S103 Discovering Science Diary
Block 11
[ Block 1 ] [ Block 2 ] [ Block 3 ] [ Block 4 ] [ Block 5 ] [ Block 6 ] [ Block 7 ] [ Block 8 ] [ Block 9 ] [ Block 10 ] [ Block 12 ]
6th July 2003
This, of course, is the block I've opted not to study, so I am slowly reading through it without having to worry at all about doing a TMA. VERY, VERY interesting - although there are lots of bits that I would spend more time over trying to understand, if I had to answer questions on it afterwards! I think, personally, we should have to do all the blocks and all the TMAs.
Forward to Block 12
Back to Block 10
Back to Block 9
Back to Block 8
Back to Block 7
Back to Block 6
Back to Block 5
Back to Block 4
Back to Block 3
Back to Block 2
Back to Block 1
Back to S103 | Block 11: Universal Processes
The expanding Universe
Measuring the disrance to galaxies
Measuring the speed of galaxies
The Hubble relationship
Expanding space
A few strange ideas
The age of the Universe
The cooling Universe
Black-body radiation
The cosmic microwave background
The hot big bang model for the origin of the Universe
Four fundamental interactions
Electromagnetic interactions
Electric forces
Magnetic forces
Electromagnetic radiation
Quantum electrodynamics
Strong interactions
How strong is strong?
Jets of hadrons
Quantum chromodynamics
Weak interactions
Comparisons of fundamental interactions
W and Z bosons
The survival of the neutron
Gravitational interactions
Newton's gravity
General relativity
Quantum gravity
Four forces in the Sun
Gravitational interactions in the Sun
Strong and weak interactions in the Sun
Electromagnetic interactions in the Sun
Unified theories
Electroweak unification
Grand unification
Superunification
The evolving Universe
Time, space, temperature and energy
The very early Universe
Inflation - a cosmic hiccup
The quark-lepton era
The hadron era
Primordial nucleosynthesis
Structure in the Universe
The future of the Universe
A closed Universe
An open Universe
A compromise ... ?
|
|