The primary damage by displacement cascades in 3C-SiC at 300 K has been stu
died by molecular dynamics (MD). A large number of cascades, with energies
from 0.2 to 50 keV, have been simulated in order to investigate the effects
of energy in defect production and clustering. The surviving defects are d
ominated by C interstitials and vacancies. The number of Frenkel pairs incr
eases with increasing cascade energy, but the efficiency of their productio
n declines with increasing energy in a similar fashion to that found in met
als. Although the number of antisite defects is smaller than that of Frenke
l pairs, their production also increases with increasing cascade energy. Mo
st surviving defects are single interstitials and vacancies, and the tenden
cy of interstitials to form clusters is very week. The size of the intersti
tial clusters is very small, which shows significantly different behavior t
han obtained by MD simulations in metals. The current results provide the s
tatistics of the primary damage states in SiC as a function of primary knoc
k-on energy, which are important in upscaling these results to model behavi
or over longer time and length scales.