Using muon physics to teach relativity, radiation, and instrumentation Daniel W. Koon 1 and Jeremy Ouellette Department of Physics St. Lawrence University.

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Presentation transcript:

Using muon physics to teach relativity, radiation, and instrumentation Daniel W. Koon 1 and Jeremy Ouellette Department of Physics St. Lawrence University Canton, NY, USA 1 SUMMARY: Muon physics provides a convenient tool for teaching various aspects of radiation physics and instrumentation in an undergraduate lab. We will describe how we have been using cosmic muons in a second-year undergraduate teaching laboratory to teach radiation physics and instrumentation. We will also describe how we recreated a classic muon decay experiment to test special relativity, using equipment available in an undergraduate laboratory and comparing measurements from both Mt. Washington (elevation 1917m) and near sea level. Finally, we will address the suitability of this test of special relativity to undergraduate teaching laboratories throughout the Americas, especially along the Cordillera de los Andes and in Central America, where the change in altitude needed can sometimes be obtained with a drive of a few hours or less. MOTIVATION: Teaching nuclear physics can be a particular challenge in a small undergraduate laboratory. A cosmic muon detection lab simplifies matters in the following ways: Muons: Cheap, plentiful Require no handling, additional radiation safety procedures Distinctive double-decay signature: easily identified, even against a noisy background Instrumentation Scintillator: Rugged radiation transducer Photomultiplier: Useful detector for general laboratory applications Storage scope: Simple solution for collecting time- domain events Fig. 1: Photomultiplier tube (left) and plastic scintillator Fig. 2: Scintillator/detector assembly inside the protective light-covering. SLU apparatus: Scintillator: 15cm diameter x 13 cm height plastic scintillator PMT: RCA 6342A, 5cm diameter end-on window Electronics: Differentiator, homemade, OP27GP-based 40x inverting op amp amplifier, homemade. Oscilloscope: Tektronix TDS 210 Shielding: Lead bricks Fig. 3: Output of storage scope Tektronix TDS 210. Trace 1 (top) shows raw scintillator signal, triggered at the left hand side of the screen. Trace 2 (bottom) shows output of an ORTEC 420 Timing SCA. Horizontal scale is 1 microsecond per division. Bottom trace clearly shows dead time of 1.3  s. There is an electronic delay of 1.4  s between top and bottom traces. EXPERIMENTS: MUON LIFE TIME, DETECTOR DEAD TIME Mean lifetime: (See Fig. 4a) Results:  = 2.23 ± 0.07  sec Accepted value: 2.20  sec Deadtime: (See Fig. 4b) 1.3 ± 0.2  sec Compare to: Geiger-Müller tube: typ. 100  sec Figure 4a: The number of muons remaining in the scintillator as a function of time, for trials on top of Mt. Washington (top) and in Canton, NY (bottom). Both graphs are labeled with best-fit exponential curve parameters. Mean lifetime is determined from this fit. Figure 4b: Mt. Washington data of Fig. 4a, on expanded scale. Dead time is measured from connecting a straight-line fit of the first three data points to the exponential curve of the rest of the data. EXPERIMENTS: PROOF OF RELATIVISTIC TIME DILATION IN COSMIC MUONS 1 Mt. Washington (elevation 1907m) Trial A150 counts / 3hr B124 C133 Average136 ± 21 (95% confidence level) Canton, NY (1770m or 6.9  s v=0.9c) Trial D61 counts / 3hr E61 F52 Average58 ± 10 (corresponds to 3.5 ± 0.4  s travel from Mt. Washington) Measured:  = 2.0 ± 0.2 Classical result:  = 1 In conclusion, we have measured the time dilation factor to definitively exclude the classical result. COSMIC MUON SPECTROSCOPY IN LATIN AMERICA Even larger discrepancies between classical and relativistic predictions are possible along the Rocky Mountains, the Andes, and the mountains of Central America, where one can reach great extremes in altitude with just a few hours’ drive. A large change in altitude allows for a much more emphatic proof of relativistic time dilation. As an example, consider Costa Rica. Predictions of the remaining flux of cosmic muons at sea level based on measured flux at the top of a 3400m summit will differ by a factor of 20 (relativistic prediction larger by a factor of 20 than the classical prediction). This provides for a conclusive test of the predictions of special relativity. Both Irazú and sea level are within three hour’s drive from San José In the Meseta Central. REFERENCE: 1. David H. Frisch and James H. Smith, “Measurement of Relativistic Time Dilation Using  -Mesons”, Am. J. Phys. 31, (1963). FOR MORE INFORMATION: LocationAltitude (m) relativistiic / classical prediction Volcán Irazú34121:1 Meseta Central :1 Sea level020:1