Abstract Recently, the mean free path of ionizing photons in z = 6 intergalactic medium (IGM) was measured to be very short, presenting a challenge existing reionization models. At face value, measurement can interpreted as evidence that IGM clumps on scales M ≲ 10 8 ⊙ , key but largely untested prediction cold dark matter (CDM) paradigm. Motivated by this possibility, we study role underlying ...