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B. Lee Roberts, Hampton University, 23 March 2007 - p. 1/31 The Muon’s Magnetic Moment What’s all the fuss about anyway? B. Lee Roberts Department of Physics.

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Presentation on theme: "B. Lee Roberts, Hampton University, 23 March 2007 - p. 1/31 The Muon’s Magnetic Moment What’s all the fuss about anyway? B. Lee Roberts Department of Physics."— Presentation transcript:

1 B. Lee Roberts, Hampton University, 23 March 2007 - p. 1/31 The Muon’s Magnetic Moment What’s all the fuss about anyway? B. Lee Roberts Department of Physics Boston University roberts@bu.eduroberts@bu.edu http://physics.bu.edu/roberts.html

2 B. Lee Roberts, Hampton University, 23 March 2007 - p. 2/31 In this talk I Must Explain: The Fuss The Muon (What?) Spin and Magnetic Moments (Why and How?) So What?

3 B. Lee Roberts, Hampton University, 23 March 2007 - p. 3/31

4 B. Lee Roberts, Hampton University, 23 March 2007 - p. 4/31 This transparency has been copied from D. Hertzog, UIUC

5 B. Lee Roberts, Hampton University, 23 March 2007 - p. 5/31

6 B. Lee Roberts, Hampton University, 23 March 2007 - p. 6/31 After only 17 years work

7 B. Lee Roberts, Hampton University, 23 March 2007 - p. 7/31 Let’s step back a moment Over the course of history, we have discovered that the constituents which make up matter seem to come in ever smaller pieces Objects → Molecules → Atoms → electrons + nuclei → neutrons + protons → leptons quarks + gluons → ????

8 B. Lee Roberts, Hampton University, 23 March 2007 - p. 8/31 What? The Muon The muon is a “lepton” (light particle) It appears to be like an electron, except heavier. It undergoes radioactive decay after 2.2  s (millionths of a second) When it was discovered in 1936, it was a big surprise!

9 B. Lee Roberts, Hampton University, 23 March 2007 - p. 9/31 The Muon: Discovered in 1936 Discovered in cosmic rays by Carl Anderson in 1936 It interacted too weakly with matter to be the “Yukawa” particle which was postulated to carry the nuclear force

10 B. Lee Roberts, Hampton University, 23 March 2007 - p. 10/31 The Muon’s Discovery was a big surprise Lifetime ~2.2  s, practically forever (on the subatomic scale). 2 nd generation lepton m   m e = 206.768 277(24) I. I. Rabi

11 B. Lee Roberts, Hampton University, 23 March 2007 - p. 11/31 Chemistry: The periodic table of Elements

12 B. Lee Roberts, Hampton University, 23 March 2007 - p. 12/31 Particle periodic table:The Standard Model Interact weakly through the Leptons e  e   Interact strongly through the gluons g Electroweak gage bosons  Z0Z0 W±W± Quarks ust dcb

13 B. Lee Roberts, Hampton University, 23 March 2007 - p. 13/31 The Leptons Have Spin spin angular momentum I = moment of inertia precession frequency = spin precesses

14 B. Lee Roberts, Hampton University, 23 March 2007 - p. 14/31 Charged Spin ½ Particles have a Magnetic Moment in the simplest theory, g ≡ 2 for spin the spinning particle is like a magnet with a magnetic moment = magnetic field lines

15 B. Lee Roberts, Hampton University, 23 March 2007 - p. 15/31 which precesses in a magnetic field The magnetic moment experiences a torque and has a (potential) energy of orientation and the spin precesses like a top

16 B. Lee Roberts, Hampton University, 23 March 2007 - p. 16/31 (in modern language) (and in English)

17 B. Lee Roberts, Hampton University, 23 March 2007 - p. 17/31 g is not exactly = 2

18 B. Lee Roberts, Hampton University, 23 March 2007 - p. 18/31 We can calculate a (or g) very precisely Forces forces in nature: –strong: holds the atomic nucleus together –electromagnetic: holds atoms together –weak: causes radioactive decay –gravitation: holds the solar system/galaxy together There are effects from the strong, weak and electromagnetic force which contribute to the value of a. This gives us something to compare the measured value with to see if the theory is really describes nature!

19 B. Lee Roberts, Hampton University, 23 March 2007 - p. 19/31 We put muons into a racetrack and measure how fast they spin around

20 B. Lee Roberts, Hampton University, 23 March 2007 - p. 20/31 The wiggles tell us how fast the muons turn

21 B. Lee Roberts, Hampton University, 23 March 2007 - p. 21/31 It appears they turn too fast (a  is too big) All E821 results were obtained with a “blind” analysis. There is a 2.7 standard deviation difference with the value predicted by the standard model Theory

22 B. Lee Roberts, Hampton University, 23 March 2007 - p. 22/31 Measurements have uncertainties No measurement is perfect! The quantity in ( ) is the standard deviation, often denoted by , which is a combination of statistical and systematic uncertainties. The statistical uncertainty depends on the amount of data The systematic error depends on the apparatus and how careful the experimenter is.

23 B. Lee Roberts, Hampton University, 23 March 2007 - p. 23/31 What does the standard deviation  mean?  gives a measure of how precise the measurement is. The smaller , the smaller the permitted range is about the measured value (permitted means probability). 1  2  3 

24 B. Lee Roberts, Hampton University, 23 March 2007 - p. 24/31 What does ppm mean? For example if you measured the distance between Norfolk Va. and Los Angeles, 2358 miles ( = 12,450,240 feet) to a precision of half a ppm, you would know it to within 6.23 feet

25 B. Lee Roberts, Hampton University, 23 March 2007 - p. 25/31 The difference is about 2 parts in a million What could cause this? –the calculation (theory) was wrong –the experiment is wrong –something was left out of the calculation New Physics? What’s the chance that there is a difference anyway? –about 98% IF IT’S ONLY STATISTICS

26 B. Lee Roberts, Hampton University, 23 March 2007 - p. 26/31 So what does 98% mean? If there’s a 98% chance of rain, would you schedule a picnic? –Probably not. If there’s a 98% chance you could double your life’s savings, would you risk losing all of them? –Probably not. If there’s a 98% chance you will arrive safely home after an airplane flight, would anyone fly? –Probably not

27 B. Lee Roberts, Hampton University, 23 March 2007 - p. 27/31 So what would it take to make you say yes? 99% ? 99.9% ? 99.99999% ? In physics, we usually ask for at least 3  ( 99.73%) to claim a discovery, and 5  (99.99994%) is “conclusive”. Is it ever 100%? –NO

28 B. Lee Roberts, Hampton University, 23 March 2007 - p. 28/31 SO WHAT?

29 B. Lee Roberts, Hampton University, 23 March 2007 - p. 29/31 So what might it mean? Have we seen a hint of new physics? Is there a mistake? –well at least our analysis was blind so we didn’t bias the answer How do we “make sure” there is something new rather than a statistical fluctuation? –need at least 3 , 5  is definitive

30 B. Lee Roberts, Hampton University, 23 March 2007 - p. 30/31 A Flight of Fancy Some people claim that we have seen the first evidence for “supersymmetry” –a theory which says that for every particle we know about, there is a companion partner (which we have never seen before)

31 B. Lee Roberts, Hampton University, 23 March 2007 - p. 31/31 In Standard Model we have: antiparticles particles supersymmetric partners (spartners) SUSY: (with thanks to Bruce Winstein)

32 B. Lee Roberts, Hampton University, 23 March 2007 - p. 32/31 Have we discovered something new? STAY TUNED Like much of science, this is a work in progress…

33 B. Lee Roberts, Hampton University, 23 March 2007 - p. 33/31 E821 Collaboration Boston, Brookhaven Lab, Budker Institute, Cornell, Fairfield, Groningen,Heidelberg, Illinois, KEK, Minnesota, Science U. Tokyo, Tokyo Tech, Yale


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