General Relativity
General Relativity is a theory of gravitation that describes gravity as the curvature of spacetime caused by mass and energy. Unlike Newtonian gravity, it treats gravity not as a force but as a geometric property of spacetime. Objects move along curved paths determined by spacetime geometry. General relativity accurately explains phenomena such as gravitational time dilation, light bending, and planetary precession. It predicts exotic objects such as black holes and neutron stars. General relativity is essential for understanding cosmology, gravitational waves, and the large-scale structure of the universe. Despite its mathematical complexity, it has been confirmed by numerous experiments. General relativity remains one of the most elegant and successful theories in physics.
Ephraim Suhir
Portland State University, United States
Alexander Unzicker
Pestalozzi Gymnasium Munchen, Germany
Paulo Cesar De Morais
University of Brasilia, Brazil
Thomas J Webster
Brown University, United States
Jon H Brasher
Stelleo Scientific Foundation, United States
Tom Lawrence
Ronin Institute of Independent Scholarship 2.0, United Kingdom
Wenjie Liu
University of Oxford, United KingdomSubmit your abstract Today
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