Aluminium energy level diagram
Energy levels and transitions of neutral aluminium (Al I): the 45 strongest classified lines below 2 µm from the NIST Atomic Spectra Database and the 33 levels they connect, each line with its vacuum wavelength, frequency and, for 45 of them, the reduced dipole matrix element derived from the NIST transition rate. Measured lifetimes, transition rates, hyperfine constants and isotope shifts from the literature are included, each with its citation.
Hover a line or a level to isolate it, click to keep it selected. Scroll to zoom, drag to move.

Download: diagram (PDF) diagram (SVG) transitions (CSV) levels (CSV) source code
Key transitions of aluminium
| Transition | λ vac (nm) | λ air (nm) | ν (THz) | |⟨J‖er‖J′⟩| (ea₀) | A (s⁻¹) | Γ/2π up. (MHz) | branch (%) | Use |
|---|---|---|---|---|---|---|---|---|
| 3p 2P°3/2 – 3d 2D5/2 | 309.3606 | 309.2708 | 969.0712 | 2.495 | 7.100e+07 | 11.37 | 99.4 | 309.4 nm laser-cooling transition 3p 2P3/2 |
| 3p 2P°1/2 – 4s 2S1/2 | 394.5122 | 394.4006 | 759.9066 | 1.688 | 4.700e+07 | 23.23 | 32.2 | 394.4 nm resonance line |
| 3p 2P°3/2 – 4s 2S1/2 | 396.2641 | 396.1520 | 756.5471 | 2.466 | 9.900e+07 | 23.23 | 67.8 | 396.2 nm line |
λ, ν from NIST level energies unless a measured frequency for this isotope is available. A: measured value or NIST. Γ/2π: natural linewidth of the upper level, 1/(2πτ).
27Al hyperfine structure (I = 5/2)
| Level | A (MHz) | B (MHz) | Shift of each F level from the centre of gravity (MHz) |
|---|---|---|---|
| 3p 2P°1/2 | 502.0346(5) | – | F=2: -878.56 F=3: +627.54 |
| 3p 2P°3/2 | 94.27723(10) | 18.915 | F=1: -481.71 F=2: -308.29 F=3: -33.97 F=4: +358.27 |
| 4s 2S1/2 | 431.11(9) | – | F=2: -754.44 F=3: +538.89 |
| 4p 2P°1/2 | 58.280 | – | F=2: -101.99 F=3: +72.85 |
| 4p 2P°3/2 | 23.120 | 2.860 | F=1: -119.38 F=2: -75.43 F=3: -7.35 F=4: +87.42 |
Measured A, B constants; sources in the data file.
Isotope shifts
| Transition | λ vac (nm) | Isotopes | Shift (MHz) |
|---|---|---|---|
| 3p 2P°3/2 – 4s 2S1/2 | 396.264 | 26m-27 | 378(3) |
| 3p 2P°3/2 – 4s 2S1/2 | 396.264 | 28-27 | -321.9(8) |
| 3p 2P°3/2 – 4s 2S1/2 | 396.264 | 29-27 | -610.7(6) |
| 3p 2P°3/2 – 4s 2S1/2 | 396.264 | 30-27 | -889.5(12) |
| 3p 2P°3/2 – 4s 2S1/2 | 396.264 | 31-27 | -1141.0(12) |
| 3p 2P°3/2 – 4s 2S1/2 | 396.264 | 32-27 | -1401(7) |
Shift = ν(first isotope) − ν(second isotope).
Closed and nearly closed transitions of aluminium
| Transition | λ vacuum (nm) | Lower level | A (s⁻¹) | Leak per scattered photon | Photons before a leak | Where the leak goes |
|---|---|---|---|---|---|---|
| 3p 2P°3/2 → 3d 2D5/2 | 309.3606 | metastable | 7.100e+07 measured | closed | – | no other level can be reached by electric-dipole decay |
| 3p 2P°3/2 → 9d 2D5/2 | 213.5407 | metastable | 1.810e+07 NIST | 0.931 % from semi-empirical calc. | 107 | 4p 2P°3/2 ≈ 0.802 %; 7p 2P°3/2 ≈ 4.69 × 10−4; 7f 2F°7/2 ≈ 1.45 × 10−4; 13 weaker lines |
| 3p 2P°3/2 → 5d 2D5/2 | 226.9798 | metastable | 6.910e+07 measured | 1.05 % from NIST data | 95 | 6p 2P°3/2 0.598 %; 4p 2P°3/2 0.382 %; 5f 2F°7/2 4.03 × 10−4; 4 weaker lines |
| 3p 2P°3/2 → 10d 2D5/2 | 212.4030 | metastable | 1.220e+07 NIST | 1.13 % from semi-empirical calc. | 88 | 4p 2P°3/2 ≈ 0.995 %; 7p 2P°3/2 ≈ 3.08 × 10−4; 5p 2P°3/2 ≈ 2.58 × 10−4; 15 weaker lines |
| 3p 2P°3/2 → 6d 2D5/2 | 221.0749 | metastable | 5.200e+07 NIST | 1.37 % from semi-empirical calc. | 73 | 4p 2P°3/2 1 %; 7p 2P°3/2 0.245 %; 5p 2P°3/2 6.66 × 10−4; 7 weaker lines |
| 3p 2P°3/2 → 7d 2D5/2 | 217.4752 | metastable | 3.530e+07 NIST | 1.73 % from semi-empirical calc. | 58 | 4p 2P°3/2 1.45 %; 5p 2P°3/2 0.201 %; 4f 2F°7/2 ≈ 2.69 × 10−4; 9 weaker lines |
| 3p 2P°3/2 → 8d 2D5/2 | 215.1376 | metastable | 2.460e+07 NIST | 2.18 % from semi-empirical calc. | 46 | 4p 2P°3/2 1.74 %; 5p 2P°3/2 0.307 %; 6p 2P°3/2 7.08 × 10−4; 11 weaker lines |
| 3p 2P°3/2 → 4d 2D5/2 | 237.3847 | metastable | 6.310e+07 measured | 2.93 % from NIST data | 34 | 5p 2P°3/2 2.55 %; 4p 2P°3/2 0.216 %; 4f 2F°7/2 0.162 %; 1 weaker lines |
A transition is closed when its upper level can decay only to the level it was excited from, so the atom keeps scattering photons. “closed”: among the levels NIST lists, no other level below the upper level has the opposite parity and |ΔJ| ≤ 1, so no other electric-dipole decay exists. Otherwise the leak is the sum of the branching ratios of the other decay lines of the upper level (or 1 − branching ratio where that of the line itself has been measured), and the number of photons is 1 / leak. “≥” and “≤”: at least one possible decay path has no listed rate, so the leak is a lower limit. These numbers are derived from the branching ratios, lifetimes and rates of this page, not measured as such; the tag names the weakest of the inputs, * marks theory and ≈ a model or semi-empirical calculation. Listed: lines that start on the ground level or on a metastable level and leak at most 10 %, unless more than three possible decay paths have no listed rate. Fine-structure levels only: hyperfine and Zeeman dark states and forbidden decays without a listed rate are not considered. Select a line in the diagram for the full list of its leak channels.
Listed Al transitions below 2 µm
| Lower level | Upper level | λ vacuum (nm) | λ air (nm) | ν (THz) | Type | |⟨J‖er‖J′⟩| (ea₀) | A (s⁻¹) | Branching (%) | Source of matrix element / A |
|---|---|---|---|---|---|---|---|---|---|
| 3p 2P°1/2 | 10d 2D3/2 | 211.8986 | 211.8316 | 1414.7920 | E1 | 0.440 NIST | 1.030e+07 NIST | – | NIST ASD (accuracy C) |
| 3p 2P°3/2 | 10d 2D5/2 | 212.4030 | 212.3359 | 1411.4325 | E1 | 0.588 NIST | 1.220e+07 NIST | – | NIST ASD (accuracy C) |
| 3p 2P°3/2 | 10d 2D3/2 | 212.4030 | 212.3359 | 1411.4325 | E1 | 0.195 NIST | 2.000e+06 NIST | – | NIST ASD (accuracy D) |
| 3p 2P°1/2 | 9d 2D3/2 | 213.0335 | 212.9663 | 1407.2549 | E1 | 0.539 NIST | 1.520e+07 NIST | – | NIST ASD (accuracy C) |
| 3p 2P°3/2 | 9d 2D5/2 | 213.5407 | 213.4733 | 1403.9128 | E1 | 0.722 NIST | 1.810e+07 NIST | – | NIST ASD (accuracy C) |
| 3p 2P°3/2 | 9d 2D3/2 | 213.5433 | 213.4760 | 1403.8954 | E1 | 0.240 NIST | 3.000e+06 NIST | – | NIST ASD (accuracy D) |
| 3p 2P°1/2 | 8d 2D3/2 | 214.6230 | 214.5555 | 1396.8326 | E1 | 0.634 NIST | 2.060e+07 NIST | – | NIST ASD (accuracy C) |
| 3p 2P°3/2 | 8d 2D5/2 | 215.1376 | 215.0699 | 1393.4920 | E1 | 0.852 NIST | 2.460e+07 NIST | – | NIST ASD (accuracy C) |
| 3p 2P°3/2 | 8d 2D3/2 | 215.1405 | 215.0728 | 1393.4731 | E1 | 0.284 NIST | 4.090e+06 NIST | – | NIST ASD (accuracy E) |
| 3p 2P°1/2 | 7d 2D3/2 | 216.9507 | 216.8827 | 1381.8461 | E1 | 0.772 NIST | 2.960e+07 NIST | – | NIST ASD (accuracy C) |
| 3p 2P°3/2 | 7d 2D5/2 | 217.4752 | 217.4071 | 1378.5132 | E1 | 1.037 NIST | 3.530e+07 NIST | – | NIST ASD (accuracy C) |
| 3p 2P°3/2 | 7d 2D3/2 | 217.4794 | 217.4113 | 1378.4866 | E1 | 0.346 NIST | 5.880e+06 NIST | – | NIST ASD (accuracy E) |
| 3p 2P°1/2 | 8s 2S1/2 | 219.9869 | 219.9183 | 1362.7739 | E1 | 0.136 NIST | 1.750e+06 NIST | – | NIST ASD (accuracy C) |
| 3p 2P°3/2 | 8s 2S1/2 | 220.5306 | 220.4618 | 1359.4144 | E1 | 0.192 NIST | 3.490e+06 NIST | – | NIST ASD (accuracy C) |
| 3p 2P°1/2 | 6d 2D3/2 | 220.5355 | 220.4668 | 1359.3839 | E1 | 0.962 NIST | 4.370e+07 NIST | – | NIST ASD (accuracy C+) |
| 3p 2P°3/2 | 6d 2D5/2 | 221.0749 | 221.0060 | 1356.0672 | E1 | 1.290 NIST | 5.200e+07 NIST | – | NIST ASD (accuracy C+) |
| 3p 2P°3/2 | 6d 2D3/2 | 221.0819 | 221.0130 | 1356.0244 | E1 | 0.430 NIST | 8.670e+06 NIST | – | NIST ASD (accuracy C+) |
| 3p 2P°1/2 | 7s 2S1/2 | 225.8706 | 225.8007 | 1327.2751 | E1 | 0.207 NIST | 3.770e+06 NIST | – | NIST ASD (accuracy C) |
| 3p 2P°1/2 | 5d 2D3/2 | 226.4165 | 226.3464 | 1324.0753 | E1 | 1.149 measured | 5.760e+07 measured | 80.6 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°3/2 | 7s 2S1/2 | 226.4438 | 226.3737 | 1323.9156 | E1 | 0.293 NIST | 7.500e+06 NIST | – | NIST ASD (accuracy C) |
| 3p 2P°3/2 | 5d 2D5/2 | 226.9798 | 226.9096 | 1320.7892 | E1 | 1.547 measured | 6.910e+07 measured | 96.7 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°3/2 | 5d 2D3/2 | 226.9924 | 226.9222 | 1320.7158 | E1 | 0.515 measured | 1.150e+07 measured | 16.1 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°1/2 | 4d 2D3/2 | 236.7775 | 236.7052 | 1266.1357 | E1 | 1.174 measured | 5.260e+07 measured | 69.4 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°1/2 | 6s 2S1/2 | 237.2794 | 237.2070 | 1263.4577 | E1 | 0.276 NIST | 5.760e+06 NIST | 27.7 | NIST ASD (accuracy C) |
| 3p 2P°3/2 | 4d 2D5/2 | 237.3847 | 237.3122 | 1262.8974 | E1 | 1.581 measured | 6.310e+07 measured | 83.3 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°3/2 | 4d 2D3/2 | 237.4074 | 237.3350 | 1262.7762 | E1 | 0.527 measured | 1.050e+07 measured | 13.9 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°3/2 | 6s 2S1/2 | 237.9120 | 237.8394 | 1260.0982 | E1 | 0.389 NIST | 1.140e+07 NIST | 54.9 | NIST ASD (accuracy C+) |
| 3p 2P°1/2 | nd y 2D3/2 | 256.8752 | 256.7982 | 1167.0744 | E1 | 0.801 measured | 1.920e+07 measured | 56.6 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°3/2 | nd y 2D5/2 | 257.5865 | 257.5094 | 1163.8515 | E1 | 1.079 measured | 2.300e+07 measured | 67.8 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°3/2 | nd y 2D3/2 | 257.6167 | 257.5396 | 1163.7149 | E1 | 0.358 measured | 3.800e+06 measured | 11.2 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°1/2 | 5s 2S1/2 | 265.3265 | 265.2476 | 1129.9000 | E1 | 0.512 measured | 1.420e+07 measured | 28.1 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°3/2 | 5s 2S1/2 | 266.1178 | 266.0386 | 1126.5405 | E1 | 0.727 measured | 2.840e+07 measured | 56.2 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°1/2 | 3d 2D3/2 | 308.3046 | 308.2151 | 972.3904 | E1 | 1.848 measured | 5.900e+07 measured | 82.6 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°3/2 | 3d 2D5/2 | 309.3606 | 309.2708 | 969.0712 | E1 | 2.495 measured | 7.100e+07 measured | 99.4 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°3/2 | 3d 2D3/2 | 309.3735 | 309.2837 | 969.0309 | E1 | 0.838 measured | 1.200e+07 measured | 16.8 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°1/2 | 4s 2S1/2 | 394.5122 | 394.4006 | 759.9066 | E1 | 1.688 measured | 4.700e+07 measured | 32.2 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 3p 2P°3/2 | 4s 2S1/2 | 396.2641 | 396.1520 | 756.5471 | E1 | 2.466 measured | 9.900e+07 measured | 67.8 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 4s 2S1/2 | 6p 2P°3/2 | 555.8603 | 555.7059 | 539.3306 | E1 | 0.279 NIST | 2.300e+05 NIST | 11.1 | NIST ASD (accuracy C) |
| 4s 2S1/2 | 6p 2P°1/2 | 555.9488 | 555.7944 | 539.2447 | E1 | 0.197 NIST | 2.290e+05 NIST | 11.2 | NIST ASD (accuracy C) |
| 4s 2S1/2 | 5p 2P°3/2 | 669.7867 | 669.6018 | 447.5940 | E1 | 0.770 NIST | 1.000e+06 NIST | 27.5 | NIST ASD (accuracy C+) |
| 4s 2S1/2 | 5p 2P°1/2 | 670.0517 | 669.8667 | 447.4169 | E1 | 0.545 NIST | 1.000e+06 NIST | 27.5 | NIST ASD (accuracy C+) |
| 3d 2D3/2 | 4f 2F°5/2 | 1125.6271 | 1125.3189 | 266.3337 | E1 | 7.410 NIST | 1.300e+07 NIST | 78.5 | NIST ASD (accuracy A) |
| 3d 2D5/2 | 4f 2F°7/2 | 1125.7962 | 1125.4880 | 266.2937 | E1 | 8.849 NIST | 1.390e+07 NIST | 84 | NIST ASD (accuracy A) |
| 4s 2S1/2 | 4p 2P°3/2 | 1312.7007 | 1312.3417 | 228.3784 | E1 | 8.184 measured | 1.500e+07 measured | 97.5 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
| 4s 2S1/2 | 4p 2P°1/2 | 1315.4345 | 1315.0748 | 227.9038 | E1 | 5.996 measured | 1.600e+07 measured | 96.8 | Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,… |
Reduced dipole matrix elements follow the convention A = ω³|d|²/(3πε₀ħc³(2J′+1)), with J′ the upper level. Tags show where a number comes from: measured, NIST compilation, high-accuracy theory, a semi-empirical calculation (Kurucz line list, used only where no measurement or NIST value exists; typically within a factor 2), or a model calculation.
Al energy levels
Al⁺ ionisation limit 48278.48 cm⁻¹ = 5.98577 eV (207.132 nm)
Sources
- Heylen et al., Phys. Rev. C 103, 014318 (2021) (arXiv:2010.06918), Sec. III ("A(S1/2) = 4…
- NIST ASD
- NIST ASD level energies
- Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,…
- Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,…
- Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,…
- Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,…
- Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,…
- Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,…
- Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 5,…
- Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 6,…
- Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 6,…
- Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 6,…
- Papoulia, Ekman, Jonsson, Astron. Astrophys. 621, A16 (2019) (arXiv:1808.09478), Table 6,…
- Sur, Chaudhuri, Das, Mukherjee, arXiv:physics/0504087v2 (2005), "Case studies of atomic p…
- Sur, Chaudhuri, Das, Mukherjee, arXiv:physics/0504087v2 (2005), "Case studies of atomic p…
- Sur, Chaudhuri, Das, Mukherjee, arXiv:physics/0504087v2 (2005), "Case studies of atomic p…
- Sur, Chaudhuri, Das, Mukherjee, arXiv:physics/0504087v2 (2005), "Case studies of atomic p…
27Al (I = 5/2) is the only stable isotope; the isotope shifts listed on the 396 nm line are for radioactive 26m,28-32Al measured at ISOLDE/IGISOL, with delta-nu(27,A) = nu(A) - nu(27). Measured lifetimes and transition rates are quoted from the comparison tables of Papoulia, Ekman, Jonsson (2019), which name the original experiments; their accuracy grades (A <= 3%, B <= 10%, C+ <= 15%, C <= 25%, D <= 50%) are copied into the source string instead of a numeric unc. When a line has two observed values, the more recent laser measurement (Davidson 1990 / Vujnovic 2002) is the main entry. Lifetime alternatives marked theory are RCI length-form values of the same paper. rme_J_ea0 for the 3p-4s lines is sqrt(S) from a relativistic coupled-cluster calculation (same convention as the schema). Extra fields beyond SCHEMA.md: isotope_shift_factors, use_source, ionization_energy, mu_N, unc_sys.
Atoms with measured data
- Lithium-632 levels, 85 lines
- Lithium-732 levels, 85 lines
- Beryllium-917 levels, 26 lines
- Sodium-2336 levels, 106 lines
- Magnesium-2418 levels, 61 lines
- Magnesium-2518 levels, 61 lines
- Potassium-3934 levels, 84 lines
- Potassium-4034 levels, 84 lines
- Potassium-4134 levels, 84 lines
- Calcium-4035 levels, 61 lines
- Calcium-4335 levels, 61 lines
- Chromium-5256 levels, 87 lines
- Chromium-5356 levels, 87 lines
- Rubidium-8536 levels, 94 lines
- Rubidium-8736 levels, 94 lines
- Strontium-8440 levels, 70 lines
- Strontium-8640 levels, 70 lines
- Strontium-8740 levels, 70 lines
- Strontium-8840 levels, 70 lines
- Cadmium-11115 levels, 21 lines
- Cadmium-11315 levels, 21 lines
- Cadmium-11415 levels, 21 lines
- Caesium-13331 levels, 79 lines
- Barium-13744 levels, 89 lines
- Barium-13844 levels, 89 lines
- Dysprosium-16139 levels, 55 lines
- Dysprosium-16239 levels, 55 lines
- Dysprosium-16339 levels, 55 lines
- Dysprosium-16439 levels, 55 lines
- Erbium-16673 levels, 90 lines
- Erbium-16773 levels, 90 lines
- Erbium-16873 levels, 90 lines
- Thulium-16972 levels, 73 lines
- Ytterbium-17118 levels, 26 lines
- Ytterbium-17318 levels, 26 lines
- Ytterbium-17418 levels, 26 lines
- Mercury-19927 levels, 47 lines
- Mercury-20127 levels, 47 lines
- Mercury-20227 levels, 47 lines