Machine Learning Identification of Gravimentally Microlensed Gamma-Ray Bursts

Gravitational microlensing of gamma-ray bursts (GRBs) provides a unique opportunity to probe compact dark matter and small-scale structures in the universe. However, identifying such microlensed GRBs within large datasets is a significant challenge. In this study, we develop a machine learning approach to distinguish Lensed GRBs from their Non-lensed counterparts using simulated light curves. A comprehensive dataset was generated, comprising labeled light curves for both categories. Features were extracted using the Cesium package, capturing critical temporal properties of the light curves. Multiple machine learning models were trained on the extracted features, with Random Forest achieving the best performance, delivering an accuracy of 94\% and an F1 score of 95\% (94\%) for Non-Lensed (Lensed) class. This approach successfully demonstrates the potential of machine learning for identifying gravitational lensing in GRBs, paving the way for future observational applications.