Abstract
Gravitational waves, ripples in the fabric of spacetime predicted by Einstein’s theory of general relativity, have emerged as a transformative tool for modern astrophysics. Their direct detection by LIGO in 2015 confirmed a century-old prediction and opened a new observational window into the cosmos. Unlike electromagnetic radiation, gravitational waves travel virtually unimpeded through matter, carrying pristine information from the most energetic events in the universe—such as black hole mergers and neutron star collisions. This article explores the theoretical foundation, detection methodologies, and astrophysical implications of gravitational waves. It further examines their role in probing fundamental physics, including tests of general relativity, the nature of compact objects, and the early universe.

This work is licensed under a Creative Commons Attribution 4.0 International License.
Copyright (c) 2020 Dr. Ana-Maria Ionescu (Author)