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Lecture 27. Updates. Theme VII. Current theme. Theme VI. Theme V. Theme III. Theme IV. A Hot Early Universe. 1 S. T . Hot Young Universe. Temperature T. as S 0 so T ∞. 0.5. 0. 1.0. Big Bang. Scale factor S. Now. Expansion. Cooling and Thinning.
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Lecture 27 Updates
Theme VII Current theme Theme VI Theme V Theme III Theme IV
A Hot Early Universe. 1 S T Hot Young Universe Temperature T as S 0 so T ∞ 0.5 0 1.0 Big Bang Scale factor S Now
Expansion Cooling and Thinning Scale Factor (S) 10-16 10-13 10-10 108 K 1024 107 1018 104 1012 Temperature (billions of K) Density (tons/cm3) 106 10 1 10-6 1 103 10-12 10-9 10-6 10-3 1 billion K 1 sec 1 ks 1 ms 1 s 1 ps 1 ns Time (seconds)
Particles Move Faster at Higher Temperature Higher Temperature Faster Motion Lower Temperature Slower Motion
Particle Accelerators LHC at CERN RHIC at Brookhaven Tevatron at Fermilab
Beam Pipes CERN: LHC Brookhaven: RHIC
Detectors CMS at CERN ?? CMS at CERN CDF at Fermilab
Scale Factor (S) 10-16 10-13 10-10 2008 LHC/CERN 1990s 106 107 1 TeV 1980s 1960s Temperature (billions of K) 104 103 1 GeV Energy (MeV) 1950s 1 MeV 10 1 1 103 10-12 10-9 10-6 10-3 1 sec 1 ks 1 ms 1 s 1 ps 1 ns Time (seconds)
Below the Threshold Temperature photon proton electron Gas at 1 billion K Particle KE Photons Energy exchange
Electrons and Anti-electrons creation Creation Annihilation Annihilation Above the Threshold Temperature Electron Anti-electron Photon equilibrium Gas at 10 billion K Particle KE Photons Energy exchange
Temperature (billions of K) 1 106 103 50 Quarks added 40 30 1 MeV 1 TeV 1 GeV Number of kinds of particles 20 Leptons added 10 0 1 103 10-12 10-9 10-6 10-3 1 sec 1 ks 1 ms 1 s 1 ps 1 ns Time (seconds)
H Higgs The Standard Model Particles Matter Particles (Fermions) Force carriers (Bosons) Quarks Leptons EM e e d u Family 1 Z W Weak s c Family 2 gs Strong 8 b t Family 3 gv Gravity
Animation of vacuum with pcle/anti-pcle pairs. 1 3 2 4 5 6 7 8 Time sequence for animation of single particle/antiparticle pair forming out of, and disappearing back into, the vacuum (notice steps 1 & 14 are nothing). 14 13 12 11 10 9
A real particles enters and hits a virtual particle pair Have a few of these forming and dissolving pairs visible. Have a red particle enter and strike a fully formed pair.
Virtual pair becomes a real pair. After the collision, make all three particles leve the scene as free agents. Meanwhile the other pcle/antipcle pairs continue to form and dissolve.
One eye-blink Scale Factor (S) 10-16 10-13 10-10 1024 107 1018 104 1012 Temperature (billions of K) Density (tons/cm3) 106 10 1 10-6 1 103 10-12 10-9 10-6 10-3 1 sec 1 ks 1 ms 1 s 1 ps 1 ns Time (seconds)