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The recent discoveries of a remarkable glitch/antiglitch accompanied by fastradio burst (FRB)-like bursts from the Galactic magnetar SGR J1935+2154 haverevealed the physical connection between the two. In this work, we study thestatistical properties of radio bursts from the hyperactive repeating sourceFRB 20201124A and of glitches from the pulsar PSR B1737--30. For FRB 20201124A,we confirm that the probability density functions of fluctuations of energy,peak flux, duration, and waiting time well follow the Tsallis q-Gaussiandistribution. The derived q values from q-Gaussian distribution keepapproximately steady for different temporal interval scales, which indicatethat there is a common scale-invariant structure in repeating FRBs. Similarscale-invariant property can be found in PSR B1737--30's glitches, implying anunderlying association between the origins of repeating FRBs and pulsarglitches. These statistical features can be well understood within the samephysical framework of self-organized criticality systems.

Scale-invariant Phenomena in Repeating Fast Radio Bursts and Glitching Pulsars