  Model building within the Randall-Sundrum (RS) framework generally involves
placing the Standard Model fields in the bulk. Such fields may possess non-zero
values for their associated brane-localized kinetic terms (BLKTs) in addition
to possible bulk mass parameters. In this paper we clearly identify the regions
of the RS model parameter space where the presence of bulk mass terms and BLKTs
yield a setup which is free from both ghost and tachyon instabilities. Such
physically acceptable parameter space regions can then be used to construct
realistic and phenomenologically viable RS models.
