Supersymmetric In ation and Large - scale Structure
نویسنده
چکیده
In e ective supergravity theories following from the superstring, a modulus eld can quite naturally set the neccessary initial conditions for successful cosmological in ation to be driven by a hidden sector scalar eld. The leading term in the scalar potential is cubic hence the spectrum of scalar density perturbations neccessarily deviates from scale-invariance, while the generation of gravitational waves is negligible. The growth of large-scale structure is then consistent with observational data assuming a critical density cold dark matter universe, with no need for a component of hot dark matter. The model can be tested thorough measurements of cosmic microwave background anisotropy on small angular scales. Invited talk at the Inauguration Conference of the Asia-Paci c Center for Theoretical Physics, Seoul (June 4-10, 1996) Typeset using REVTEX Work done in collaboration with J.A. Adams & G.G. Ross [1]
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تاریخ انتشار 1996