The Second Peak: CDM or No CDM?

Details The Second Peak: CDM or No CDM? The Second Peak: CDM or No CDM?

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...197.5506m&link_type=abstract

American Astronomical Society, 197th AAS Meeting, #55.06; Bulletin of the American Astronomical Society, Vol. 32, p.1496

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The amplitude of the second peak in the angular power spectrum of the cosmic microwave background radiation is constrained to be small by recent experiments like Boomerang. This is surprising in the context of the Λ CDM model, which predicted a large second peak. However, this result is expected if CDM does not exist. The observed shape of the power spectrum was accurately predicted (before the fact) by a model motivated by the surprising recent successes of the modified dynamics (MOND) hypothesized by Milgrom. The author is supported in part by NSF grant AST 99-01663.

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