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Lorentz factor
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===Series expansion (velocity)=== The Lorentz factor has the [[Taylor series|Maclaurin series]]: <math display="block">\begin{align} \gamma & = \dfrac{1}{\sqrt{1 - \beta^2}} \\[1ex] & = \sum_{n=0}^{\infty} \beta^{2n}\prod_{k=1}^n \left(\dfrac{2k - 1}{2k}\right) \\[1ex] & = 1 + \tfrac12 \beta^2 + \tfrac38 \beta^4 + \tfrac{5}{16} \beta^6 + \tfrac{35}{128} \beta^8 + \tfrac{63}{256} \beta^{10} + \cdots , \end{align}</math> which is a special case of a [[binomial series]]. The approximation <math display="inline">\gamma \approx 1 + \frac{1}{2}\beta^2</math> may be used to calculate relativistic effects at low speeds. It holds to within 1% error for {{mvar|v}} < 0.4 {{mvar|c}} ({{mvar|v}} < 120,000 km/s), and to within 0.1% error for {{mvar|v}} < 0.22 {{mvar|c}} ({{mvar|v}} < 66,000 km/s). The truncated versions of this series also allow [[physicist]]s to prove that [[special relativity]] reduces to [[Newtonian mechanics]] at low speeds. For example, in special relativity, the following two equations hold: <math display="block">\begin{align} \mathbf p & = \gamma m \mathbf v, \\ E & = \gamma m c^2. \end{align}</math> For <math>\gamma \approx 1</math> and <math display="inline">\gamma \approx 1 + \frac{1}{2}\beta^2</math>, respectively, these reduce to their Newtonian equivalents: <math display="block">\begin{align} \mathbf p & = m \mathbf v, \\ E & = m c^2 + \tfrac12 m v^2. \end{align}</math> The Lorentz factor equation can also be inverted to yield <math display="block">\beta = \sqrt{1 - \frac{1}{\gamma^2}} .</math> This has an asymptotic form <math display="block">\beta = 1 - \tfrac12 \gamma^{-2} - \tfrac18 \gamma^{-4} - \tfrac{1}{16} \gamma^{-6} - \tfrac{5}{128} \gamma^{-8} + \cdots\,.</math> The first two terms are occasionally used to quickly calculate velocities from large {{mvar|Ξ³}} values. The approximation <math display="inline">\beta \approx 1 - \frac{1}{2}\gamma^{-2}</math> holds to within 1% tolerance for {{nobr|{{math|''Ξ³'' > 2}},}} and to within 0.1% tolerance for {{nobr|{{math|''Ξ³'' > 3.5}}.}}
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