摘要
We investigate the imprints of memory-burdened primordial black holes (PBH) on the global 21 cm signal during the cosmic dawn. Recent studies reopened the possibility of a mass window of PBHs as a compelling candidate for dark matter, particularly in low-mass regimes ( M PBH < 10 15 g) where conventional constraints from evaporation are being revisited in light of quantum gravitational effects. One such effect, the memory burden effect , slows down black hole evaporation by incorporating the backreaction of radiation on the black hole microstates, substantially extending the lifetime of light PBHs and thus modifying their late-time emission spectra. This prolonged emission can dramatically alter the energy injection history in the early universe. By computing the modified energy injection rates into the intergalactic medium and incorporating them into the thermal and ionization evolution of neutral hydrogen, we obtain projected constraints on the fraction of dark matter. The bounds are obtained from the fact that these low mass PBHs, which were thought otherwise evaporated, can modify the absorption amplitude in the global 21-cm signal at redshift z ≈ 17. Considering the two viable scenarios of transition to the memory-burden phase: fast (or instantaneous) and slow (transition with a finite width), we show how the 21 cm bounds are sensitive to different mass ranges. For a broad transition with δ = 10 -2 we find that PBHs in the mass range M PBH ≃ 10 8 –10 13 g are excluded at the level of f PBH ≳ 10 -8 . In contrast, for a fast-transition case with the lowest suppression exponent k = 1, the evaporation is suppressed so efficiently that no meaningful 21 cm constraint remains for M PBH ≳ 10 7 g.