one hypothesis is that an oxygen-neon white dwarf won't accrete fast enough to reach explosive oxygen ignition temperature because of rapid neutrino cooling https://arxiv.org/pdf/1710.04417.pdf …
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models suggest that under the right conditions, carbon flares will occur but not large enough to actually cause mass loss, allowing the WD to burn accreted helium while continuing to grow https://arxiv.org/pdf/1706.03843.pdf …
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they're apparently a very interesting possible NS creation pathway, with possible implications for pulsar populations (ex: millisecond pulsar formation). https://sci-hub.tw/10.1111/j.1365-2966.2009.15988.x …
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