“…The two best developed models currently available are the BFKL pomeron [ 6], calculated within the leading logarithmic approximation (LLA) by Mueller and Tang [ 7] and implemented into the HERWIG Monte Carlo [ 8,9], and the soft colour rearrangement model [ 10]. The recent gaps between jets analysis by the D0 Collaboration [ 1] favoured the soft colour model to the BFKL pomeron, although conclusions from gaps between jets measurements may be difficult to draw due to the uncertainties in the role of multiple interactions, which are poorly understood theoretically at the present time [ 11,12]. Furthermore, gaps between jets measurements at both HERA and the TEVA-TRON are limited by the requirement that two jets are observed in the detector, severely restricting the accessible gap size.…”