Korunur, M.Salti, M.Aydogdu, O.2024-04-242024-04-2420071434-60441434-6052https://doi.org/10.1140/epjc/s10052-006-0195-1https://hdl.handle.net/11468/17817An axially symmetric scalar field is considered in teleparallel gravity. We calculate, respectively, the tensor, the vector and the axial-vector parts of torsion and energy, momentum and angular momentum in the ASSF. We find the vector parts are in the radial and (e) over cap (theta) directions, the axial-vector, momentum and angular momentum vanish identically, but the energy distribution is different from zero. The vanishing axial-vector part of torsion gives us the result that there occurs no deviation in the spherical symmetry of the spacetime. Consequently, there exists no inertia field with respect to a Dirac particle, and the spin vector of a Dirac particle becomes constant. The result for the energy is the same as obtained by Radinschi. Next, this work also (a) supports the viewpoint of Lessner that the Moller energy-momentumcomplex is a powerful concept for the energy-momentum, (b) sustains the importance of the energy-momentum definitions in the evaluation of the energy distribution of a given spacetime, and (c) supports the hypothesis by Cooperstock that the energy is confined to the region of non-vanishing energy-momentumtens or of the matter and all non-gravitational fields.eninfo:eu-repo/semantics/openAccess[No Keyword]An axially symmetric scalar field and teleparallelismAn axially symmetric scalar field and teleparallelismArticle501101107WOS:0002490101000122-s2.0-3394741614610.1140/epjc/s10052-006-0195-1Q1Q2