In the Franck-Hertz experiment, electrons emitted from a heated cathode are accelerated through a dilute atomic vapour toward a collector. A small retarding potential before the collector rejects electrons that have lost too much kinetic energy. Below the first excitation threshold, mainly elastic collisions occur and the collector current rises as the accelerating voltage increases. At threshold an inelastic collision can transfer a definite excitation energy to an atom, causing a current drop because the slowed electron cannot overcome the retarding potential.
Raising the voltage further permits acceleration again, and repeated losses produce successive current minima. For mercury their spacing is about 4.9V, corresponding to an atomic excitation of about 4.9eV and an associated ultraviolet photon near 254nm. Contact potentials shift the absolute voltages, so the spacing is more informative than the first minimum's position alone. Discrete energy losses support discrete atomic energy levels; a continuously variable excitation energy would not produce the same recurring fixed loss scale. The experiment establishes quantized excitations without requiring the classical electron orbit of the Bohr model to be literally correct.
A classical orbiting electron accelerates and therefore radiates according to the Larmor formula. Its mechanical energy becomes more negative, its radius decreases, and the orbit spirals inward rather than remaining a stable atom. The Bohr model replaces this prediction with postulated nonradiating stationary states and quantized orbital angular momentum, together with photon emission or absorption only between states, hν=∣En−Em∣.
For a heavy nucleus, mevr=nℏ. Since the de Broglie wavelength is h/(mev), this impliesThe electronic wave fits an integer number of wavelengths around the orbit. This is a standing-wave consistency interpretation of the quantization rule, not a classical mechanism that prevents an accelerating charge from radiating. For finite nuclear mass, the two-body relative coordinate uses reduced mass μ=meM/(me+M); the next derivation retains that correction. In the limit M≫me, it reduces to the fixed-nucleus electron description above.
2πr=nλ,n=1,2,….
Let r be the electron-nucleus separation and use the reduced mass μ=meM/(me+M). Coulomb attraction supplies the relative centripetal force, and Bohr quantization fixes the relative angular momentum:Eliminating v givesThe total energy is E=μv2/2−Ze2/(4πϵ0r)=−Ze2/(8πϵ0r), henceHere a0 is the ordinary Bohr radius and R∞ the infinite-nuclear-mass Rydberg constant. The electron's radius about the centre of mass is Mrn/(M+me); for a heavy nucleus this distinction and the reduced-mass correction are small, but the supplied nuclear mass permits them to be stated precisely.
rμv2=4πϵ0r2Ze2,μvr=nℏ.
rn=μZe24πϵ0ℏ2n2=a0μmeZn2.
En=−2(4πϵ0)2ℏ2n2μZ2e4=−hcRMn2Z2,RM=R∞meμ.
The emitted photon carries the decrease in atomic energy, so hc/λ=En−Em for n>m. Using the preceding energy levels givesThe lower state's energy is more negative, making the right-hand side positive. This is the hydrogenic Rydberg formula, with the finite-nuclear-mass factor included in RM.
λ1=RMZ2(m21−n21).
At room temperature, kBT is of order 0.026eV, far smaller than the electronic excitation gaps of the inferred hydrogenic ion. Ground-state absorption is therefore the natural interpretation. Assign the three lines to 1→2, 1→3, and 1→4. Dividing each reciprocal wavelength by its corresponding factor 1−1/n2 givesThe small scatter is consistent with the rounded wavelength data. Since R∞≃1.0974×107m−1 and μ≃me,The ion is thus hydrogen-like lithium, Li2+. If “effective Rydberg constant” denotes only the reduced-mass constant rather than the charge-inclusive spectral coefficient, its value is RM≃Reff/9≃1.097×107m−1. The two conventions are explicitly distinguished; the rounded lines do not determine a precise isotope mass.
Reff=RMZ2≃(9.8765,9.8684,9.8765)×107m−1.
Reff≃9.87×107m−1,Z≃Reff/R∞=3.
For Coulomb binding, the virial theorem gives a typical kinetic energy of the order of the binding energy. Taking ptyp≃2me∣E1∣ and using the Heisenberg uncertainty relation estimate rtyp∼ℏ/ptyp givesThe Bohr model gives r1=a0/Z=a0/2=2.65×10−11m for a heavy helium nucleus, agreeing with the characteristic scale. Equivalently, minimizing the localization estimate E(r)∼ℏ2/(2mer2)−Ze2/(4πϵ0r) gives that same scale.
rtyp∼2me(54.4eV)ℏ=2.65×10−11m.
This is an order-of-magnitude radius estimate, not an exact deduction of the cloud's expected value from the inequality alone. Numerical coefficients depend on which spread is used; ΔxΔp≥ℏ/2 does not assert ⟨r⟩=ℏ/p. For the exact hydrogenic 1s state, ⟨r⟩=3a0/(2Z)=3.97×10−11m at Z=2, one and a half times the Bohr orbital radius. An electron cloud has a radial distribution, whereas the Bohr model assigns a definite radius.
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