Since an electron on a circular orbit around a proton has a centripetal acceleration, it should radiate

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Since an electron on a circular orbit around a proton has a centripetal acceleration, it should radiate energy according to the Larmor relation dE/dt¼-2/3 (q2/4πε0) (a2/c3) where q, a, ε0, and c are, respectively, the electron charge, its acceleration, the vacuum permittivity, and the velocity of light in vacuum. Therefore, in classical mechanics, it should spiral and crash on the nucleus. How long would this decay take, supposing that the size of the initial orbit is 10 -10 m and the nucleus is a point charge (i.e., radius ¼ 0)?

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