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Astrophysics, Cosmology & Relativity

Special Relativity

Albert Einstein's 1905 theory describing the physical behavior of space and time for observers moving in uniform non-accelerated inertial frames.

Governing formula E² = (p c)² + (m₀ c²)², γ = 1 / √(1 - v²/c²)
SI unit Theoretical Framework

In depth

Rests on two fundamental postulates: the laws of physics are identical in all inertial reference frames, and the speed of light in vacuum c is a universal constant for all observers regardless of motion. Predicts time dilation, length contraction, and mass-energy equivalence.

Examples in the real world

Cosmic ray muons reaching Earth's surface due to relativistic time dilation expanding their apparent lifetime.