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16 May 2005 Debbie Harris, PARTICLE DAY 1
From Illinois to Minnesota in 1/400 of a second
Debbie HarrisFermilab
PARTICLE DAY
16 May 2005 Debbie Harris, PARTICLE DAY 2
What is this all about?
• What’s a neutrino?• Where do they come from?• How do you make them?• Why would you send them from
Fermilab (in Illinois) to Minnesota?
16 May 2005 Debbie Harris, PARTICLE DAY 3
Neutrinos are Everywhere…
• Neutrinos are tiny particles with no charge that weigh less than any other particle we know about (except for light)
• There are more neutrinos than any other particle in the universe—by more than a billion! (except for light)
16 May 2005 Debbie Harris, PARTICLE DAY 4
How did they get here?
• Neutrinos are made all the time:• In the Beginning• As the sun shines• As the supernova
explodes• As the banana splits• Every time atoms fall apart or
come together
16 May 2005 Debbie Harris, PARTICLE DAY 5
So why haven’t I heard of them before?
• One neutrino can go through a distance of 200 earths before interacting!
• Someone only figured out they might exist in ~1930 (Pauli)
• Seen for the first time in 1956 by putting a detector near a nuclear reactor (Reines and Cowan)
ν …
16 May 2005 Debbie Harris, PARTICLE DAY 6
How can humans make neutrinos?• Nuclear Reactors
• Huge amount of energy leaves reactor as neutrinos!• Make a beam of particles that decay to neutrinos
• Start with particles you already have: protons• Give the protons energy with an accelerator • Slam high energy protons against a target to make
new unstable particles• Focus!• Give the particles free space to fly through so they
can decay instead of interact
16 May 2005 Debbie Harris, PARTICLE DAY 7
So what’s the catch?
• Since neutrinos interact so rarely (1 in a billion…)• Have to make a lot of them
(billions)
• Have to give them a lot of chances to interact (huge detectors)
16 May 2005 Debbie Harris, PARTICLE DAY 8
How can you shoot a beam to Minnesota?• Imagine you have a laser, and you
want to shoot from here to Boston• What direction would you point your
flashlight? (hint: the earth is round)
• The neutrino beam has to go at that same angle (3.5o down from horizon)
735 km
16 May 2005 Debbie Harris, PARTICLE DAY 9
Digging a hole towards Minnesota• Using the latest in subway line
excavation, we built a huge tunnel 2/3 mile long, 21’ diameter
16 May 2005 Debbie Harris, PARTICLE DAY 10
Filling the hole towards Minnesota• Have to lower magnets weighing many tons down
the shafts• Have to put a big pipe
down the shaft
• Have to pour concrete all around the decay pipe to use as shielding for all the stuff that gets made that hits the walls
• Have to put a near detector in the last section of the hole
16 May 2005 Debbie Harris, PARTICLE DAY 11
Getting the Protons to the target
16 May 2005 Debbie Harris, PARTICLE DAY 12
Target and shielding
• .9m of graphite, has to absorb the power of 200 hair dryers on a spot 2mm in diameter!
Hint: to do this,Need lots of
cooling…
16 May 2005 Debbie Harris, PARTICLE DAY 13
Focusing what comes off the target• Has to be able to take
200,000 Amps!
Better cool this too!
16 May 2005 Debbie Harris, PARTICLE DAY 14
What else gets made?
• When these unstable particles decay, they make neutrinos and muons
• There are also some protons left over that went straight through the target
• Want separate detectors to measure both!
absorber
16 May 2005 Debbie Harris, PARTICLE DAY 15
How can you see a neutrino?
• These three neutrinos (ν’s) are associated with three charged particles, who are as different in size as • Squirrel (e: electron)• Lion (μ: muon)• Elephant (τ: tau)
ν
p
e,μ,or τ
n
You can’t see the neutrino, but you can see their partners
16 May 2005 Debbie Harris, PARTICLE DAY 16
Neutrino Detectors
• Because neutrinos interact so rarely, need LOTS of detector…
Far detector:
•5400 tons of Steel and scintillator•2½ stories tall!•½ mile underground in Soudan Mine, MN
Near detector: 5x Smaller, 1000 times closer
16 May 2005 Debbie Harris, PARTICLE DAY 17
Why are you sending neutrinos from Illinois to Minnesota?
• There are three kinds of neutrinos, and there is evidence that they can change from one kind to another
• For these neutrinos, need towait ~1/400 of a second: if you’re traveling the speed of light, this means about 450 miles
e μ τ
16 May 2005 Debbie Harris, PARTICLE DAY 18
Why study changing neutrinos?• Neutrinos changing
from one flavor to another might tell us about • why there is so
much more matter than antimatter in the universe…
• Why we have so many particles that have such very different weights
16 May 2005 Debbie Harris, PARTICLE DAY 19
Anatomy of an experiment• Design• Construction • Commission –does everything
work the way you planned? • Take the data • Analyze the data• Publish your results
Sounds familiar, doesn’t it?
16 May 2005 Debbie Harris, PARTICLE DAY 20
How long does this take?
• Design can take several years• Getting funding takes time…• Construction:
• Detectors were 1-2 year long projects• Beamline took 4 years! (including all the
underground construction)• Commission: 6 months?• Run: 3 to 5 years• Analyze data: depends, but can be a few
more years…• Moral: need to be patient, or work on more
than one experiment at once…
16 May 2005 Debbie Harris, PARTICLE DAY 21
Who is on this experiment?
• ~250 physicists and engineers from 6 countries
16 May 2005 Debbie Harris, PARTICLE DAY 22
So what do I have to do with all this?
• I have been on this experiment for 5 years• Proton Detectors
• Before the target: how many do we need?• After the target: can one be built to survive?
• Muon Detectors• What can they tell us about the neutrinos?• How big, how many do we need?
We’re just now starting to take data, so now I get to see how well everything works…
16 May 2005 Debbie Harris, PARTICLE DAY 23
First Protons to the beamline: December 3In 10 carefully planned shots,Got the proton beam all the way From the Main Injector to the End of the decay pipe
Hit the monitor dead center to within an inch, a mile from where the protons started!
16 May 2005 Debbie Harris, PARTICLE DAY 24
First Neutrinos seen in Near Detector January 21
• Put target in the way of the protons, make the particles that decay to neutrinos
• See muons(madewith neutrinos) right away
• See neutrinos by4th time we sent protons to the target
16 May 2005 Debbie Harris, PARTICLE DAY 25
First neutrinos seen in Far Detector: March 20• Learn how to send 10 TRILLION
protons to the target every 3 seconds
• Learn how to cool everything the protons hit fast enough
• Roughly every 1019 protons, should get a neutrino in Minnesota
16 May 2005 Debbie Harris, PARTICLE DAY 26
First Neutrino from Illinois• Arrived 2.5msec after sending
protons to target
This is a high energy lion-type neutrino!
16 May 2005 Debbie Harris, PARTICLE DAY 27
Do all lab experiments work perfectly?
• Leaky Target• the target has pipes
around it that carry water to cool it
• On March 23, discovered a leak
• What does it look like to the detector at the end of the beamline?
16 May 2005 Debbie Harris, PARTICLE DAY 28
Fixing the problem
• 6 weeks later, we came up with a solution (pushing on the hole from the other side) and we are starting to run again (see next far detector neutrino event)• What happens with a target that had
water in it?• How long will the leak stay plugged?• How quickly can we build all the spare
parts we need?
16 May 2005 Debbie Harris, PARTICLE DAY 29
More neutrinos arriving daily…
• This looks like a lion (with low energy)
16 May 2005 Debbie Harris, PARTICLE DAY 30
So what have I learned?
• Be prepared: you’ll never predict what will go wrong with your experiment but something will go wrong…
• Lots of things will work just like you predicted—but it will seem like magic anyway
• Stay tuned, we’ll learn soon if we see neutrinos changing!
16 May 2005 Debbie Harris, PARTICLE DAY 31
So what have you learned?
• Questions? Please ask!!!
• Or visit http://www-numi.fnal.gov