Introduction to Cosmology Example Exam Question

Lecture 9: Inflation

In the context of the standard (pre-inflation) Big Bang model, explain what is meant by the following catch-phrases, and why they are described as "problems":
(i)   the horizon problem; [2]
(ii)  the flatness problem; [2]
(iii) the monopole problem. [2]
Briefly explain the term "inflation", and explain why introducing a period of inflation solves the above problems. [2]
Inflation is generally modelled as a large positive cosmological constant. Show that in this model the expansion factor of the universe during inflation is given by a(t) = a(ti) exp[H(t – ti)], where ti is the time that inflation starts. If we assume that inflation starts at 10-35 s, ends at 10-33 s, and involves 100 e-foldings of expansion, what is the implied value of the cosmological constant Λ? [3]

(2005 Resit Q5(a) and (c).)

Go to the hints and suggestions.