C.T.R. Wilson. Charles Wilson is 2nd from right in the front row. Can you find Paul Langevin and...

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C.T.R. Wilson

Transcript of C.T.R. Wilson. Charles Wilson is 2nd from right in the front row. Can you find Paul Langevin and...

Page 1: C.T.R. Wilson. Charles Wilson is 2nd from right in the front row. Can you find Paul Langevin and O.W. Richardson?

C.T.R. Wilson

Page 2: C.T.R. Wilson. Charles Wilson is 2nd from right in the front row. Can you find Paul Langevin and O.W. Richardson?

Charles Wilson is 2nd from right in the front row.Can you find Paul Langevin and O.W. Richardson?

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Nobel Prizewith Compton

1927

2 major paperswith illustrationspublished 1923

first photos ofα,β particles

1911

first chamber- x ray photos

1895

Cloud Chamber

" published Theory of "Thundercloud Electricity

1956

promoted to Reader of Electrical Meteorology

1918

. Observer in Met Physics Solar Physics Observatory

1913appointed

Meteorological Societyemployment

1899

AtmosphericElectricity

MAJOR INTERESTS

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“the most original and wonderful instrument in scientific history.”

- Rutherford

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• ALPHA broad, straight track

• BETA thin, bending track

• GAMMA no tracks as too few ions are

produced in the air

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1911 photo

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1912 Wilson photo

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Compton Scattering : What?

• X-ray photons collide with electrons in carbon atoms.

• The scattered photons are shifted to longer wavelengths (lower energies).

incoming

photon λiscattered

photonλse- at reste-

recoil

angleθ

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Compton Scattering : So What?

• The particle theory of light was still controversial in the 1920’s, despite Einstein’s photoelectric effect.

• Compton used a particle model of the photon, and classical conservation of momentum, to explain the shift in wavelength of the observed scattered x-rays.

Δλ = hmec(1-cosθ)

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• evidence of Compton Effect (Nobel Prize Compton & Wilson 1927)

• evidence of transmutation of elements (Rutherford’s N + α -> O + p)

• discovery of positron and the pair creation-annihilation of electrons & positrons (Nobel Prize Anderson 1936)

• discovery of muon

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• P. BLACKETT “counter controlled cloud chamber” (Nobel Prize 1948) added a Geiger Counter above & below the c.c. Cosmic rays triggered gas expansion and their own photos when impulses hit both counters simultaneously.

• D.A. GLASER “bubble chamber” replaced the c.c. in 1952, using liquid He or H2. Higher density medium allowed photos of high-E particles that were too fast for the c.c.

Beyond the Cloud Chamber

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Web Resources

• http://home.houston.rr.com/molerat/cloud.htm how to make a cloud chamber

• http://www.nobel.se/physics/laureates/1948/press.html Wilson’s Nobel address

• http://hyperphysics.phy-astr.gsu.edu/hbase/quantum/comptint.html#c1 Compton Effect

• http://www.boltlightningprotection.com/lightning_physics.htm lightning physics