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      Comments on: "Almost All Carbon/Oxygen White Dwarfs Can Support Double Detonations"

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          Abstract

          I critically review some claims in the paper ``Almost All Carbon/Oxygen White Dwarfs Can Support Double Detonations'' (arXiv:2405.19417). The claim of that paper that the community converges on a leading scenario of type Ia supernovae (SNe Ia), the double detonation scenario, is wrong, as hundreds of papers in recent years study five and more different SN Ia scenarios and their channels. Moreover, the finding by that paper that the double detonation scenario with the explosion of the secondary white dwarf (WD; the mass-donor WD) is common, i.e., the triple-detonation channel and the quadruple-detonation sub-channel, implies highly no-spherical explosions. The highly non-spherical explosions contradict the morphologies of many SN Ia remnants. I find that the results of that paper strengthen the claim that the double detonation scenario (with its channels) might account for a non-negligible fraction of peculiar SNe Ia but only for a very small fraction (or non at all) of normal SNe Ia.

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          Journal
          11 June 2024
          Article
          2406.07363
          47e812cf-5fca-4e61-915c-1cf2096fe97e

          http://creativecommons.org/licenses/by/4.0/

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          Four-pages comments on arXiv:2405.19417
          astro-ph.HE

          High energy astrophysical phenomena
          High energy astrophysical phenomena

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