The zero-temperature effective equation of motion is derived for a scalar h
eld interacting with other fields. For a broad range of cases, involving in
teraction with as few as one or two fields, dissipative regimes are found f
or the scalar field system. The zero-temperature limit constitutes a baseli
ne effect that will be prevalent in any general statistical state. Thus, th
e results found here provide strong evidence that dissipation is the norm n
ot the exception for an interacting scalar field system. For application to
inflationary cosmology, this provides convincing evidence that warm inflat
ion could be a natural dynamics once proper treatment of the interactions i
s done. The results found here also may have applicability to entropy produ
ction during the chiral phase transition in heavy-ion collision.