Abstract

Main predictions of the baryon isocurvature model for structure formation are reproduced if the primeval entropy per baryon is constant and homogeneity is broken by a clumpy distribution of seed masses. The constant entropy per baryon may reconcile the cosmogony with the standard model for the origin of the light elements. The seeds could be long-lived cosmic field structures or inhomogeneously produced nonbaryonic cold dark matter, if the needed primeval space distribution could be arranged. The constraints from the large-scale distributions of galaxies and the thermal cosmic background radiation require a {OMEGA} ~ 0.1. In some cases the primeval seed rms mass constrast δρ_c_/ρ_c_ exceeds unity on the scale of clusters of galaxies, meaning the fluctuations cannot be Gaussian, which could permit cluster formation in a low-density universe.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.