General relativity is a fundamental theory in physics that describes gravity as the curvature of spacetime caused by mass and energy.
Overview
Key Concepts
Historical Context
Modern Developments
Experimental Evidence
Mathematical Foundations
Astrophysical Implications
Challenges And Misconceptions
Applications Of General Relativity
Quantum Mechanics
Quantum Gravity
Albert Einstein
Solar Eclipse
Edwin Hubble
Isaac Newton
Black Holes
Equation
Universe
๐ General relativity, proposed by Albert Einstein in 1915, describes gravity as the curvature of spacetime caused by mass.
๐ One of its predictions is that massive objects, like stars and planets, can bend light, creating gravitational lensing.
๐ Black holes are a direct consequence of general relativity, where spacetime is warped so intensely that not even light can escape.
๐ฐ๏ธ Time runs slower in stronger gravitational fields, a phenomenon known as time dilation.
๐ The theory has been confirmed by multiple experiments, including the observation of the bending of starlight during a solar eclipse.
๐ญ General relativity revolutionized our understanding of the universe, enabling the prediction of phenomena like gravitational waves.
๐ The equation E=mcยฒ, which relates mass and energy, is a result of the principles found in general relativity.
๐ธ GPS satellites account for general relativity to provide accurate positioning, as they experience less gravity than those on Earth.
๐ General relativity unifies space and time into a single four-dimensional continuum known as spacetime.
๐ The theory has implications for cosmology, explaining the expansion of the universe and the behavior of galaxies.
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