Inflationary Big Bang Cosmology Timeline
HTML version by Peter Lamb.
Timeline values are expressed as time after the Big Bang in seconds; temperatures are in Kelvin.
THE QUANTUM GRAVITY ERA
- 1x10^-43 s
Quantum limit of classical general relativity
THE INFLATION AND SYMMETRY BREAKING ERA
- 1x10^-38 s
Limit of perturbative interaction thermalization of universe
- 1x10^-35 s
Grand unification spontaneous symmetry breaking
- 1x10^-34 s
Approximate start of inflation
- 1x10^-32 s
Approximate start of reheating and end of inflation
- 1x10^-11 s
Electroweak unification spontaneous symmetry breaking
THE QUARK-LEPTON ERA
- 2x10^-7 s
Tauon anti-tauon annihilation
- 1x10^-5 s
Formation of hadrons from quarks
- 7x10^-5 s
Muon anti-muon annihilation
- 5x10^-4 s
By this time the universe has a baryon-antibaryon asymmetry which results from post-inflationary B,C,CP violating processes
- 1x10^-1 s
Neutral current weak interactions become too slow and neutrinos decouple
- 1x10^0 s
Charged current weak interactions become too slow and neutron to proton ratio freezes out
- 1x10^1 s
Electron positron annihilation
THE RADIATION ERA
- 1x10^2 s
Typical photon energies drop below the deuteron binding energy and nucleosynthesis begins
- 1x10^3 s
Particle energies drop below coulomb barrier energies and nucleosynthesis ends
- 4x10^10 s
Matter density becomes equal to radiation density
THE MATTER ERA
- 4x10^12 s
Electrons and protons recombine into hydrogen atoms
- 6x10^12 s
Photon decoupling
- 2x10^16 s
Formation of galaxies
- (X-1.4x10^17) s
Formation of the solar system
- (X-9.9x10^16) s
Emergence of life on Earth
- X ~ 4.7x10^17 s
Today
These values are rough estimates only. I have taken Omega_0=1, Lambda_0=0, and h=1.
- BS
- Annual Reviews of Astronomy and Astrophysics, 23, 322 by Boesgaard and Steigman
- HA
- Cosmology: The Science of the Universe by Harrison
- KT
- The Early Universe by Kolb and Turner