Microwave Background Anisotropies Induced by Global Scalar Fields: The Large N Limit

Details Microwave Background Anisotropies Induced by Global Scalar Fields: The Large N Limit Microwave Background Anisotropies Induced by Global Scalar Fields: The Large N Limit

1996-12-20

arxiv.org/abs/astro-ph/9612202v1

Phys.Rev.D55:4516-4520,1997

Astronomy and Astrophysics

Astrophysics

11 pages Latex, 5 postscript figures included

Scientific paper

10.1103/PhysRevD.55.R4516

We present an analysis of CMB anisotropies induced by global scalar fields in the large N limit. In this limit, the CMB anisotropy spectrum can be determined without cumbersome 3D simulations. We determine the source functions and their unequal time correlation functions and show that they are quite similar to the corresponding functions in the texture model. This leads us to the conclusion that the large N limit provides a 'cheap approximation' to the texture model of structure formation.

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