Evanescent modes of the electromagnetic field are seldom invoked in convent
ional far-field optics, as their contribution far from the source (a few wa
velengths) is negligible. Contradicting this fact, in recent theoretical wo
rks, based on a particular decomposition of the free-space Green tensor, it
has been asserted that evanescent waves do indeed contribute to the far fi
eld, where they appear as an additional similar to 1/r component of the fie
ld. We provide an explicit demonstration that evanescent modes do not contr
ibute to the power radiated to the far field by any dipolar source. First w
e derive an expression for the free-space field susceptibility in which con
tributions from evanescent and homogeneous modes are separated, and then we
use linear response theory to compute the decay rate for an atomic dipole
in vacuum. (C) 2000 Optical Society of America OCIS codes: 260.2510, 350.56
10.