cosmic rays in a thermos flask 1.european physics education conference bad honnef thomas trefzger...
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Cosmic rays in a thermos flask 1.European Physics Education Conference
Bad Honnef
Thomas Trefzger Universität Mainz
Motivation
Mystic experiments in school
Introduction to special relativity Introduction to (astro-)particle physics
Minor complexity
Cosmic radiation Interaction of high
energetic primary particles (85% protons, 14% alpha particles) with nuclei of the atmosphere
Surface of the earth: a few hundred charged particles per qm per second
Mostly muons
The muon Group of leptons mass (muon) ~200 x mass of the electron Mean lifetime 2.2 microseconds Decay of the muon:
e
e
e
e
Decay of the muon
Radioactive decay law
Muons should not reach the surface of the earth
1 muon per second
smittNtN 2.2)exp(0
msctvs 660102.29999.0 6
Special Relativity time dilation (observer at earth)v=0.9999c: muon lives longer:
Length contraction, 20km (observer moves along with the muon)
sec106.171
1
1 4
2
2
cv
mss 2821
First Experiment
Measurement without water -> no signalMeasurement with water -> signals
Existence of something which gives a reaction in the thermos flask
Lifetime– it is relative !
Number of events vs. microseconds
0 5 0 5 Microseconds Microseconds
linea
r
loga
rithm
ic
What can we learn ? Cosmic radiation is omnipresent and
can be detected Frequency of occurence, penetration
rate, angular rate dependence
Statistical aspects, randomness of events
Didactic Potential
Exotic particles in school Statistical aspects Aspects of special relativity Ongoing research Elementary particles as part of our
world Computer in measurement control
and analysis