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Comments on: "Almost All Carbon/Oxygen White Dwarfs Can Support Double Detonations"
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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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Cited by 1 Pith paper
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A double-degenerate scenario with a merger to explosion delay time to explain type Ia supernova SN 2020aeuh
The author proposes that SN 2020aeuh's early carbon-oxygen circumstellar interaction is the delayed explosion of a merged white dwarf, about one to two years after the merger.
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