Cosmic rays and how a Bristol Physicist won the Nobel Prize Dr Helen Heath.
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Transcript of Cosmic rays and how a Bristol Physicist won the Nobel Prize Dr Helen Heath.
Cosmic raysand how a Bristol Physicist won the Nobel Prize
Dr Helen Heath
1788
http://books.google.co.uk/books?id=by5EAAAAcAAJ
100 years of Cosmic Rays
NASA TV
What are cosmic rays
• Primary Cosmic rays• 85% protons• 12% helium nuclei (alpha particles)• 3% heavier nuclei• 2% electrons
http://www.phys.uu.nl/~thooft/quarks.gif
Baryons
Mesons
Particle Energy(MeV) v year
1900 1920 1940 1960 1980 2000 20201
10
100
1000
10000
100000
1000000
10000000
First Cy-clotron
BevatronAntiproton
LHC
Mass of lightest “new particles”
Natural Radioactivty
Cecil Frank Powell
• Nobel Prize 1950
“for his development of the photographic method of studying nuclear processes and his discoveries regarding mesons made with this method.
The Start of Big Physics?
• “These developments in international collaboration formed an essential background to the setting up of large international laboratories such as CERN”
D.H.Perkins
40 years of Particle Physics Conference
Bristol July 1987
Sub-atomic particles
• Nucleus• Protons • Neutrons
• Electrons• First antimatter particle – positron• Photons
Yukawa
• Proposed a field theory of nuclear forces.• Field theory requires field quanta.
• We can estimate the mass of such a quanta from the Uncertainty Principle• E t ≈ h (h=6.63x10-34Js)• t ≈10-15/c ≈ 0.3x10-22s• E ≈ 2.2x10-11J• E = mc2 m=0.24 x 10-27 kg=0.14mp
Mesons
• If Yukawa’s theory was correct • there must be a field particle
• The hunt was on for a meson• Today we use meson to mean a combination
of a quark and an antiquark• Originally it was a particle with a mass
between the proton and electron• Mesos – Intermediate
(Modern Aside)
• Mass is unexplained • Proposed Higgs
Mechanism• Requires Higgs Field• ..and therefore the
Higgs boson
Experimental techniques
• Cloud Chambers• Bubble Chambers• Emulsions• Solid detectors
Cloud Chamber
• The discovery of the positron• Carl D. Anderson – Physical Review 1933
Bubble Chamber
©CERN photo
Cecil Powell
• Cecil Powell started an autobiography which can be found at• http://www.phy.bris.ac.uk/history.html
• He succeeded academically winning a scholarship to Judd School and then moving on to Sidney Sussex Cambridge
• From an early age he was an enthusiastic, if not always, talented investigator.
After Cambridge
• Nearly became a teacher
• Research student at Cambridge • Supervised by Wilson
• Recruited by Tyndall to Bristol in 1928
The emulsion technique
• Cloud chambers and bubble chambers need to be photographed
• Emulsions are continuously active• Emulsions are also rather portable
• Important for early observatories & balloons
http://www.imcce.fr/phemu03/Promenade/pages5/545.html
Photographic Emulsion
• Grains of silver bromide suspended in gelatine.
• Light causes changes to the silver bromide.
• Developer changes the affected grains to silver
• Fixer removes the remaining silver bromide
Powell’s research group
The pion
• In 1936 C. Anderson and S Neddermeyer observed negatively charged particles with mass intermediate between that of the proton and the electron• Initially called mesotrons• Renamed the mu-meson in 1947
• Now mesons are a subset of hadrons • The mu meson is a lepton
Measuring energies
• Energy loss in the Emulsion is approximately continuous.• The range of a particle depends on its energy
Double meson events
• Seen in events from the Jungfrau Joch• The second meson has a range of 600 m
Interpretation
• In Double meson events one meson decays to another
• - -
• Since the pion has stopped all the kinetic energy of the decay products comes from the change in mass• Pion mass =139.6 MeV/c2
• Muon mass = 105.7 MeV/c2
After the Nobel Prize• Powell continued
to work with emulsions
• Left is the first example of a Kaon decay to three pions
• Work switched to balloons rather than mountains.
Modern Cosmic Ray Work
LHC Energies
Open Question
• Origin of very energetic cosmic rays
• GZK –Cutoff
(Griesen-Zatsepin-Kuzmin)
Cronin, J. W., 1999, Cosmic Rays: the most energetic particles in the universe, RvMA 71, 165–172
Sparse Array – Large area
HiSPARC project High School Project
on Astrophysics Research with Cosmics
>100 detector across
The Netherlands
HiSPARC – school detector
Students build their own detector
And place it on top of the roof of the school