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• W3201588617 endingPage "110" @default.
• W3201588617 startingPage "110" @default.
• W3201588617 abstract "Abstract Observational signatures of the circumstellar material (CSM) around Type Ia supernovae (SNe Ia) provide a unique perspective on their progenitor systems. The pre-supernova evolution of the SN progenitors may naturally eject CSM in most of the popular scenarios of SN Ia explosions. In this study, we investigate the influence of dust scattering on the light curves and polarizations of SNe Ia. A Monte Carlo method is constructed to numerically solve the process of radiative transfer through the CSM. Three types of geometric distributions of the CSM are considered: spherical shell, axisymmetric disk, and axisymmetric shell. We show that both the distance of the dust from the SN and the geometric distribution of the dust affect the light curve and color evolutions of SN. We found that the geometric location of the hypothetical circumstellar dust may not be reliably constrained based on photometric data alone, even for the best observed cases such as SN 2006X and SN 2014J, due to the degeneracy of CSM parameters. Our model results show that a time sequence of broadband polarimetry with appropriate time coverage from a month to about one year after explosion can provide unambiguous limits on the presence of circumstellar dust around SNe Ia." @default.
• W3201588617 created "2021-09-27" @default.
• W3201588617 creator A5010642871 @default.
• W3201588617 creator A5046871799 @default.
• W3201588617 creator A5087929908 @default.
• W3201588617 date "2022-06-01" @default.
• W3201588617 modified "2023-10-03" @default.
• W3201588617 title "The Effects of Circumstellar Dust Scattering on the Light Curves and Polarizations of Type Ia Supernovae*" @default.
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• W3201588617 doi "https://doi.org/10.3847/1538-4357/ac6be5" @default.
• W3201588617 hasPublicationYear "2022" @default.
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