Generation of isothermal density perturbations in the inflationary universe

Physics

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Scientific paper

It is shown that not only adiabatic perturbations of the density but also isothermal density perturbations are generated in the inflationary universe. The magnitude of isothermal perturbations can be sufficiently large for the subsequent galaxy formation. The spectrum of isothermal perturbations can differ considerably from a flat one.
I am grateful to G.V. Chibisov, A.G. Doroshkevich, M.Yu. Khlopov, L.A. Kofman, V.F. Mukhanov, I.D. Novikov, A.A. Starobinsky and Ya.B. Zeldovich for many useful and stimulating discussions.

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