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PSI 27/6/2006

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Need for space at the back of the MEG area for the accelerator installation ' ... C-W accelerator at 7 m from the COBRA centre ... – PowerPoint PPT presentation

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Title: PSI 27/6/2006


1
PSI 27/6/2006 C.Bemporad
THE TAMING OF MEG News on Calibration Methods
Cockcroft-Walton Accelerator ?-sources on
wire ?-lines from neutron capture on Ni ?-decay
2
THE MEG EXPERIMENT COCKCROFT-WALTON
ACCELERATOR PROTON BEAM-LINE
DELIVERY OF THE COCKCROFT-WALTON
ACCELERATOR DEFINITION OF THE PROTON BEAM
LINE BELLOWS SYSTEM FOR THE TARGET INSERTION
INTO COBRA REQUEST FOR SPACE BEHIND THE MEG
AREA FINANCING ETC.
3
POINTS TO BE CONSIDERED
  • The C-W accelerator is delivered on June-July
    2007, after the
  • start of the MEG data taking
  • The installation of the C-W accelerator at PSI
    and the C-W tuning
  • requires at least one month
  • The C-W accelerator installation should not
    interfere with the MEG
  • running
  • From time to time, some interventions and
    repairs on the C-W will
  • be needed
  • The mutual effects between the C-W accelerator
    and the COBRA
  • magnet must be small. Keep an adequate
    distance between them.
  • A large amount of space is needed (and
    available) in the MEG area for the
  • bellows system and for the p-beam optical
    elements
  • It is convenient that the turning on and the
    tuning of the C-W accelerator
  • take place while the MEG experiment is in
    normal running

4
CONSEQUENCES
  • Need for space at the back of the MEG area for
    the accelerator installation
  • Radiation Safety independently surveyed area
  • Bellows system for p-beam and Li target
    introduction into COBRA
  • p-beam opposite to the ?-beam and on the same
    line (simpler !)
  • C-W accelerator at ? 7 m from the COBRA centre
  • Optical elements needed for beam focusing and
    centring
  • (4 steering magnets, 2 quadrupoles)
  • The C-W accelerator construction and the bellows
    system preparation depend on a decision on the
    availability of the space downstream of the MEG
    area
  • A RATHER COMPLEX PROJECT ! 1) MEG collaborative
    work 2) Help from the National
    Laboratories of Legnaro (advice and spare items)
    (Letter to/from and from the Lab. Director
    G.Puglierin)

RELIABLE AND EASY CALIBRATIONS ARE ESSENTIAL TO
MEG An earlier C-W installation translates into a
saving in time, in effort, in money (The
experiment can be tuned when the PSI beam is not
allocated to MEG and during machine-off periods)
5
PROBLEMS WE ARE IMMEDIATELY FACING URGENT
SOLUTION NEEDED !
C-W accelerator in the engineering phase. Some
characteristics depend on the accelerator
position and hall space availability. Wait for a
decision........? Delayed delivery ! The order
and the construction of the bellows system depend
on the C-W position. The cost of the bellows
system is approx. 85.000 euro If immediately
ordered, it could be ready by November
2006. Desirable a BVR positive recommendation
about the use of hall space for the C-W
installation during this June 27th meeting.
Present INFN financial difficulties. Decision
on our requests (To be based on hall space
availability !) during the July 3rd, or
successive Commission 1 September meeting
6
Cockroft-Walton Accelerator in a fixed
position and Bellows system for inserting the
p-beam and the LiF target into COBRA
P-beam and target inserted into COBRA
(not to scale)
P-Beam and target out of COBRA
7
THE PRESENT MEG AREA The Bellows System and the
p-beam optics (4 steering magnets and 1
quadrupole doublet) can be arranged in the MEG
area
8
Present position of the shielding walls behind
the MEG area
MEG AREA
AREA ON THE BACK OF MEG
9
Proposed position of the new shielding
walls Behind the MEG area
10
Possibility of bellows system, beam optics, C-W
accelerator installation in a single MEG area
(not advisable.......)
11
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12
SINGLETRON COCKCROFT-WALTON ACCELERATOR
13
BELLOWS SYSTEM FOR THE INTRODUCTION OF THE PROTON
BEAM AND OF THE LiF TARGET INTO COBRA
  • The bellows system project is ready
  • (the beam section from the accelerator to the
    bellows system must be completed)
  • It is advisable that the bellows system be built
    during the summer 2006,
  • be fully tested under vacuum and be tuned
    before the end of the year
  • Development of the safety system and of the
    computer controls
  • Improvements in the LiF target and holder.
    Cooling. Beam centring and
  • beam current readings. Beam optics controls
  • Avoid, if possibile, a time-overlap between the
    installation of the bellows system
  • and the delivery, mounting, tuning of the C-W
    accelerator
  • ESTIMATED COST OF THE BELLOWS SYSTEM ? 85 Keuro
  • (if the beam optics elements and power supplies
    are all available at no cost)

14
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15
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17
microphoto of LiF TARGET
very small p-beam irradiation cells of approx.
30 ?m
intermediate p-beam irradiation
18
heavy irradiation at p-beam spot
IMPROVE Lithium Fluoride TARGETS BETTER CARE OF
TARGET COOLING AND GOLD PROTECTION
19
?-sources on wire recent improvements
20
Polonium Wire-Sources RINGS IN LIQUID XENON PMT
Q.E. Measurements
Now in print on Nuclear Instruments Methods
Great if used in the bulk of any Liquid Detector
!
21
Quantum efficiency determinations in Large
Prototype
CHECK OF PMT PROPERTIES IN THE FINAL
CALORIMETER DURING THE EXPERIMENT Americium WIRE
SOURCES 5 WIRES, 5 DOT-SOURCES PER WIRE
Wire of ?100 micron diameter Material gold
plated steel or tungsten Total length 150
cm Spacing of dot-sources 12.4 cm Linear
dimension of dots 1-2 mm Activity ? 200 Bq per
dot
22
first SORAD/ISOTOPE PRODUCTS AMERICIUM
WIRE-SOURCES made by a thermocompression method
Irregular rings, well simulated by the Monte
Carlo Method !
23
EXTRA RD BY SORAD New modified sources
shipped to Pisa on June 18th Elimination of the
wing and of its shadow
24
EXTRA RD BY SORAD interesting new
method Thermocompression of an Am-source strip
wound around the wire
25
thermal neutron capture on nickel and 9 MeV
?-line
26
Calorimeter monitoring by NEUTRONS AND
NICKEL-LINE (Americium Source) hourly
calibration
large-prototype
NaI
NaI ?/E2.5
PROBLEM in the LXe the line is worse larger
background due to fast neutron reactions n2n,
n1?, n2?, n3?, ..
27
  • WAY-OFF
  • reduce the neutron energy by use of a
    Californium source
  • better reject ?-particles from sources on wire
  • select thermal neutrons events by a delayed gate
    window
  • (? 100 ?s) and a trigger from fission prompt
    ?s (lower rate)
  • A GENERATOR OF 9 MEV ?s FROM NICKEL
  • MUST BE READY IN TIME FOR THE FIRST MEG RUN
  • present problems with status of large Sodium
    Iodide Detector

28
hydrogen target to be used inside COBRA (new
test JUST NOW in Pisa !)
29
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30
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31
THE TAMING OF MEG
all proposed calibration methods were tested and
most of them are up to expectations WE ARE
READY..
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