Alternate Models to Dark Energy

2); (2) Department of Physics; (3) Udaipur Solar Observatory; (4) Indian Institute of Astrophysics; A Prasad (3); Bari Road; Bengaluru-560029; Bengaluru-560034; Christ Junior College; Christ University

arxiv: 1708.09269 · v1 · pith:GW4CTNUMnew · submitted 2017-08-21 · ⚛️ physics.gen-ph

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

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India (2) Department of Physics Christ Junior College (3) Udaipur Solar Observatory Physical Research Laboratory Dewali Bari Road Udaipur 313001 (4) Indian Institute of Astrophysics Bengaluru-560034 India)

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classification ⚛️ physics.gen-ph

keywords darkenergyacceleratedalternateexpansionmeasurementsmodelssupernovae

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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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Alternate Models to Dark Energy

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