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Type Ia supernovae, standardizable candles, and gravity

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  • William Simcoe Wright
  • Baojiu Li
Type Ia supernovae (SNe Ia) are generally accepted to act as standardizable candles, and their use in cosmology led to the first confirmation of the as yet unexplained accelerated cosmic expansion. Many of the theoretical models to explain the cosmic acceleration assume modifications to Einsteinian general relativity which accelerate the expansion, but the question of whether such modifications also affect the ability of SNe Ia to be standardizable candles has rarely been addressed. This paper is an attempt to answer this question. For this we adopt a semianalytical model to calculate SNe Ia light curves in non-standard gravity. We use this model to show that the average rescaled intrinsic peak luminosity—a quantity that is assumed to be constant with redshift in standard analyses of Type Ia supernova (SN Ia) cosmology data—depends on the strength of gravity in the supernova’s local environment because the latter determines the Chandrasekhar mass—the mass of the SN Ia’s white dwarf progenitor right before the explosion. This means that SNe Ia are no longer standardizable candles in scenarios where the strength of gravity evolves over time, and therefore the cosmology implied by the existing SN Ia data will be different when analysed in the context of such models. As an example, we show that the observational SN Ia cosmology data can be fitted with both a model where (ΩMΛ)=(0.62,0.38) and Newton’s constant G varies as G (z) = G0(1+z)−1/4 and the standard model where (ΩMΛ)=(0.3,0.7) and G is constant, when the Universe is assumed to be flat.
Original languageEnglish
Article number083505
Number of pages22
JournalPhysical Review D
Volume97
Issue number8
DOIs
Publication statusPublished - 9 Apr 2018

Documents

  • PhysRevD.97.083505

    Rights statement: The final published version of this article Bill S. Wright and Baojiu Li., 'Type Ia supernovae, standardizable candles, and gravity' Phys. Rev. D. 97, 083505, can be located online at https://doi.org/10.1103/PhysRevD.97.083505. © 2018 American Physical Society.

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