  In this paper, we explore the energy-momentum distribution of locally
rotationally symmetric (LRS) spacetimes in the context of the teleparallel
theory of gravity by considering the three metrics, I, II and III, representing
the whole class of LRS sapcetimes. In this regard, we use the teleparallel
versions of the Einstein, Landau-Lifshitz, Bergmann-Thomson, and
M$\ddot{o}$ller prescriptions. The results show that the momentum density
components for the Einstein, Bergmann-Thomson, and M$\ddot{o}$ller
prescriptions turn out to be same in all cases of the metrics I, II and III,
but are different from those of the Landau- Lifshitz prescription, while the
energy components remain the same for these three prescriptions only in all
possible cases of the metrics I and II. We mention here that the
M$\ddot{o}$ller energy-momentum distribution is independent of the coupling
constant $\lambda$; that is, these results are valid for any teleparallel
models.
