4.7 Article

JWST early Universe observations and Lambda CDM cosmology

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 524, Issue 3, Pages 3385-3395

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stad2032

Keywords

galaxies: high-redshift; cosmology: early Universe, dark energy, cosmological parameters

Ask authors/readers for more resources

Deep space observations of the JWST suggest that very early Universe galaxies may be as evolved as galaxies that have existed for much longer, which contradicts the Lambda CDM cosmological model. While tired light models explain the JWST data, they don't account for other observations like isotropy of the cosmic microwave background. Hybrid models that combine tired light and Lambda CDM have been proposed, with covarying coupling constants and yielding a stretched age of the Universe that resolves the "impossible early galaxy" problem.
Deep space observations of the JWST have revealed that the structure and masses of very early Universe galaxies at high redshifts (z similar to 15), existing at similar to 0.3 Gyr after the Big Bang, may be as evolved as the galaxies in existence for similar to 10 Gyr. The JWST findings are thus in strong tension with the Lambda CDM cosmological model. While tired light (TL) models have been shown to comply with the JWST angular galaxy size data, they cannot satisfactorily explain isotropy of the cosmic microwave background (CMB) observations or fit the supernovae distance modulus versus redshift data well. We have developed hybrid models that include the tired light concept in the expanding universe. The hybrid Lambda CDM model fits the supernovae type 1a data well but not the JWST observations. We present a model with covarying coupling constants (CCC), starting from the modified FLRW metric and resulting Einstein and Friedmann equations, and a CCC + TL hybrid model. They fit the Pantheon + data admirably, and the CCC + TL model is compliant with the JWST observations. It stretches the age of the Universe to 26.7 Gyr with 5.8 Gyr at z = 10 and 3.5 Gyr at z = 20, giving enough time to form massive galaxies. It thus resolves the 'impossible early galaxy' problem without requiring the existence of primordial black hole seeds or modified power spectrum, rapid formation of massive population III stars, and super Eddington accretion rates. One could infer the CCC model as an extension of the Lambda CDM model with a dynamic cosmological constant.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.7
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available