| Abstract: In my talk, I will introduce the cosmological perturbation theory. First of all, I will start with gravitational field equation in the presence of perturbations. Then I will introduce scalar, vector and tensor decomposition (irreducible representations). The concept of gauge invariant quantities is another important part which will be covered in my talk. Finally, I will briefly study solutions of the perturbation equations for special cases.
Time: Thursday, July 4, 2013 at 11:00 in Larak Seminar Room
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