New Results from Using Inhomogeneous Cosmological Models in an Era of Precision Cosmology Observations

Details New Results from Using Inhomogeneous Cosmological Models in an Era of Precision Cosmology Observations New Results from Using Inhomogeneous Cosmological Models in an Era of Precision Cosmology Observations

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21931203i&link_type=abstract

American Astronomical Society, AAS Meeting #219, #312.03

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We use general Szekeres inhomogeneous cosmological models (i.e. not spherically symmetric and not axially symmetric) in order to derive observable functions such as cosmological distances and redshift. We also derive growth rate equations for some sub-cases. We will discuss some of our recent results using these new frameworks and show how they can offer new interpretations of the cosmological data. The results can have interesting implications for dark matter, dark energy, and large scale structure formation. This work is supported by a grant from NASA.

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