Inflationary parameters and primordial perturbation spectra

Details Inflationary parameters and primordial perturbation spectra Inflationary parameters and primordial perturbation spectra

2003-06-25

arxiv.org/abs/astro-ph/0306523v1

New Astron.Rev. 47 (2003) 781-786

Astronomy and Astrophysics

Astrophysics

10 pages, latex with elsart, no figures; to appear in New Astronomy Reviews, Proceedings of the CMBNET Meeting, 20-21 February

Scientific paper

I discuss how parameters describing inflation in the very early universe may be related to primordial perturbation spectra. Precision observations of anisotropies in the cosmic microwave background (CMB) such as those provided by the WMAP satellite offer an unprecedented window onto the physics of the very early universe. To theorists exploring speculative models of physics at high energies, the CMB offers us the chance to put our ideas to the test.

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