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Abstract

<jats:p>The Lorentz factor plays a central role in Special Relativity, describing space dilation, time contraction, and relativistic momentum-energy relations. In the regime where velocities are significantly smaller than the speed of light, the classical equations of Newtonian mechanics must be recovered. This note presents a detailed, step-by-step derivation of the low-velocity binomial approximation for the Lorentz factor and demonstrates how this approximation bridges relativistic dynamics with classical kinetic energy.</jats:p>

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Keywords

lorentz factor relativistic classical approximation

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