Implications of MAX for CDM
Astrophysics
2008-11-26 v1 High Energy Physics - Phenomenology
Abstract
We analyze the Gamma Ursae Minoris (GUM) and Mu Pegasii (MuP) scans of the Millimeter-wave Anisotropy eXperiment in the context of cold dark matter (CDM) models of structure formation, paying particular attention to the two-dimensional nature of the GUM scan. If all of the structure in the (foreground subtracted) data is attributed to cosmic microwave background anisotropy, then there is a detection in each scan. For a standard CDM model, the amplitudes of the signals are individually compatible with the COsmic Background Explorer measurement, but marginally inconsistent with each other.
Keywords
Cite
@article{arxiv.astro-ph/9309006,
title = {Implications of MAX for CDM},
author = {Mark Srednicki and Martin White and Douglas Scott and Emory T. Bunn},
journal= {arXiv preprint arXiv:astro-ph/9309006},
year = {2008}
}
Comments
10 pages in Plain TeX + 3 PS figures, CfPA-93-TH-27