  For light and medium mass systems the capture cross-section may be considered
to be the same as that for complete fusion, whereas for heavy systems leading
to superheavy formations the evaporation residue cross-section is dramatically
reduced due to the quasifission (QF) and fusion-fission processes thus making
the capture cross-section to be essentially the sum of these two
cross-sections, with QF occurring at a much shorter time-scale. Consequently,
quasifission is the primary reaction mechanism that limits the formation of
superheavy nuclei. Within the last few years the time-dependent Hartree-Fock
(TDHF) approach has been utilized for studying the dynamics of quasifission.
The study of quasifission is showing a great promise to provide insight based
on very favorable comparisons with experimental data. In this article we will
focus on the TDHF calculations of quasifission observables for the
$^{48}$Ca+$^{249}$Bk system.
