Franck-Hertz experiment Created 2026-10-14 Updated 2026-10-20
The Franck-Hertz experiment connects a reproducible loss of electron kinetic energy with excitation of a chemical atom. The original mercury-vapor experiments were performed during 1912–1914 while investigating ionization; they were not designed as a test of the Bohr model. Their later interpretation distinguished internal excitation from removal of an electron. [ref].
In a modern mercury tube, a heated cathode emits electrons and a positive perforated grid accelerates them through Hg vapor. A collector slightly below the grid's electric potential rejects slow electrons. The oven controls vapor density and hence the mean free path. Keep heating and retarding settings fixed, sweep the accelerating electric potential difference , and record collector electric current . These measured quantities indirectly probe atomic excitation. [ref].
The curve shows repeated current minima, typically about apart. In the collision model, an electron gains approximately of kinetic energy, with the positive elementary charge. An inelastic collision transfers about to internal excitation. Near the grid, this can prevent the electron crossing the retarding region, lowering collected electric current. Further acceleration restores collection; repeated excitation losses produce further minima. These represent multiple collisions, rather than equally spaced atomic energy eigenvalues. Contact potentials shift the first minimum, so compare several successive spacings instead of identifying the first dip's voltage with the excitation cost. [ref].
The optical comparison supplies a second observable: mercury radiation at a wavelength near was detected through a window in the tube. Its inferred photon energy agrees with the characteristic collision loss, with the speed of light. This agreement supports the interpretation as a transition between internal atomic energies. It does not make the collector trace a complete spectrum. In particular, the lowest excited mercury level, labeled , is metastable because an electric-dipole selection rule forbids its direct transition to the ground state; the nearby level emits the quoted ultraviolet line. Collision excitation and optical detection therefore have different sensitivities to the available excited states. [ref].
Initial electron kinetic energy spread and varying collision positions broaden real minima. Repeat traces at different retarding settings and oven temperatures to distinguish excitation from collection effects. This probes a discrete energy-transfer channel, rather than every energy eigenspace, its dimension, or an absolute ground-state energy. [ref].
James Franck and Gustav Ludwig Hertz presented their paper on 24 April 1914. Its heated platinum wire sat inside a cylindrical platinum mesh, with a collector 1–2 mm beyond it. A heated bath and pumping prepared the vapor; guard rings suppressed leakage. They differentiated retarding-electric current scans to study outgoing energies.[ref]
Their 1925 Nobel Prize preceded their lectures of 11 December 1926. James Franck described choosing pressure for many collisions before the mesh but few afterward.[ref] Gustav Ludwig Hertz explained how a field-free collision region narrowed excitation thresholds.[ref]
Hydrogenic donor state 2026-10-18
A shallow donor impurity in an isotropic semiconductor can be approximated by an electron of effective mass in a Coulomb potential screened by relative permittivity . Its ground-state binding energy and radius are
The donor level lies below the conduction band. These are magnitudes: the bound electron's energy relative to the band edge is negative. Band anisotropy, short-distance impurity structure and screening by mobile carriers can invalidate the simple Bohr model rescaling.
Hydrogen spectral series 2026-10-18
A family of hydrogen emission lines terminating at a fixed lower principal quantum number . In the nonrelativistic Bohr model, their inverse wavelengths are for integers . Holding fixed and increasing gives lines approaching the series limit . Reduced mass shifts the Rydberg constant, while additional interactions produce corrections to this gross spectral pattern.
Hydrogen transition wavelengths in the Bohr model Created 2026-10-18 Updated 2026-10-20
For emission take integers . Applying conservation of energy to the model's internal energy difference, while neglecting the much smaller whole-atom photon recoil, gives
Thus Johannes Robert Rydberg's Rydberg formula is a difference of two energy levels expressed as a spectroscopic wavenumber. The same constants determine every line; there is no new parameter for each electronic transition. With the chosen inputs, . All wavelengths below are calculated in vacuum, not air, and are rounded model predictions rather than historical measurements.
Electronic transition SeriesPhoton energy in electronvoltsVacuum wavelength in Lyman seriesLyman seriesBalmer seriesBalmer seriesBalmer seriesBalmer series
The conventional names commemorate Theodore Lyman and Johann Jakob Balmer. Fixing produces the ultraviolet Lyman series, beginning with the Lyman-alpha line; fixing produces the Balmer series. As , the wavelength approaches : at the Lyman limit and for the Balmer series. Crowding follows directly from . Discreteness therefore coexists with a series limit.
Figure 1.
Calculated hydrogen atom energy levels and selected Lyman series and Balmer series emissions
. Original Bohr model prediction using the stipulated finite nuclear mass. Left: the full energy scale with the ionization energy threshold at zero. Right: an expanded upper-level view makes the Balmer series arrows readable. Downward arrows mark internal energy differences, not spatial electron trajectories; their selection does not predict relative line strengths. Details.
Correct line positions do not give wave intensities, lifetimes or electric-dipole selection rules for hydrogen. Those require a theory of the wavefunctions and their coupling to electromagnetic radiation. The circular model also omits spin, relativistic corrections and the Lamb shift. Its successful gross energy levels do not make its assumed orbits modern atomic orbitals.
Niels Bohr Created 2026-10-18 Updated 2026-10-31
A physicist associated with the Bohr model of the chemical atom. His 1922 Nobel Prize in Physics concerned atomic structure and radiation.[ref][ref]
Figure 1.
Portrait of Niels Bohr
. Bain News Service, publisher; Library of Congress, George Grantham Bain Collection, ggbain.35303; restoration credited on the File to Bammesk. Library of Congress: no known copyright restrictions; Commons additionally records origin/life-plus-70-or-shorter and pre-1931 United States public-domain grounds., via Wikimedia Commons. Source.
Awarded to Niels Bohr for atomic structure and radiation from chemical atoms. The Bohr model explains the connection to discrete spectral lines.[ref]
With the proton treated as fixed and electron mass , the classical energy and angular momentum are
For a circular orbit, and Coulomb's law determines its centripetal acceleration:
Eliminating gives . Thus the Bohr radius and orbit radii are
The kinetic energy is half the magnitude of the attractive potential energy. Hence
This is the circular-orbit Bohr model; including proton recoil replaces by the reduced mass.
The agreement is in the energy levels, not in electron trajectories. The Bohr model assumes a particle on a circular orbit, with orbital angular momentum quantized as . The Coulomb bound states here are spatially distributed wavefunctions with no definite classical orbit. Their probability density is spherically symmetric, and their orbital angular momentum is zero because . Their radial distributions also depend on and can have nodes. A real radial wavefunction times a global stationary phase has zero probability current, unlike the circulating point charge in the Bohr picture.
The Bohr model combines classical circular motion in the Coulomb potential with explicitly quantum postulates. A one-electron atom of nuclear charge has electron–nucleus reduced mass . With , the relative circular orbit obeys
Bohr postulates permitted nonradiating stationary orbits with , for . These assumptions give
For hydrogen with the nucleus taken infinitely heavy, the radius is the Bohr radius, . The finite reduced mass gives the small nuclear-motion correction, and increasing contracts the one-electron orbit.
The circular-motion equation gives while the potential energy is , so the total energy is . Substituting the quantized radius yields
For the heavy-nucleus hydrogen approximation, . The ionization threshold is zero energy, so removing the ground-state electron requires about .
The model further postulates that radiation is emitted or absorbed only in transitions between stationary orbits, with photon energy . Emission from gives
Thus it reproduces the principal hydrogen spectral series, their limiting wavelengths, and the gross hydrogenic energy levels. For example, in hydrogen has and , a visible line. Absorption reverses the transition when the photon matches the energy gap.
The achievement is that quantized energies explain discrete spectra, but the model's stationary orbits are postulates rather than consequences of classical electrodynamics: an accelerating classical charge would radiate. It does not provide a general calculation of line intensities or transition selection rules and fails as a quantitative theory of many-electron atoms. Spin, fine structure and the full Zeeman effect require further physics. Modern quantum mechanics replaces definite electron orbits by wavefunctions and quantum probabilities. In particular, the true hydrogen ground state has , so its orbital angular momentum vanishes; the model's rule should not be identified with the modern orbital eigenvalue rule . Bohr's energy quantization remains a successful hydrogenic approximation, while its literal orbital picture does not.
For a hydrogenic donor state, replace the bare electron mass by and the Coulomb permittivity by with . Rescaling the Bohr model gives the positive ground-state binding magnitude
The radius is
using the Bohr radius . The supplied positive hydrogen “energy” formula should be interpreted as a binding magnitude; the bound level's energy relative to the conduction-band edge is .
At , , about five times the binding energy. Thus a substantial fraction, ordinarily most of the shallow donors in the dilute nondegenerate regime, will be ionised. An exact fraction also depends on the Fermi level, donor concentration and degeneracies; comparing with alone does not determine it exactly. The large radius explains why a weakly bound donor extends across many unit cells.
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 , corresponding to an atomic excitation of about and an associated ultraviolet photon near . 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, .
For a heavy nucleus, . Since the de Broglie wavelength is , this implies
The 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 ; the next derivation retains that correction. In the limit , it reduces to the fixed-nucleus electron description above.
For Coulomb binding, the virial theorem gives a typical kinetic energy of the order of the binding energy. Taking and using the Heisenberg uncertainty relation estimate gives
The Bohr model gives for a heavy helium nucleus, agreeing with the characteristic scale. Equivalently, minimizing the localization estimate gives that same scale.
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; does not assert . For the exact hydrogenic state, at , one and a half times the Bohr orbital radius. An electron cloud has a radial distribution, whereas the Bohr model assigns a definite radius.
The Bohr model assumes Coulomb attraction and classical circular motion between transitions; selected stationary orbits do not radiate; their angular momentum is ; and a transition exchanges a photon of energy . The first two dynamical equations give
Here , is the electron mass under the fixed-proton approximation, its charge magnitude, and the vacuum permittivity. The stationary-orbit postulate deliberately suspends the classical radiation prediction; this is a historical model, not a consistent deduction from classical electrodynamics.
Rydberg formula 2026-10-18
For the elementary hydrogen atom derivation, see the Bohr model.