What value is expected for baryon to photon density?

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SUMMARY

The observed baryon to photon density is approximately 6.1 x 10-10, which is considered too small according to current cosmological standards. The expected ratio remains uncertain, as precision measurements have not yet led to a comprehensive theoretical framework to predict baryon density accurately. Key references include the WMAP parameters table and the Particle Data Group's review of cosmological parameters, both of which highlight the challenges in understanding baryon density within the context of precision cosmology.

PREREQUISITES
  • Understanding of baryon and photon densities in cosmology
  • Familiarity with precision cosmology concepts
  • Knowledge of the WMAP parameters and their implications
  • Basic grasp of theoretical frameworks in astrophysics
NEXT STEPS
  • Research the latest findings on baryon density from the WMAP mission
  • Explore the implications of baryon to photon ratios in cosmological models
  • Study the Particle Data Group's reviews on cosmological parameters for updated insights
  • Investigate the role of dark matter and neutrinos in baryon density calculations
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Astronomers, cosmologists, and astrophysicists interested in the fundamental properties of the universe and the ongoing challenges in understanding baryon and photon interactions.

arroy_0205
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It is generally stated that observed baryon to photon density (about 6.1x10^(-10)) is too small. What is the reason? What ratio is expected?
 
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http://lambda.gsfc.nasa.gov/product/map/pub_papers/firstyear/basic/wmap_params_table.pdf

This paper confirms your number of 6.1 * 10^(-1).

http://pdg.lbl.gov/2012/reviews/rpp2012-rev-cosmological-parameters.pdf

"A typical collection would be baryons, photons, neutrinos, and
dark matter (given charge neutrality, the electron density is guaranteed to be too small
to be worth considering separately and is included with the baryons)."

This would appear to answer your question as to whether or not it is commonplace to claim the ratio to be too small.

As for your question about what ratio is expected, I think my first link should suffice, but as to why this is so, I am not knowledgeable enough to know. I just used google and spent twenty minutes or so reading through papers.

"Even the baryon density, now measured to an accuracy of a few percent, lacks an underlying theory able to predict it even within orders of magnitude. Precision cosmology may have arrived, but at present many key questions remain to motivate and challenge the cosmology community." - (second link)

This article was updated June 18th, 2012, so that would lead to suggest some uncertainty in regards to our understanding of baryons and photons.
 
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https://en.wikipedia.org/wiki/MoM-z14 Any photon with energy above 24.6 eV is going to ionize any atom. K, L X-rays would certainly ionize atoms. https://www.scientificamerican.com/article/whats-the-most-distant-galaxy/ The James Webb Space Telescope has found the most distant galaxy ever seen, at the dawn of the cosmos. Again. https://www.skyatnightmagazine.com/news/webb-mom-z14 A Cosmic Miracle: A Remarkably Luminous Galaxy at zspec = 14.44 Confirmed with JWST...

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