Ascertain the value of the memory burden suppression parameter k
Ascertain the physical value of the parameter k that quantifies the suppression of the evaporation rate due to the memory burden effect in primordial black holes, where the emission rate beyond half-decay is reduced by a factor proportional to S(qM0)^{-k} relative to the semiclassical rate; determine k from first-principles theory or observational inference to enable definitive constraints on the primordial black hole dark matter fraction.
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References
Here, we compute the bounds on the dark matter fraction of PBHs as a function of the currently unknown parameter k that quantifies the strength of the memory burden effect.
— Breakdown of Hawking Evaporation opens new Mass Window for Primordial Black Holes as Dark Matter Candidate
(2402.17823 - Thoss et al., 27 Feb 2024) in Section 4 (Summary and Conclusions)