Space and astrophysical plasmas typically possess particle distributio
n functions with a power-law tail (in energy) that are well modeled by
generalized Lorentzian distributions with an associated spectral inde
x kappa. Dispersion equations for linear waves of any mode in a plasma
described by a Lorentzian-type particle distribution involve the modi
fied plasma dispersion function Z(kappa), a special function analogou
s to the plasma dispersion function Z that arises when the particle di
stribution is Maxwellian. The function Z(kappa), originally defined b
y Summers and Thorne [Phys. Fluids B 3, 1835 (1991)] for integral valu
es of kappa, was recently generalized to real values of kappa by Mace
and Hellberg [Phys. Plasmas 2, 2098 (1995)]. In the present paper, a g
eneral formula is derived for the modified plasma dispersion function
Z(kappa) corresponding to half-integral values of kappa, and simple,
explicit closed-form expressions are given for the functions Z(3/2),
Z(5/2), Z(7/2)*, Z(9/2)*, and Z(11/2)*. These results complement the
simple, closed-form expressions for the functions Z(kappa), for kappa
=1, 2, 3,..., that already exist in the literature. (C) 1996 American
Institute of Physics.