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CNGS - CERN Neutrinos to Gran Sasso. > “Neutrinos” and “Gran Sasso” > CNGS Schedule > Main components, installation at CERN > Neutrinos at CNGS (some numbers). A sincere “ THANK YOU ! “ to the many colleagues who are contributing, - PowerPoint PPT Presentation
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29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 1
CNGS - CERN Neutrinos to Gran Sasso
> “Neutrinos” and “Gran Sasso”
> CNGS Schedule
> Main components, installation at CERN
> Neutrinos at CNGS (some numbers)
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 2
A sincere “ THANK YOU ! “
to the many colleagues who are contributing,at CERN and elsewhere, to the CNGS project
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 3
What are Neutrinos () ?
elementary particles
come in three flavors (LEP) (pistachio, chocolate, vanilla)
electric charge: zero !mass: very small zero? interaction with matter:
“very weak”
“ the elusive particle “
Leptons electric particle charge
e -1
e 0 ------------------------------------
-1
0-------------------------------------
-1
0
+ a
ntip
article
s
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 4
Where are the Neutrinos ?
“all around us” -> radioactive decay of atomic nuclei (natural)
n --> p + e + e
every person is a neutrino – emitter: 340 millions per day20 milligrams radioactive potassium (40K)
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 5
Where are the Neutrinos ?
-> from nuclear reactors -> from the sun
4x1014 neutrinos per second from the sunare traversing our body, but ...
...in 100 years, only 1 solar neutrino interacts with our body.
One would need an iron block 1016 meters long in order to “stop” 50% of the solar neutrinos
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 6
-> at accelerators… (high energy neutrinos)
(proton + Nucleus -> pions -> decay)
Where are the Neutrinos ?
-> from collisions of cosmic rays with nuclei in the atmosphere
-> everywhere around us (cosmic ...)
... ...
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 7
How do we detect neutrinos ?
e
e
p,n,,K...
p,n,,K...
p,n,,K...
neutrinos interact VERY rarely with matter - when they do,they often produce a lepton of their “own flavour”:
NOTE: a minimum amount of energy is needed (to create the mass of the lepton):
me = 0.5 MeV, - m = 106 MeV - m = 1770 MeV
The higher the neutrino energy, the more likely the interaction !
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 8
Neutrino mass ?
Standard model of particle physics: masses “ZERO”
“Direct” mass measurements -> upper limits( in decay experiments measuring kinetic energy of “the partner” )
me < 2.2 eV m
< 170 keV m < 15.5
MeV
What’s the problem ? OBSERVATION 1 : SOLAR NEUTRINO “DEFICIT”
only about 50% of the e expected are actually observed: e
disappear “en route” from the sun to the earth …
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 9
OBSERVATION 2 : “ATMOSPHERIC NEUTRINO ANOMALY”
much less “from below”observed w.r.t. expectations
disappear “en route” over 10’000 km … ?
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 10
Neutrino Oscillation
’s change flavor ! Is this possible? --> Yes, “if neutrinos have mass”!
Gran Sasso
e
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 11
In Dec. 1999, CERN council approved the CNGS project:
build an intense beam at CERN-SPS
search for appearance at Gran Sasso laboratory (730 km from CERN)
“long base-line” -- oscillation experiment
note: K2K (Japan) completed; NuMI/MINOS (US) running
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 12
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 13
ORGANISATION of CNGS
CERN INFNConvention
builds and operatesCNGS neutrino beam
operates the Gran Sassounderground Laboratory,which houses detectors
International
Collaborations
bilateral co-ordinationcommittee
CERN and LNGSscientific committees
special contributionsfinance a large fraction of CNGS
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 14
The Gran Sasso Laboratory(LNGS)
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 15
730 km might seem too short -but look at the details :Background low enough,event rate still acceptable--> 730 km almost perfectAND, VERY IMPORTANT:
- existing laboratory with its infrastructure (since 1987)- large halls directed to CERN- caverns in the GS mountains: 1500 m of rock shielding- tradition in very successful neutrino physics experiments (solar ’s)
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 16
e
,e,
p,n,,K...
Detecting at Gran Sasso
-> look for the lepton:extremely difficult -
travels less than 1 mm before decaying
-> two approaches: (a) very good position resolution (see the decay “kink”) -> OPERA (b) very good energy and angle resolution -> ICARUS
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 17
decay “kink”
~ 0.6 mm
Neutrinos
Electron(or muon)
Hadrons
A tau event can be identifiedbecause it leaves several tracks starting at the same « point » (the neutrino interaction vertex) – one of the tracks (the tau) shows a kink after about ~1 mm.
A detector with excellent spatial resolution is required !
1 mm
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 18
massive « target » : lead platesmicrometric precision : emulsions
assembled in small units called bricks modular detector rapid analysis
56 lead plates (1 mm thick) alternating with56 photographic films (emulsions).
8.3kg
10.2 x 12.7 x 7.5 cm
Brique
Brick
Pb
Couche de gélatine photographique 40 m
1 mm
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 19
OPERA: 1800 tons of “detector mass”walls made of bricks (total more than 200’000)
-> bricks made of “sandwiches”-> sandwiches made of lead and nuclear emulsion
(type of film)
artists view (2001)
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 20
artists view (2004)
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 21
Target SM1
SM1 SM2
Aimants
OPERA status, November 2005
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 22
p + C (interactions) , K (decay in flight)
CNGS beam-line: the main components (1)
(based on CERN experience: PS / SPS neutrino beams -> WANF)
“back to CERN”...
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 23
p + C (interactions) , K (decay in flight)
CNGS: the main components (2)
vacuum
700 m 100 m 1000m 67 m
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 24
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 25
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 26
CNGS schedule
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 27
CNGS works
ground breaking ceremony: 12 October 2000
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 29
CNGS civil engineering
more than 3 km of tunnels and caverns (diameter 3.1 m -> 6.0 m)
more than 45’000 m3 rockto be removed
more than 12’000 m3 concreteto be “sprayed” or poured
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 30
CNGS -- proton beam
-> protons from SPS, 400 GeV-> NEW fast extraction - tested in 2004
-> this extraction system needed for TI8 -> LHC transfer line (but modified for CNGS)
-> CNGS p-beam branches off after 100 metres
-> 700 metres of proton beam line to CNGS target (proton beam spot: = 0.5 mm)
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 31
Electrical distribution
box
Beam position monitor control electronics
MagnetInterlockelectronics
Dipole corrector
Quadrupole
5.6% slope
BEAM
BEAM
CNGS -- proton beam
typical “half cell”
73 deflection (dipole) magnets (6.4 m long, 11 tons) +21 quadrupole magnets + correction dipoles + ...
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 32
Proton beam tunnel – February 2002
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 33
Proton beam tunnel – April 2003
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 34
Proton beam tunnel – Dec. 2004
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 35
Proton beam tunnel – Feb. 2005
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 36
Proton beam tunnel – 1 July 2005
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 37
Proton beam tunnel – 13 July 2005
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 38
Proton beam – November 2005
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 39Proton beam: Monitoring equipment and vacuum system
beam position
beam profile
ion pump
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 40Proton beam: Final focusing towards the target
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 41Proton beam: last beam position / beam profile monitors upstream of the target station collimator and shielding
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 42
-> 10 cm long graphite rods, Ø = 5mm and/or 4mm
CNGS -- target
protonbeam
Note: - target rods thin / interspaced to “let the pions out”
- target rods need to be precisely aligned (0.1 mm)
- target needs to be cooled (particle energy deposition)
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 43
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 44
target unit (assembly of Alu container)
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 45
target magazine (4 spare target units)
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 46Target station installed in final configuration – 8 March 2006
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 47
target magazine with motors, in the lab
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 48
target station motor / indexing finger
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 49
CNGS -- focusing devices
length: 6.5 mdiameter: 70 cmweight: 1500 kg
Pulsed devices:150kA / 180 kA, 7 ms
water-cooled:distributed nozzles
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 50
“Magnetic Horn” (S. van der Meer, CERN 1961)
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 51
0.35 m
35 GeV positively charged particles leaving the target
Principle of focusing with a Magnetic Hornmagnetic volume given by “one turn” at high current:
specially shaped inner conductor - end plates cylindrical outer conductor
inner conductor
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 52
secondary beam focusing with horn/reflector
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 53
CNGS -- focusing devicesDesign criteria:>95% probability to work for 20 Mio. pulses
courtesy LAL/IN2P3
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 54
The inner conductor:- as thin as possible (particle absorption)- as thick as necessary (mechanical stability)
courtesy LAL/IN2P3
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 55
reflector assembly – inner and first “barrel” of outer conductor
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 56
reflector assembly – inner and second “barrel” of outer conductor
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 57
reflector assembly – connection plate with GRAFOIL ring and glass disk
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 58
reflector assembly – connection plates onto first “barrel”
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 59
magnetic horn completed (in the laboratory)
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 60horn in the lab – beam entrance side
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 61horn in the lab – beam exit side (“neck”)
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 62
reflector transport – arrival at BA4
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 63reflector transport – in the service gallery
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 64horn installation in the target chamber – 31 Jan. 2006
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 65
Powering of a Magnetic Horn6000 V / 9000 A
400 V / 150000 A
”Stripline”
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 66
“stripline”150000 A
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 67
3 twistedcables6000 V /9000 A
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 68in progress: horn roof closure
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 69
horn roof shieldingcompleted
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 70
Helium Tank and shielding
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 71
/ K profile at entrance to decay tunnel
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 72
CNGS -- decay tube
- dimensions of decay tube: 2.45 m diameter steel tubes, 6 m long pieces, 1 km length welded together in-situ vacuum: ~1 mbar tube embedded in concrete
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 73decay tube sleeves produced and delivered “just in time”
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 74
6 m long sectionlowered down theCE shaft
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 756m long tube transported along the access gallery
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 76
target chamber: assembling the 18m long sections
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 7718m section transported along the decay tunnel
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 78
Welding inside decay tube
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 79
CNGS -- hadron stop
- hadron stop: 3.2 m graphite 15 m iron blocks
upstream end: water cooled
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 80
11 July 2003 – near the shaft PGCN
graphite
cooling modules
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 81
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 82Hadron stop – 28 July 2003
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 83Hadron stop – 2 Sept. 2003
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 84
CNGS -- muon detectors
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 85
expected CNGS muon profiles
first muon chamber second muon chamber
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 86
muon detectors(ionisation chambers)
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 87
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 88
Radial distribution of the- beam at Gran Sasso
detector cross section
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 89
Neutrinos at CNGS – some numbers:
For 1 day of CNGS operation, we expect:
protons on target 2 x 1017
pions / kaons at entrance to decay tunnel 3 x 1017
in direction of Gran Sasso 1017
in 100 m2 at Gran Sasso 3 x 1012
events per day in OPERA 25 per day
events (from oscillation) 2 per year
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 90
29 June 2006CERN Neutrinos to Gran Sasso
Seminar for CERN guides, by K. Elsener 91
more information:
www.cern.ch/cngs