Atomic energy level diagrams

Mercury-199 energy level diagram

Energy levels and transitions of neutral 199Hg (Hg I, nuclear spin I = 1/2): the 47 strongest classified lines below 2 µm from the NIST Atomic Spectra Database and the 27 levels they connect, each line with its vacuum wavelength, frequency and, for 46 of them, the reduced dipole matrix element. Level energies come from NIST and refer to the natural isotope mixture; transition rates are 43 NIST, 3 measured, 1 HFR fit (this site). Hyperfine constants and measured frequencies are those of this isotope.

Hover a line or a level to isolate it, click to keep it selected. Scroll to zoom, drag to move.

Mercury-199 energy level diagram with transition wavelengths and dipole matrix elements

Download: diagram (PDF) diagram (SVG) transitions (CSV) levels (CSV) source code

Key transitions of 199Hg

Transitionλ vac (nm)λ air (nm)ν (THz)|⟨J‖er‖J′⟩| (ea₀)A (s⁻¹)Γ/2π up. (MHz)branch (%)Use
5d106s2 1S0 – 5d106s6p 1P°1184.9499–1620.93832.6407.440e+08118.899.7184.9 nm resonance line
5d106s2 1S0 – 5d106s6p 3P°1253.7283253.65211181.54910.4407.992e+061.272100253.7 nm intercombination line: MOT / cooling, optical pu…
5d106s2 1S0 – 5d106s6p 3P°0265.6380265.55891128.5753–6.920e-011.101e-07100265.6 nm optical lattice clock transition
5d106s6p 3P°1 – 5d106s8s 1S0285.7770285.69301049.04340.1131.100e+061.8959.24285.7 nm
5d106s6p 3P°0 – 5d106s6d 3D1296.8150296.72831010.03151.3354.600e+07––296.7 nm
5d106s6p 3P°1 – 5d106s6d 3D2312.6579312.5673958.85132.2316.600e+0714.7471.3312.7 nm
5d106s6p 3P°1 – 5d106s6d 3D1313.2462313.1555957.0505≈1.7897.036e+07––313.2 nm, optical pumping out of the 253.7 nm MOT
5d106s6p 3P°2 – 5d106s6d 3D3365.1198365.0158821.07974.6581.290e+08––365.0 nm
5d106s6p 3P°0 – 5d106s7s 3S1404.7707404.6564740.64761.4262.070e+0719.4117404.7 nm
5d106s6p 3P°1 – 5d106s7s 1S0407.8988407.7837734.96770.3664.000e+065.13412.4407.8 nm
5d106s6p 3P°1 – 5d106s7s 3S1435.9561435.8336687.66662.6215.600e+0719.4145.9435.8 nm
5d106s6p 1P°1 – 5d106s8s 1S0491.7418491.6045609.65430.5835.800e+061.89548.7491.6 nm
5d106s6p 3P°2 – 5d106s7s 3S1546.2267546.0750548.84253.4394.900e+0719.4140.2546.1 nm
5d106s6p 1P°1 – 5d106s7s 1S01014.25671013.9787295.57853.7362.710e+075.134841014 nm
5d106s6p 1P°1 – 5d106s7s 3S11207.49001207.1596248.27740.9133.200e+0519.410.2621207 nm intercombination branch of 7s 3S1

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).

Isotope shifts

Transitionλ vac (nm)IsotopesShift (MHz)
5d106s2 1S0 – 5d106s6p 3P°1253.728196-1984179.95(3)
5d106s2 1S0 – 5d106s6p 3P°1253.728200-198-4805.52(4)
5d106s2 1S0 – 5d106s6p 3P°1253.728202-198-10101.224(22)
5d106s2 1S0 – 5d106s6p 3P°1253.728204-198-15311.60(4)
5d106s2 1S0 – 5d106s6p 3P°1253.728199-198-652(6)
5d106s2 1S0 – 5d106s6p 3P°1253.728201-198-6410(6)
5d106s2 1S0 – 5d106s6p 3P°0265.638199-2015729.668(8)
5d106s2 1S0 – 5d106s6p 3P°0265.638198-199654.48
5d106s6p 3P°1 – 5d106s6d 3D2312.658196-198-289.4(12)
5d106s6p 3P°1 – 5d106s6d 3D2312.658200-198328.0(6)
5d106s6p 3P°1 – 5d106s6d 3D2312.658202-198686.7(6)
5d106s6p 3P°1 – 5d106s6d 3D2312.658204-1981038.3(6)
5d106s6p 3P°1 – 5d106s6d 3D1313.246196-198-307.5(10)
5d106s6p 3P°1 – 5d106s6d 3D1313.246200-198347.2(6)
5d106s6p 3P°1 – 5d106s6d 3D1313.246202-198725.5(6)
5d106s6p 3P°1 – 5d106s6d 3D1313.246204-1981097.8(6)

Shift = ν(first isotope) − ν(second isotope).

Closed and nearly closed transitions of 199Hg

Transitionλ vacuum (nm)Lower levelA (s⁻¹)Leak per scattered photonPhotons before a leakWhere the leak goes
5d106s2 1S0 → 5d106s6p 1P°1184.9499ground7.440e+08 measuredclosed–no other level can be reached by electric-dipole decay
5d106s2 1S0 → 5d106s6p 3P°1253.7283ground7.992e+06 measuredclosed–no other level can be reached by electric-dipole decay
5d106s6p 3P°2 → 5d106s6d 3D3365.1198metastable1.290e+08 NIST≥ 0.141 % from this site's HFR fit≤ 7095d96s26p 2[3/2]°2 ≈ 0.141 %; 5d106s7p 3P°2 ≈ 6.04 × 10−6; 1 more possible path without a listed rate

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 199Hg transitions below 2 µm

Lower levelUpper levelλ vacuum (nm)λ air (nm)ν (THz)Type|⟨J‖er‖J′⟩| (ea₀)A (s⁻¹)Branching (%)Source of matrix element / A
5d106s2 1S05d106s6p 1P°1184.9499–1620.9383E12.640 measured7.440e+08 measured99.7Porsev, Safronova, Safronova, 'A theoretical study of the g-factor and lifetime of the 6s…
5d106s6p 3P°05d106s8d 3D1237.9050237.83241260.1353E10.268 NIST3.600e+06 NIST–NIST ASD (accuracy D)
5d106s2 1S05d106s6p 3P°1253.7283253.65211181.5491E1 (intercombination)0.440 measured7.992e+06 measured100Gravina, Clivati, Castrillo, Fasci, Chishti, Galzerano, Levi, Gianfrani, 'Measurement of …
5d106s6p 3P°15d106s7d 3D2265.2832265.20421130.0848E11.340 NIST3.900e+07 NIST–NIST ASD (accuracy B+)
5d106s6p 3P°15d106s7d 1D2265.5920265.51301128.7706E1 (intercombination)0.713 NIST1.100e+07 NIST42.4NIST ASD (accuracy B)
5d106s2 1S05d106s6p 3P°0265.6380265.55891128.5753clock–6.920e-01 measured100Porsev, Safronova, Safronova, 'A theoretical study of the g-factor and lifetime of the 6s…
5d106s6p 3P°05d106s8s 3S1275.3596275.27821088.7309E10.434 NIST6.100e+06 NIST–NIST ASD (accuracy B)
5d106s6p 3P°15d106s8s 1S0285.7770285.69301049.0434E1 (intercombination)0.113 NIST1.100e+06 NIST9.24NIST ASD (accuracy D+)
5d106s6p 3P°15d106s8s 3S1289.4448289.36001035.7499E10.751 NIST1.570e+07 NIST–NIST ASD (accuracy B+)
5d106s6p 3P°25d106s9s 3S1292.6269292.54131024.4871E10.545 NIST8.000e+06 NIST–NIST ASD (accuracy D)
5d106s6p 3P°05d106s6d 3D1296.8150296.72831010.0315E11.335 NIST4.600e+07 NIST–NIST ASD (accuracy D)
5d106s6p 3P°25d106s7d 3D3302.2384302.1504991.9072E12.206 NIST5.100e+07 NIST–NIST ASD (accuracy B+)
5d106s6p 3P°25d106s7d 3D2302.4355302.3475991.2607E10.801 NIST9.400e+06 NIST–NIST ASD (accuracy B)
5d106s6p 3P°25d106s7d 1D2302.8370302.7489989.9465E1 (intercombination)0.368 NIST1.980e+06 NIST7.62NIST ASD (accuracy C+)
5d106s6p 3P°15d106s6d 3D2312.6579312.5673958.8513E12.231 NIST6.600e+07 NIST71.3NIST ASD (accuracy B+)
5d106s6p 3P°15d106s6d 3D1313.2462313.1555957.0505E11.789 HFR fit (this site)7.036e+07 HFR fit (this site)–This site: Cowan-code HFR calculation of Hg I with the parameters fitted to the NIST ener…
5d106s6p 3P°25d106s8s 3S1334.2444334.1483896.9258E10.964 NIST1.680e+07 NIST–NIST ASD (accuracy B+)
5d106s6p 3P°25d106s6d 3D3365.1198365.0158821.0797E14.658 NIST1.290e+08 NIST–NIST ASD (accuracy B+)
5d106s6p 3P°25d106s6d 3D2365.5884365.4843820.0272E11.490 NIST1.840e+07 NIST19.9NIST ASD (accuracy B)
5d106s6p 3P°25d106s6d 3D1366.3930366.2887818.2264E10.512 NIST3.600e+06 NIST–NIST ASD (accuracy C)
5d106s6p 3P°05d106s7s 3S1404.7707404.6564740.6476E11.426 NIST2.070e+07 NIST17NIST ASD (accuracy B)
5d106s6p 3P°15d106s7s 1S0407.8988407.7837734.9677E1 (intercombination)0.366 NIST4.000e+06 NIST12.4NIST ASD (accuracy B)
5d106s6p 1P°15d106s9s 1S0410.9214410.8054729.5616E10.275 NIST2.200e+06 NIST31.2NIST ASD (accuracy D)
5d106s6p 1P°15d106s7d 3D2434.0443433.9223690.6956E1 (intercombination)0.765 NIST2.900e+06 NIST–NIST ASD (accuracy C+)
5d106s6p 1P°15d106s7d 1D2434.8717434.7495689.3814E11.306 NIST8.400e+06 NIST32.3NIST ASD (accuracy B)
5d106s6p 3P°15d106s7s 3S1435.9561435.8336687.6666E12.621 NIST5.600e+07 NIST45.9NIST ASD (accuracy B)
5d106s6p 1P°15d106s8s 1S0491.7418491.6045609.6543E10.583 NIST5.800e+06 NIST48.7NIST ASD (accuracy D+)
5d106s6p 1P°15d106s8s 3S1502.7032502.5631596.3607E1 (intercombination)0.0709 NIST2.670e+04 NIST–NIST ASD (accuracy B)
5d106s6p 3P°25d106s7s 3S1546.2267546.0750548.8425E13.439 NIST4.900e+07 NIST40.2NIST ASD (accuracy B)
5d106s6p 1P°15d106s6d 3D2577.1210576.9609519.4621E1 (intercombination)3.346 NIST2.360e+07 NIST25.5NIST ASD (accuracy B)
5d106s6p 1P°15d106s6d 3D1579.1286578.9680517.6613E1 (intercombination)0.415 NIST6.000e+05 NIST–NIST ASD (accuracy D)
5d106s6p 1P°15d106s6d 1D2579.2276579.0670517.5728E13.856 NIST3.100e+07 NIST33.8NIST ASD (accuracy D)
5d106s7s 3S15d96s26p 2[3/2]°1607.4340607.2658493.5392E10.141 NIST6.000e+04 NIST–NIST ASD (accuracy E)
5d106s7s 3S15d106s8p 3P°2690.9367690.7462433.8928E11.141 NIST1.600e+06 NIST–NIST ASD (accuracy D)
5d106s6p 1P°15d106s7s 1S01014.25671013.9787295.5785E13.736 NIST2.710e+07 NIST84NIST ASD (accuracy B+)
5d106s7s 3S15d106s7p 1P°11118.00111117.6950268.1504E1 (intercombination)2.767 NIST3.700e+06 NIST–NIST ASD (accuracy D)
5d106s7s 3S15d106s7p 3P°21129.05421128.7451265.5253E111.31 NIST3.600e+07 NIST–NIST ASD (accuracy D)
5d106s6p 1P°15d106s7s 3S11207.49001207.1596248.2774E1 (intercombination)0.913 NIST3.200e+05 NIST0.262NIST ASD (accuracy D)
5d96s26p 2[3/2]°25d106s7d 3D31213.15911212.8272247.1172E13.767 NIST2.300e+06 NIST–NIST ASD (accuracy D)
5d106s7p 3P°05d106s7d 3D11321.38031321.0190226.8783E14.527 NIST6.000e+06 NIST–NIST ASD (accuracy D)
5d106s7p 3P°15d106s7d 3D21343.00221342.6351223.2256E15.467 NIST5.000e+06 NIST–NIST ASD (accuracy D)
5d106s7p 3P°15d106s7d 3D11347.23371346.8654222.5245E13.404 NIST3.200e+06 NIST–NIST ASD (accuracy E)
5d106s7p 3P°15d106s7d 1D21350.95571350.5864221.9114E1 (intercombination)4.272 NIST3.000e+06 NIST11.6NIST ASD (accuracy D)
5d106s7s 1S05d106s7p 1P°11357.45261357.0814220.8493E114.91 NIST6.000e+07 NIST–NIST ASD (accuracy D)
5d106s7s 3S15d106s7p 3P°11367.71251367.3386219.1926E112.61 NIST4.200e+07 NIST–NIST ASD (accuracy D)
5d106s7s 3S15d106s7p 3P°01395.42981395.0484214.8388E18.189 NIST5.000e+07 NIST–NIST ASD (accuracy D)
5d106s7s 3S15d96s26p 2[3/2]°21529.96321529.5452195.9475E19.860 NIST1.100e+07 NIST–NIST ASD (accuracy D)

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, this site's own Cowan-code calculation with the parameters fitted to the NIST energies (HFR fit; inputs and fit report in the repository folder cowan/; used only where nothing else gives a rate; strong lines typically within a factor 2, weak lines worse), or a model calculation.

199Hg energy levels

LevelEnergy (cm⁻¹)JParityLifetimegJHyperfine A (MHz)Hyperfine B (MHz)Lifetime sourceHyperfine source
5d106s2 1S00.0000evenstable–––––
5d106s6p 3P°037644.9820odd1.445 s measured–––Porsev, Safronova, Safronova, 'A theoretical study of the g-factor and lifetime of the 6s…–
5d106s6p 3P°139412.2371odd125.1 ns measured1.4861––Gravina, Clivati, Castrillo, Fasci, Chishti, Galzerano, Levi, Gianfrani, 'Measurement of …–
5d106s6p 3P°244042.9092odd–1.501––––
5d106s6p 1P°154068.6831odd1.34 ns measured1.0145––Porsev, Safronova, Safronova, 'A theoretical study of the g-factor and lifetime of the 6s…–
5d106s7s 3S162350.3251even8.2 ns measured2.0029––Mosburg & Wilke, 'Some new transition probabilities for mercury I', J. Quant. Spectrosc. …–
5d106s7s 1S063928.1200even31 ns measured–––Mosburg & Wilke, 'Some new transition probabilities for mercury I', J. Quant. Spectrosc. …–
5d96s26p 2[3/2]°268886.4302odd––––––
5d106s7p 3P°069516.5760odd––––––
5d106s7p 3P°169661.8031odd––––––
5d106s7p 3P°271207.2962odd––––––
5d106s7p 1P°171294.8601odd––––––
5d106s6d 1D271333.0532even10.9 ns measured1.058––Mosburg & Wilke, 'Some new transition probabilities for mercury I', J. Quant. Spectrosc. …–
5d106s6d 3D171336.0051even–0.49864––––
5d106s6d 3D271396.0732even10.8 ns measured1.1091––Mosburg & Wilke, 'Some new transition probabilities for mercury I', J. Quant. Spectrosc. …–
5d106s6d 3D371431.1803even–1.3343––––
5d106s8s 3S173961.1351even–2.0038––––
5d106s8s 1S074404.5600even84 ns measured–––Mosburg & Wilke, 'Some new transition probabilities for mercury I', J. Quant. Spectrosc. …–
5d106s8p 3P°276823.4302odd–1.4825––––
5d106s7d 1D277063.9702even38.5 ns measured1.0219––Mosburg & Wilke, 'Some new transition probabilities for mercury I', J. Quant. Spectrosc. …–
5d106s7d 3D177084.4201even–0.4996––––
5d106s7d 3D277107.8072even–1.1465––––
5d106s7d 3D377129.3723even–1.3306––––
5d106s9s 3S178216.1201even–2.0088––––
5d106s9s 1S078404.2400even142 ns measured–––Mosburg & Wilke, 'Some new transition probabilities for mercury I', J. Quant. Spectrosc. …–
5d96s26p 2[3/2]°178813.0201odd–1.2103––––
5d106s8d 3D179678.5701even––––––

Hg⁺ ionisation limit 84184.15 cm⁻¹ = 10.43750 eV (118.787 nm)

Sources

Conventions. (1) Isotope-shift keys 'a-b' mean nu(a) - nu(b); the 253.7 nm and 313 nm shifts are relative to 198Hg as printed. 199Hg / 201Hg shifts of the 253.7 nm line are hyperfine centres of gravity corrected by Schelfhout & McFerran for the second-order hyperfine interaction. (2) Clock frequencies exceed double precision: use value_Hz_str / unc_Hz. frequency_THz_<A> carries further isotopes. (3) Fields beyond SCHEMA.md: natural_linewidth_*, hyperfine_component_frequencies, frequency_ratios, magic_frequency_MHz, g_factor_<A>Hg (g of the J=0 clock state, x1 not x1e3), top-level 'rydberg' (ionization limit) and 'conflicts'. (4) A_s, linewidth and rme_J_ea0 of the 253.7 nm line are derived here from the measured lifetime (schema convention, single decay channel). (5) Only the 201Hg magnetic hyperfine constants could be sourced; the 199Hg values are missing (see not_found).

Atoms with measured data

All elements: periodic table