The decreasing long-duration waiting-time peaks of FRBs 20121102A and 20201124A are attributed to orbital decay of eccentric neutron star-white dwarf binaries through stable or unstable mass transfer and common-envelope ejection.
[The CHIME/FRB Collaboration]
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Reconciling the Waiting Time Peaks Variations of Repeating FRBs with an Eccentric Neutron Star--White Dwarf Binary
The decreasing long-duration waiting-time peaks of FRBs 20121102A and 20201124A are attributed to orbital decay of eccentric neutron star-white dwarf binaries through stable or unstable mass transfer and common-envelope ejection.