Abstract
A rectifying curve \gamma in the Euclidean 3-space \mathbb{E}^3 is defined as a space curve whose position vector always lies in its rectifying plane (i.e., the plane spanned by the unit tangent vector field T_\gamma and the unit binormal vector field B_\gamma of the curve \gamma), and an f-rectifying curve \gamma in the Euclidean 3-space \mathbb{E}^3 is defined as a space curve whose f-position vector \gamma_f, defined by \gamma_f(s) = \int f(s) d\gamma, always lies in its rectifying plane, where f is a nowhere vanishing real-valued integrable function in arc-length parameter s of the curve \gamma. In this paper, we introduce the notion of f-rectifying curves which are null (lightlike) in the Minkowski 3-space \mathbb{E}^3_1. Our main aim is to characterize and classify such null (lightlike) f-rectifying curves having spacelike or timelike rectifying plane in the Minkowski 3-Space \mathbb{E}^3_1.