Alternate Models to Dark Energy
arXiv:1708.09269 · doi:10.1016/j.asr.2017.08.006
Abstract
One of the unresolved questions currently in cosmology is that of the non-linear accelerated expansion of the universe. This has been attributed to the so called Dark Energy (DE). The accelerated expansion of the universe is deduced from measurements of Type Ia supernovae. Here we propose alternate models to account for the Type Ia supernovae measurements without invoking dark energy.
9 pages, 3 figures, 1 table
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Cited by in corpus (5)
- Effects of dark matter in star formation
- Dark Energy Constraints on Masses and Sizes of Large Scale Cosmic Structures
- Constraining Temporal Oscillations of Cosmological Parameters Using Type Ia Supernovae
- Effects of Dark Matter in Red Giants
- Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars