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Matter wave
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=== Phase velocity === The [[phase velocity]] in isotropic media is defined as: <math display="block">\mathbf{v_p} = \frac{\omega}{\mathbf{k}}</math> Using the relativistic group velocity above:<ref name="WhittakerII"/>{{rp|p=215}} <math display="block">\mathbf{v_p} = \frac{c^2 }{\mathbf{v_g}}</math> This shows that <math>\mathbf{v_{p}}\cdot \mathbf{v_{g}}=c^2</math> as reported by R.W. Ditchburn in 1948 and J. L. Synge in 1952. Electromagnetic waves also obey <math>\mathbf{v_{p}}\cdot \mathbf{v_{g}}=c^2</math>, as both <math>|\mathbf{v_p}|=c</math> and <math>|\mathbf{v_g}|=c</math>. Since for matter waves, <math>|\mathbf{v_g}| < c</math>, it follows that <math>|\mathbf{v_p}| > c</math>, but only the group velocity carries information. The [[Faster-than-light|superluminal]] phase velocity therefore does not violate special relativity, as it does not carry information. For non-isotropic media, then <math display="block">\mathbf{v}_\mathrm{p} = \frac{\omega}{\mathbf{k}} = \frac{E/\hbar}{\mathbf{p}/\hbar} = \frac{E}{\mathbf{p}}. </math> Using the [[special relativity|relativistic]] relations for energy and momentum yields <math display="block">\mathbf{v}_\mathrm{p} = \frac{E}{\mathbf{p}} = \frac{m c^2}{m \mathbf{v}} = \frac{\gamma m_0 c^2}{\gamma m_0 \mathbf{v}} = \frac{c^2}{\mathbf{v}}.</math> The variable <math>\mathbf{v}</math> can either be interpreted as the speed of the particle or the group velocity of the corresponding matter wave—the two are the same. Since the particle speed <math>|\mathbf{v}| < c </math> for any particle that has nonzero mass (according to [[special relativity]]), the phase velocity of matter waves always exceeds ''c'', i.e., <math display="block">| \mathbf{v}_\mathrm{p} | > c ,</math> which approaches ''c'' when the particle speed is relativistic. The [[Faster-than-light|superluminal]] phase velocity does not violate special relativity, similar to the case above for non-isotropic media. See the article on ''[[Dispersion (optics)#Group velocity dispersion|Dispersion (optics)]]'' for further details.
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