WMAP tend to coincide with radio emissions from the Milky Way

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SUMMARY

The discussion centers on the controversial claims made by physicist Gerrit L. Verschuur regarding the temperature variations observed in the WMAP (Wilkinson Microwave Anisotropy Probe) data. Verschuur argues that these variations are linked to radio emissions from neutral hydrogen in the Milky Way, challenging the prevailing view that they are evidence of early universe density perturbations. However, Richard Lieu and his team conducted a wavelet analysis comparing WMAP data with HI (neutral hydrogen) clouds and found no statistically significant associations, thereby refuting Verschuur's claims.

PREREQUISITES
  • Understanding of cosmic microwave background (CMB) radiation
  • Familiarity with WMAP (Wilkinson Microwave Anisotropy Probe) data analysis
  • Knowledge of neutral hydrogen (HI) in astrophysics
  • Experience with wavelet analysis techniques in data comparison
NEXT STEPS
  • Research the implications of WMAP findings on cosmological models
  • Study wavelet analysis methods in astrophysical data interpretation
  • Explore the role of neutral hydrogen in cosmic structure formation
  • Examine critiques of Gerrit L. Verschuur's theories in astrophysics literature
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Astronomers, astrophysicists, and researchers interested in cosmic microwave background studies, as well as those analyzing the relationship between interstellar hydrogen and cosmic radiation.

jal
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Have these papers been discused.
http://arxiv.org/abs/0704.1125
High Galactic Latitude Interstellar Neutral Hydrogen Structure and Associated (WMAP) High Frequency Continuum Emission
Authors: Gerrit L. Verschuur
(Submitted on 9 Apr 2007 (v1), last revised 23 Jul 2007 (this version, v2))

Tiny temperature variations found in maps of the cosmic microwave background are commonly thought to be proof that stars, galaxies and other large-scale structures grew from density perturbations in the early universe. But one physicist in the US is controversially claiming that these observed variations are in fact caused by hydrogen atoms in our own galaxy. If he is right, cosmologists will have to drastically rethink their models of the universe’s evolution.
Gerrit Verschuur, a physicist from the University of Memphis in the US, disagrees. He has noticed that the temperature variations recorded by WMAP tend to coincide with radio emissions from neutral hydrogen in the Milky Way. In other words, the fluctuations may not be part of the CMB at all (Astro. J. in publication; preprint available at arXiv.org:0704.1125v2).

http://arxiv.org/abs/0704.3021
On the Critical Ionization Velocity Effect in Interstellar Space and Possible Detection of Related Continuum Emission
Authors: Gerrit L. Verschuur
(Submitted on 23 Apr 2007)
 
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An interesting paper, but also read this discussion in the CosmoCoffee forum , which concluded with this post by Richard Lieu (University of Alabama, Huntsville, Position: Professor of Physics,
Research Interests:clusters of galaxies & cosmology):
I performed an extensive study (with B. Z. Jiang, a PhD student of Prof. S.N. Zhang at Tsinghua, Beijing) using wavelet analysis of the WMAP and HI data, then cross comparing the number of close associations between the degree-scale wavelet hot spot centroids and HI clouds with that expected from simulated WMAP data where the hot spot locations are by definition randomized.

The verdict is that we found no statistically significant associations between the first acoustic peak hot spots and HI. We therefore cannot support the claim of Verschuur.

Garth
 
Last edited:
For a laugh, you could also read v1 of the Verschuur paper (I think it's still available on arXiv), it contains some real howlers ...
 

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