photoelectron spectrometers survey of the universe harry kroto 2004

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Page 1: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Photoelectron Spectrometers

Page 2: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004
Page 3: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Survey of the Universe Harry Kroto

2004

Page 4: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Interstellar MatterHarry Kroto 2004

Page 5: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004
Page 6: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004
Page 7: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

http://www.ugcs.caltech.edu/~yukimoon/BigBang/

Page 8: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004
Page 9: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Gamow

Page 10: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004
Page 11: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Big Bang Hydrogen

Page 12: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004
Page 13: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004
Page 14: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Milky Way Fog

Page 15: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

We can only see about 1/6 (ca 6000ly) of the way to the Galctic Centre due to

scattering by gas and dust in the disk

Page 16: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Harry Kroto 2004

H...H

3 Body Collision

Page 17: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Total energy must be conserved and in a plant at snooker or

billiards the blue ball takes away the energy and the white and red can thus remain in contact after

collision

Page 18: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Reaction Coordinate - Energy

Harry Kroto 2004

A + BProducts C

Page 19: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004
Page 20: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Radioastronomy History

Page 21: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Harry Kroto 2004

3 Degree Background

Page 22: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004
Page 23: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Harry Kroto 2004

Men’n

Franck Condon

Page 24: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Harry Kroto 2004

Ro-vib-ronic Spectra

Page 25: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Harry Kroto 2004

[Ho + V(t)] = iħ/t

Time Dependent Theory

Page 26: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Fermi Golden Rule I

Page 27: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

Harry Kroto 2004

.CN

CN Spectrum

Page 28: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004
Page 29: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004

H2 Dissociation Energy GH&M K&W

Page 30: Photoelectron Spectrometers Survey of the Universe Harry Kroto 2004