Time-line in an INFLATIONARY BIG BANG COSMOLOGY

Time (s)       T  (Kelvin) Reference  Event
                CBR

THE QUANTUM GRAVITY ERA


1x10^-43       1x10^32     KT 72      Quantum limit of classical general

                                      relativity



THE INFLATION AND SYMMETRY BREAKING ERA




1x10^-38       1x10^29     KT 72      Limit of perturbative interaction

                                      thermalization of universe

1x10^-35       1x10^28     KT 72      Grand unification spontaneous

                                      symmetry breaking

1x10^-34       1x10^27     KT 274     Approximate start of inflation

1x10^-32       1x10^27     KT 274     Approximate start of reheating and

                                      end of inflation

1x10^-11       3x10^15     KT 72      Electroweak unification spontaneous

                                      symmetry breaking



THE QUARK-LEPTON ERA




2x10^-7        2x10^13    HA 353      Tauon anti-tauon annihilation

1x10^-5        2x10^12    KT 72       Formation of hadrons from quarks

7x10^-5        1x10^12    HA 353      Muon anti-muon annihilation

5x10^-4        4x10^11    KT 159, 281 By this time the universe has a

                                      baryon-antibaryon asymmetry

                                      which results from post-inflationary

                                      B,C,CP violating processes

1x10^-1        3x10^10    BS          Neutral current weak interactions

                                      become too slow and neutrinos

                                      decouple

1x10^0         1x10^10    BS          Charged current weak interactions

                                      become too slow and neutron to

                                      proton ratio freezes out

1x10^1         5x10^9     BS          Electron positron annihilation



THE RADIATION ERA




1x10^2         1x10^9     BS          Typical photon energies drop below

                                      the deuteron binding energy and

                                      nucleosynthesis begins

1x10^3         4x10^8     BS          Particle energies drop below coulomb

                                      barrier energies and nucleosynthesis

                                      ends

4x10^10        6x10^4     KT 77       Matter density becomes equal to

                                      radiation density



THE MATTER ERA




4x10^12        3.5x10^3   KT 78       Electrons and protons recombine into

                                      hydrogen atoms

6x10^12        3.0x10^3   KT 80       Photon decoupling

2x10^16        20         HA 349      Formation of galaxies

(X-1.4x10^17)  ---        KT 12       Formation of the solar system

(X-9.9x10^16)  ---        HA 390      Emergence of life on Earth

X ~ 4.7x10^17  2.726      KT 12       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