
  • Shift 2 men
    for one month
  • developement 1-2 men for
    one month

25
SFTEmul. Bricks 56.3 K
PMT (22) OPERA
Scint. Strips 800X1 m 2 K
Fibers 800X3 m 4.8 K
Scint. Endcaps 11 K
Scint. Readout OPERA?
RPC Readout 3 K
Lead OPERA
Mechanical structure 2 K
Infrastructure 100 K
TOTAL 180 K
Write a Comment
User Comments (0)
About PowerShow.com