Anisotropic compact stars: Constraining model parameters to account for physical features of tidal Love numbers

In this paper, we develop a new class of models for compact star with anisotropic stresses inside the matter distribution. By assuming linear equation state composition solve Einstein field equations. our approach, interior solutions use particular form ansatz metric function $g_{rr}$. The exterior solution is assumed as Schwarzschild and joined obtained across boundary star. These matching metrices along condition vanishing radial pressure at lead us to determine model parameters. physical acceptability has verified by making current estimated data available from pulsar 4U1608-52. Thereafter, anisotropy due tidal effects calculate Love numbers compare results observed stars, viz. KS 1731- 260,4U 1608- 52,4U 1724- 207,4U 1820- 30,SAX J1748.9-2021 EXO 1745-268. overall situation confirms viability proposed approach,which can shed light on relativistic objects.