Photon number emission in synchrotron radiation: Systematics for high-energy particles

preprint2004arXivOpen access

Abstract

A recent derivation of an explicit elementary expression for the mean number <N><N> of photons emitted per revolution in synchrotron radiation allows a systematic high-energy analysis leading to the result <N>≃5πα/3(1−β2)+a0α+πα1−β2/103<N>\simeq 5πα/\sqrt{3(1-β^2)}+a_0α+πα\sqrt{1-β^2}/10\sqrt{3} where a0a_0 is a constant, with relative errors of 2.2%, 0.64%, 0.017%, in comparison to the well-known formula tabulated in the literature of 160%, 82%, 17% for β=0.8β=0.8, 0.9, 0.99, respectively.

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