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3. (a)...
3. (a) Show that [e-21/a (1 + 2r/a + 2r2/a?)] = -4r²e-20/a. (b) Use this result to show that the ground state wavefunction of the hydrogen atom is properly normalized: S• P(r) dr = 1. In astronomy, analysis of the photons emitted from very hot plasmas (such as are ob- served at the surface of stars, or during supernova explosions) commonly reveals spec- tral lines from highly ionized iron (see e.g. the paper by Decaux et al., which is available on the Problem Set 9 Assignment web-page). (c) Treating 25-times ionized iron as a hydrogenic atom to which the usual Schrödinger [4] equation applies, calculate: i. the most-probable distance to find the electron from the nucleus (hint: see sample problem 39.06 in H&R); ii. the energy of photons emitted for a transition between the 2s and is states. Are these photons in the infra-red, visible, ultra-violet, x-ray or 7-ray part of the spec- trum? (d) If you were to treat the kinetic energy of the electron, in the 1s state, as classical (i.e. [2] K =(half of the binding energy), and K = mv2) what would be the speed of the electron? Should we be using special relativity to describe the electron in the ground state of 25-times ionized iron? (e) If we were to use special relativity, one obvious thing we would have to do (there are [1] others) is to replace m with ym, where y=1/11 - 02/c2. Would this change mean that the electron is closer on average, or farther, from the nucleus, than we found above?