Dawson Pritchard
06/04/2024 · High School
\( R _ { \mu v } - \frac { 1 } { 2 } R g _ { \mu v } + \Lambda g _ { \mu v } = \frac { 8 \pi G } { c ^ { 4 } } T _ { \mu v } \)
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The Einstein field equation describes how matter and energy affect the curvature of spacetime, with the left side representing geometry and the right side representing matter and energy. It includes the cosmological constant, which accounts for dark energy.
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