Slide 1Dr Martin Hendry University of Glasgow Slide 2 Why are we here?…. The period of inflation in the very early Universe was invoked to explain some apparent fine tuning…
Modern CosmologyChapters 1-6Ed Copeland1 and Costas Skordis2School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, UKAbstractThese lecture notes cover…
Baryon density of the Universe : a trace of a scalar field? Reaction rate : G (T, h10)=Cross section (T) × number densities(h10,T) Thermal equilibrium : G/H > 1 Frozen…