VACUUM POLARIZATION BY FERMIONIC FIELDS IN HIGHER DIMENSIONAL COSMIC STRING SPACE-TIME

In this paper we investigate vacuum polarization effects associated with charged massive quantum fermionic fields in a six-dimensional cosmic string space-times considering the presence of a magnetic flux running along it score. We have shown that for specific values of the parameters which codify the presence of the cosmic string,and the fractional part of the ratio of the magnetic flux by the quantumone,a closed expression for the respective Green function is obtained. Adopting this result,we explicitly calculate the renormalized vacuum expectation value of the energy-momentum tensor, < T-B(A)> Ren, and analyse this result in some limiting cases.