Alternate Models to Dark Energy
Kenath Arun (1, 2), S B Gudennavar (1), A Prasad (3), C Sivaram (4), ((1) Department of Physics, Christ University, Bengaluru-560029, Karnataka,, India, (2) Department of Physics, Christ Junior College, Bengaluru-560029,, Karnataka, India, (3) Udaipur Solar Observatory

TL;DR
This paper proposes alternative models to explain the universe's accelerated expansion observed through Type Ia supernovae, challenging the dark energy paradigm in cosmology.
Contribution
It introduces new models that account for supernovae data without relying on dark energy, offering a different perspective on cosmic acceleration.
Findings
Models successfully fit supernovae data without dark energy
Provides a potential alternative explanation for cosmic acceleration
Challenges the necessity of dark energy in cosmological models
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.
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