Balmer series 2026-10-18
Hydrogen atom spectral lines terminating at principal quantum number ; see the Bohr model for the elementary wavelength calculation.
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]
https://labs.physik.kit.edu/prakt-klass-physik-manuals/P2/Franck_Hertz_Versuch/. KIT physics laboratory, H23 Franck-Hertz-Versuch, Motivation
.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]
https://physlab.org/wp-content/uploads/2016/03/Franck_exp_v12015.pdf. Shah, Alam and Anwar, Electron energy loss investigated through the Franck-Hertz Experiment, sections 3–4
.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]
https://physlab.org/wp-content/uploads/2016/03/Franck_exp_v12015.pdf. Shah, Alam and Anwar, sections 3.1–4 and Figure 3
.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]
https://ocw.mit.edu/courses/8-13-14-experimental-physics-i-ii-junior-lab-fall-2016-spring-2017/afdfff9f8bbe067239af19c8b178a764_MIT8_13-14F16-S17exp7.pdf. MIT Junior Lab, The Franck-Hertz Experiment, section VI and the discussion following Figure 6
.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]
Transformations of Kinetic Energy of Free Electrons into Excitation Energy of Atoms by Impacts by James Franck. Nobel Lectures, Physics 1922–1941; pp. 98, 100–101
Gustav Ludwig Hertz explained how a field-free collision region narrowed excitation thresholds.[ref]The Results of the Electron-Impact Tests in the Light of Bohr’s Theory of Atoms by Gustav Ludwig Hertz. Nobel Lectures, Physics 1922–1941; pp. 112, 119–120
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 areThe 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, givesThus 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.
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.
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.
Lyman series 2026-10-18
Hydrogen atom spectral lines terminating at principal quantum number ; see the Bohr model for the elementary energy difference calculation.
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]
The Nobel Prize (Niels Bohr) by Niels Bohr Institute. The Nobel Prize: atomic theory and the 1922 award
[ref]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. Nobel Prize in Physics in 1922 2026-10-18
Awarded to Niels Bohr for atomic structure and radiation from chemical atoms. The Bohr model explains the connection to discrete spectral lines.[ref]
The Nobel Prize in Physics 1922 by Nobel Prize Outreach. Official award record: Bohr, atomic structure and radiation
Past exam of the mathematics course of the University of Cambridge 2004 ib Paper 3 9D Solution Created 2026-09-24 Updated 2026-10-14
With the proton treated as fixed and electron mass , the classical energy and angular momentum areFor a circular orbit, and Coulomb's law determines its centripetal acceleration:Eliminating gives . Thus the Bohr radius and orbit radii areThe kinetic energy is half the magnitude of the attractive potential energy. HenceThis is the circular-orbit Bohr model; including proton recoil replaces by the reduced mass.
Past exam of the mathematics course of the University of Cambridge 2016 ib Paper 3 16B b Solution Created 2026-09-24 Updated 2026-10-06
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 obeysBohr postulates permitted nonradiating stationary orbits with , for . These assumptions giveFor 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 yieldsFor 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 givesThus 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.
Past exam of the physics A course of the University of Cambridge 2017 Paper 2 Section C C11 Donor binding energy, size and thermal ionisation Created 2026-10-18 Updated 2026-10-20
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 magnitudeThe radius isusing 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.
Rydberg formula 2026-10-18
For the elementary hydrogen atom derivation, see the Bohr model.

