Hydrogen Atom Energy Levels and Degeneracy
Drop a single electron into the Coulomb field of a proton and something remarkable happens. The energy of the resulting bound states depends on exactly one quantum number, not three. This is strange. The Schrödinger equation for the Hydrogen Atom involves a wavefunction . It depends on three quantum numbers , , . Yet the energy eigenvalue collapses to
with no trace of or anywhere. Every other central-potential problem you will ever solve shows energies that do depend on . This includes the particle on a sphere with a non-Coulomb potential. It includes an atom in a crystal field, or a diatomic vibrator-rotor. Hydrogen is the exception. Understanding why it is an exception is one of the most instructive stories in quantum chemistry. This matters far beyond a curiosity of one textbook problem. The degeneracy pattern of hydrogen is states (or with spin) crowded into a single energy. This pattern is the scaffolding for the periodic table's orbital energetics. It is also the reason multi-electron atoms break that degeneracy in the way they do. Screening lifts the -degeneracy, giving the familiar ordering. The Lyman, Balmer, and Paschen series in the hydrogen emission spectrum are direct photographs of the ladder. The fine structure and Lamb shift experiments that made 20th-century physics famous are essentially precision measurements. They show how real hydrogen deviates from this idealized formula. The big picture is this: the Coulomb potential is special among central potentials. It possesses a hidden symmetry beyond ordinary rotational symmetry. This is a conserved quantity called the Laplace–Runge–Lenz vector. This vector is familiar from the classical Kepler problem. There, it explains why planetary orbits are closed ellipses that do not precess. Quantum mechanically, this extra symmetry enlarges the group of transformations that commute with the Hamiltonian. It grows from (rotations only) to . This enlargement forces states of different but the same to share an energy. This is called accidental degeneracy. However, "accidental" is a historical misnomer for something that is in fact deeply structural. This article builds the full degeneracy picture from the ground up. It covers the origin of the formula from the The Radial Equation and Radial Wavefunctions. It explains why ranges over and over . It shows how these combinatorics give exactly spatial states. It also explains why the Coulomb potential specifically, and no other radial potential, makes the energy blind to . Along the way you will see how the degeneracy shows up in the Balmer spectrum. You will see how it gets broken by external fields (Zeeman, Stark) and by relativistic corrections. Finally, you will see how it reappears as the conceptual seed for Term Symbols and Atomic States in multi-electron atoms.
- Hydrogen-like energies depend on principal quantum number alone: Ry, with no dependence on or .
- For each , allowed values are and , giving spatial orbitals, with spin.
- -degeneracy ( states per ) is essential, guaranteed by rotational symmetry alone — it survives in any central potential.
- -degeneracy (all within a given sharing one energy) is accidental, special to the exact Coulomb potential, and traces to the conserved Runge–Lenz vector.
- Any perturbation that is not perfectly or not perfectly isotropic — screening in multi-electron atoms, external electric/magnetic fields, relativistic corrections — splits this accidental degeneracy.
- Key idea: hydrogen's energy levels depend only on because the Coulomb potential has a hidden symmetry beyond ordinary rotations, making the -degeneracy structural rather than coincidental.
Where this lives today
The / degeneracy counting is the direct ancestor of the shell-capacity numbers () used every day in general chemistry to build up the periodic table, even though real multi-electron atoms break the -part of the degeneracy (which is exactly why fills before , a fact with enormous consequences for transition-metal chemistry, catalysis, and coordination chemistry). Precision spectroscopy of hydrogen and hydrogen-like ions remains one of the most stringent tests of quantum electrodynamics and fundamental constants: modern laser spectroscopy of the – two-photon transition in atomic hydrogen has been measured to better than one part in , and comparing the measured splitting between states that would be "accidentally" degenerate in the pure Coulomb picture (like and , the Lamb shift) directly probes vacuum polarization and electron self-energy — QED effects with no classical analogue. In astrophysics, hydrogen-like ion spectra (He⁺, Li²⁺, and highly stripped heavy ions in stellar coronae, solar flares, and X-ray binary accretion disks) are read off using exactly the scaling worked out above, letting astronomers infer both the ionization state and temperature of extremely hot plasmas from X-ray line positions. In quantum control and Rydberg-atom physics — a field central to modern quantum computing and quantum simulation platforms — atoms are excited to very high (Rydberg states), where the near-degeneracy of different within a shell (slightly broken by quantum defects in non-hydrogenic atoms) is deliberately exploited to engineer strong, tunable, long-range dipolar interactions between atoms for two-qubit gates. Finally, the entire conceptual toolkit here — separating essential (symmetry-guaranteed) from accidental (potential-specific) degeneracy — recurs whenever chemists analyze Term Symbols and Atomic States in multi-electron atoms, and whenever spectroscopists interpret Radial Distribution Functions to rationalize orbital penetration and shielding effects that ultimately lift hydrogen's special accidental degeneracy in every atom heavier than hydrogen.
Ask the tutor: How exactly does electron screening in a multi-electron atom convert the flat -degenerate hydrogen shell into the split ordering used in the aufbau principle?
The physical picture
Solving the Hydrogen Atom Schrödinger equation by separation of variables in spherical coordinates gives . The angular factor , the spherical harmonic, is completely universal: it is the same function for any central potential , because it comes purely from the angular part of the kinetic energy operator (the operator) commuting with any Hamiltonian of the form . The radial factor , by contrast, is where the specific shape of enters, and it is the radial equation that ultimately fixes the energy. For the hydrogen-like radial equation, imposing square-integrability (a bound, normalizable state) forces a quantization condition that, after the dust settles, reads
where is the number of radial nodes. This is the origin of the famous rule : since , we need . The energy formula that emerges from solving the radial equation depends only on the combination — not on and separately. That is the mathematical fingerprint of accidental degeneracy: two completely different orbitals, say () and (), both have and are exactly degenerate, even though one has a radial node and no angular node while the other has an angular node and no radial node. The figure below shows the degeneracy structure for hydrogen levels, with the orbital "boxes" grouped horizontally by but sitting at the same height (same ) within each shell.
Notice what this diagram is really asserting: the and bars sit at exactly the same height, Ry, even though they are drawn at different horizontal positions to distinguish them by shape. In any non-Coulombic central potential (say, a screened potential in a many-electron atom, or a 3-D isotropic harmonic oscillator with an added anharmonic term), the and bars would separate vertically — that is precisely how orbital energy ordering ( before , for instance) arises in the periodic table. The next figure decomposes a single shell into its full -degeneracy as well, making explicit the counting that gives states.
The distinction drawn at the bottom of that figure is the conceptual heart of this article. The states within a fixed (the -degeneracy) exist because empty space has no preferred axis: rotate your coordinate system and is unchanged, so states related by rotation must be degenerate. This is essential degeneracy — it is required by symmetry in every central potential without exception, hydrogen or not. The further degeneracy across different within the same is a much more delicate, Coulomb-specific effect, discussed in the derivations below.
The core ideas
The hydrogen-like (one electron, nuclear charge ) bound-state energy is
where:
- is the nuclear charge (1 for H, 2 for He⁺, 3 for Li²⁺, …),
- is the reduced mass of the electron–nucleus system, ,
- is the principal quantum number, running over positive integers,
- is the Rydberg energy, and eV (hartree) is the atomic energy unit, so .
Reading: the energy is negative (bound state, energy measured relative to the ionized, infinitely separated electron and nucleus at rest), scales as (a more highly charged nucleus binds the electron much more tightly — this is why He⁺'s ground state is deeper than H's), and falls off as (levels crowd together rapidly as increases, converging to the ionization threshold ). The allowed quantum numbers for a given are
where:
- is the azimuthal (orbital angular momentum) quantum number, restricted by the radial quantization condition to be strictly less than ,
- is the magnetic quantum number, whose allowed values follow from the eigenvalue spectrum of once is fixed.
Reading: an -shell contains subshells ( through ), and subshell contains orbitals. This produces the shell-filling pattern 1 (for : only ), 4 (for : ), 9 (for ), etc. The total spatial degeneracy of level is obtained by summing over all :
where:
- the sum is an arithmetic series of odd numbers , which is a classical identity equal to .
Reading: this is the single most quoted degeneracy fact in atomic quantum chemistry. Including the two spin states of the electron (spin degeneracy is entirely separate physics — it has nothing to do with the spatial Coulomb symmetry, it is a relativistic/intrinsic property), the total degeneracy including spin is , which is exactly the capacity rule behind the shell structure that underlies (in a simplified, pre-screening form) the layout of the periodic table.
Derivations
Goal. Show explicitly that solving the hydrogen-like radial equation for bound states produces an energy that depends on the single combination , so that different pairs sharing the same are exactly degenerate.
Step 1 — Set up the radial equation. After separating , the radial function satisfies
The term is the centrifugal barrier coming purely from the angular kinetic energy; it enters the radial equation as an effective addition to the potential, which is why could, in principle, affect the energy — as it does for any potential other than pure Coulomb.
Step 2 — Substitute and go dimensionless. Defining turns the equation into a 1-D Schrödinger-like form,
Introduce the Bohr radius and the dimensionless variable together with (positive for bound states, since ). The equation becomes
Step 3 — Extract asymptotic behavior and posit a series solution. As the equation reduces to , giving (the decaying solution is kept for normalizability). As , the centrifugal term dominates and (again, keeping only the solution regular at the origin). Writing
and substituting into the differential equation produces a recursion for the power-series coefficients of :
Step 4 — Impose normalizability: the series must terminate. If the series for does not terminate, its coefficients behave like those of for large , which would make blow up at infinity — unacceptable for a bound, square-integrable state. The only way to avoid this is for the numerator to vanish at some non-negative integer , i.e.
Define (so since and ). Then simply .
Step 5 — Convert back to energy. Recall , so
Using (a standard identity relating the Bohr radius to the Rydberg energy), this becomes
Conclusion. The crucial point is in Step 4: the termination condition involves and only through their sum . Nowhere does the derivation produce a term depending on alone. That is a direct consequence of the potential being exactly — an inverse-first-power law — which is what allows the term in Step 3 to combine so cleanly with the exponential ansatz. Change the power of in the potential (e.g., add a term, or use a screened Yukawa-type potential), and the termination condition will involve independently, immediately lifting the -degeneracy.
Go deeper · Derivation B · 2 minWhy the Coulomb ℓ-degeneracy is not an accident: the Runge–Lenz vector
Goal. Show, using the symmetry argument (rather than brute-force solving the radial equation), why the Coulomb potential specifically produces extra conserved quantities that connect different values at fixed , explaining the term "accidental degeneracy" and why it is really a hidden dynamical symmetry.
Step 1 — Ordinary rotational symmetry and its consequence. In any central potential , the Hamiltonian commutes with all three components of orbital angular momentum, . This algebra closes among the alone: , generating rotations, i.e. the group . Because , , and can be simultaneously diagonalized, states of the same but different are automatically degenerate — this is the essential -fold degeneracy, guaranteed for every central potential with no further assumption.
Step 2 — The classical clue: the Runge–Lenz vector. In the classical Kepler problem with , in addition to angular momentum , there is a second conserved vector,
which points along the major axis of the classical elliptical orbit and whose constancy is exactly the statement that Kepler orbits do not precess — a special feature of the potential (Bertrand's theorem shows only and potentials give closed orbits for all bound trajectories). No other central-force law has a similarly conserved vector.
Step 3 — Quantum Runge–Lenz operator. The quantum-mechanical (symmetrized, Hermitian) analogue is
Direct (if lengthy) commutator algebra shows : the Runge–Lenz operator is conserved for the Coulomb Hamiltonian, and only for the Coulomb Hamiltonian among central potentials. Crucially, does not commute with : applying to a state of angular momentum produces a superposition containing and components (much as a raising/lowering operator connects adjacent quantum numbers). Because , states connected by must share the same energy eigenvalue — so states of different (but the same ) are forced into degeneracy by this extra symmetry.
Step 4 — The enlarged algebra: . Suitably rescaling (dividing by , valid within a fixed bound-state energy shell) and combining it with , one finds that the six operators close under commutation into the Lie algebra of (equivalently, two commuting copies of the / algebra after forming and ). Each irreducible representation of built this way has dimension and corresponds exactly to one principal quantum number shell — reproducing, by pure representation theory (no radial equation needed), both the correct energy spectrum and the degeneracy .
Conclusion. The -degeneracy of hydrogen is not a coincidence of the algebra in the derivation above (which could easily have failed to simplify) — it is a direct signature of the dynamical symmetry group being rather than merely . This is exactly analogous to (and historically inspired by) the 3-D isotropic harmonic oscillator, whose potential is the other potential satisfying Bertrand's theorem and which shows its own accidental degeneracy with symmetry group . Any deviation of the potential from pure — however small — breaks the Runge–Lenz conservation and splits the -degeneracy; this is exactly what happens physically inside multi-electron atoms.
Worked examples
Example 1 (foundational): Full quantum-number enumeration and energy for , hydrogen atom (). List every allowed combination for and verify the total count equals . Allowed : since , we have (spectroscopic labels ). For each , the number of values is :
Sum:
The energy for every one of these 16 states is identical:
Limiting-case check: as , (states pile up just below the ionization limit — this is the hallmark of a Coulomb potential's infinite bound-state ladder, in contrast to, e.g., a finite square well which has only finitely many bound states). Including spin doubles every count: total spin-orbitals in the shell, matching the familiar "" shell-capacity sequence.
Example 2 (applied): Comparing He⁺ () and H () at , and connecting to the Balmer-series-like transition. He⁺ is a hydrogen-like ion (one electron, ) — a system of real spectroscopic importance (its transition mimics part of the hydrogen Balmer series and was historically confused with it in early stellar spectra, the "Pickering series"). For He⁺, using the exact formula (ignoring the small reduced-mass correction, which shifts things by less than 0.03%):
At :
Compare with hydrogen's ground state, eV. These are numerically coincident (up to the reduced-mass correction) — this is a direct manifestation of the scaling: He⁺ at mimics H at because . Now consider the emission transition in He⁺:
Converting to a wavelength using J and :
This falls in the blue-green visible region — one member of the He⁺ Pickering series, historically mistaken for a hydrogen line before it was correctly assigned to He⁺. Limiting-case check: as larger values (say a hydrogen-like Fe²⁵⁺ ion, ), the same transition would scale as , pushing the emission from visible light all the way into the X-ray region — precisely how astrophysicists identify highly ionized species in solar-flare and accretion-disk X-ray spectra.
Example 3 (exam / competition level): Constructing an explicit degenerate pair at and demonstrating the accidental degeneracy numerically from the radial wavefunctions. Show explicitly, using the normalized radial functions, that () and () — which look completely different in shape — are eigenfunctions of the same radial Hamiltonian eigenvalue Ry, by evaluating the expectation value of the Hamiltonian directly (rather than trusting the general formula) at one representative sample point argument, and cross-checking with the general quantization condition. The hydrogen-like radial functions (in units where ; here consider Z=1 for simplicity so ) are:
Both functions decay with the same exponential rate — note that this exponential decay constant is set only by (recall from the derivation, , and ), not by . This is already a strong hint of the shared energy, since the asymptotic decay rate of a bound-state wavefunction is directly tied to via ; identical decay constants can only occur for identical . To make this quantitative, apply the quantization condition from the derivation directly to each case: For : (two radial nodes — matching the two roots of the quadratic factor ), , so
For : (no radial nodes — the function is nodeless for ), , so
Both give , hence identically
Despite having two radial nodes and zero angular nodes while has zero radial nodes and two angular nodes (the or real angular parts), the total node count is identical: in both cases. This total-node invariant, , is exactly what the Coulomb potential conserves, and is the operational, calculation-level manifestation of the symmetry argument. Limiting-case check: if we instead used a modified potential with small (a Coulomb-plus-centrifugal perturbation, as occurs approximately for penetrating orbitals in alkali-metal valence electrons), the effective in the radial equation would be replaced by , giving an effective non-integer and a quantization condition that depends on separately — immediately splitting below (lower penetrates the core more and is stabilized), exactly the origin of the orbital energy ordering used in Term Symbols and Atomic States and the aufbau principle for real multi-electron atoms.
Limiting cases, scope & common traps
| Situation | What happens to the degeneracy | Why |
|---|---|---|
| Exact one-electron Coulomb potential (H, He⁺, Li²⁺,…) | Full -fold degeneracy ( with spin) | Exact potential, hidden /Runge–Lenz symmetry |
| Multi-electron atoms (Na, Fe, …) | -degeneracy destroyed; | Core electrons screen the nuclear charge non-uniformly; effective potential is no longer pure |
| External magnetic field (Zeeman effect) | -degeneracy lifted; sublevels split | Breaks rotational () symmetry itself by picking out a preferred axis |
| External electric field (Stark effect) | Mixes states of different , same ; can partially lift degeneracy at first order | Couples states already accidentally degenerate via -like operator ( has matrix elements between and ) |
| Relativistic corrections (fine structure, Lamb shift) | Splits degeneracy within same (spin–orbit) and even vs (Lamb shift) | Relativistic kinetic energy and QED effects are not exactly -symmetric under |
| Levels crowd toward ; degeneracy | Coulomb potential supports infinitely many bound states (unlike a finite well) | |
| large (hydrogen-like heavy ions) | Degeneracy pattern unchanged, but scales as | The symmetry argument is -independent; only overall energy scale changes |
The chemist behind it
Origins · 1 minErwin Schrödinger and how this was discovered
Erwin Schrödinger solved the hydrogen atom wave equation in his landmark 1926 papers, obtaining the (Rydberg-scaled) spectrum directly from the newly proposed wave mechanics, matching the empirical Rydberg–Ritz formula that had summarized hydrogen's spectral lines for decades before any theoretical derivation existed. His derivation used the same separation-of-variables and Laguerre-polynomial machinery that underlies the radial equation treatment above. Schrödinger himself, along with Wolfgang Pauli (using matrix mechanics and the algebraic Runge–Lenz-vector method) and later Pauli's independent 1926 letter to Jordan, recognized that the extra -degeneracy pointed to a symmetry beyond simple rotational invariance — foreshadowing the group-theoretic () understanding fully worked out later by Vladimir Fock (1935) and Valentine Bargmann (1936), who made the connection to the four-dimensional rotation group rigorous.
Why doesn't the hydrogen energy depend on ℓ at all?
Because the Coulomb potential has an extra conserved quantity beyond ordinary angular momentum: the quantum Runge–Lenz vector. This vector commutes with the Hamiltonian but not with , so it connects states of different while forcing them to share the same energy. Solving the radial equation directly shows the same thing algebraically: the quantization condition only involves the combination , never and separately, so different pairs adding to the same are exactly degenerate. This is a special feature of the exact potential, not a general property of central potentials.
Is the m-degeneracy the same kind of thing as the ℓ-degeneracy?
No, and this distinction is essential. The -degeneracy (the states for a given ) is guaranteed by ordinary rotational symmetry, : since no direction in space is special for an isolated atom, states related by rotation must share the same energy. This holds for any central potential — a screened atomic potential, a 3-D harmonic oscillator, anything. The -degeneracy (different 's at the same ) is a much rarer, Coulomb-specific effect tied to the hidden symmetry, and it disappears the moment the potential deviates from exact .
Why do real multi-electron atoms show filling before if hydrogen's energies only depend on n?
In hydrogen, only one electron feels a pure, unscreened nuclear potential, so the accidental -degeneracy holds exactly. In multi-electron atoms, each electron feels the nucleus plus the averaged repulsion of every other electron — an effective potential that is no longer pure Coulomb. Lower- orbitals (like ) penetrate closer to the nucleus through the electron cloud more than higher- orbitals of similar (like ), so they feel less screening and are stabilized. This penetration/screening effect breaks the accidental degeneracy and produces the empirical orbital energy ordering used in the aufbau principle.
What happens to hydrogen's degeneracy under a magnetic field?
An external magnetic field along, say, the -axis picks out a preferred spatial direction, which breaks the rotational symmetry responsible for the -degeneracy itself (not just the accidental -degeneracy). The energy gains a term proportional to (the Zeeman term ), so the states of a given split into distinct, evenly spaced sublevels. This is the normal Zeeman effect, and it is a direct experimental demonstration that the -degeneracy, unlike the deeper structure of quantum mechanics, is entirely a consequence of the absence of any external symmetry-breaking field.
Does the accidental degeneracy survive relativistic corrections?
Not exactly. The non-relativistic Schrödinger treatment gives exact -degeneracy within a shell, but once you include relativistic kinetic-energy corrections and spin–orbit coupling (the Dirac equation treatment), states are labeled by total angular momentum rather than and separately, and levels with the same and but different (such as and ) remain degenerate in the pure Dirac theory — but this residual degeneracy is finally broken by quantum electrodynamic effects, the Lamb shift, measured by Lamb and Retherford in 1947. So the Coulomb accidental degeneracy is progressively (and instructively) lifted as you add more complete physics.
How is this degeneracy related to Bertrand's theorem?
Bertrand's theorem is a classical mechanics result stating that among all possible central-force laws, only the inverse-square force (, giving Kepler ellipses) and the Hooke's-law force (, the isotropic harmonic oscillator) produce closed orbits for every bound trajectory, regardless of initial conditions. This classical non-precession is the direct classical shadow of the extra conserved quantities (Runge–Lenz vector for Coulomb, a symmetric tensor for the oscillator) that, upon quantization, produce accidental degeneracy. So Bertrand's theorem essentially predicts in advance which two quantum central-potential problems will show extra (-independent) degeneracy: exactly the hydrogen atom and the 3-D isotropic harmonic oscillator.
Why is the degeneracy called "n² " and not something else?
Because summing the number of magnetic sublevels over every allowed from to is precisely the sum of the first odd numbers, , a classical arithmetic identity that equals exactly. This is not a coincidence of hydrogen specifically — it's simply the combinatorial consequence of the rule (itself derived from the radial quantization condition) combined with the universal rule that each carries magnetic sublevels. Including electron spin doubles it to , matching the shell capacities familiar from general chemistry.