“…Prime examples [4] of dissipation by reconnection occur in astrophysical plasmas (such as solar flares [5,6] and magnetic substorms [7,8]) and sawtooth crashes in fusion devices [9], where magnetic energy is dissipated by the acceleration of nearby particles [10,11,12,13,14]. Reconnection has also been studied in liquid crystals [2], superconductors [3,15,16], cosmic strings [17], viscous [18,19,20] and Euler [21] vortices, Bose-Einstein condensates [22] and superfluids [23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38]. * The authors of this manuscript would not be studying this subject were it not for the influence and collaboration of K.R.…”