The yields of neutrons and the spatial distributions of radionuclides
generated by neutrons in hadronic cascades are computed. Simulation th
at employs the SHIELD code is based on the Dubna version of the cascad
e model for describing hadron-nucleus interactions and on the quark-gl
uon string model for describing interactions of high-energy particles.
Cascade arising from interactions between negative pions with energie
s in the range 0.3-10.0 GeV and nuclei in water are considered. A code
simulating nuclear deexcitation is used to take into account Fermi br
eakup, multifragmentation, and evaporation (or fission). Neutron trans
port is included in the analysis through the original algorithm LOENT.
More than 50% of neutrons and radionuclides generated by them are dis
tributed at distances greater than 0.57 m form the shower core. The re
sults may be used to estimated background due to cosmic muons in exper
imental searches for rare and hypothetical processes.