⚛️ Build 01 · Atomic Species Selector

Choose an Atomic Species

Compare laser-coolable atoms by the decisions an experimentalist actually faces: species choice, laser system, qubit platform, cooling strategy, and nearby papers or groups.

Species choice workflow

Use the library to make a design decision, not just to look up a number.

The same atom can be attractive for one goal and painful for another. Start with your experimental goal, then use the tables and data sheets to check whether the lasers, cooling, and coherence story are compatible.

01Choose a species

Start with mass, linewidth, recoil, hyperfine structure, and whether you need alkali or alkaline-earth physics.

02Compare platforms

Map species to tweezers, clocks, molecules, Rydberg gates, quantum gases, and imaging constraints.

03Design lasers

Use wavelengths and linewidths to plan cooling, repump, trapping, clock, and Rydberg beams.

04Find groups and papers

Jump from species to canonical data sheets, representative labs, and literature trails.

🧪 Periodic Table Explorer

The 15 isotopes in this library come from nine elements, lit up below. Pick one to see its numbers, energy levels, data sheets and the groups that use it, or colour the whole table by a property to see the periodic trends behind choosing a species.

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Energy levels

Schematic: level spacings are not to scale.

These are representative US groups, organized by their primary atom. The full directory, with a map, is the AMO Group Finder.

📋 All 15 isotopes at a glance

Filter:
Atom Z A Statistics Family Cool. λ (nm) Γ/2π (MHz) T_D (μK) 2E_r/k_B (μK) Nuclear spin I HF split (GHz) Key notes
⁶Li 36 Fermion Alkali 671.05.871417.08 10.228 Strong Feshbach res.; Li-Cs molecules
⁷Li 37 Boson Alkali 671.05.871416.07 3/20.804 Early BEC; light mass → large recoil
²³Na 1123 Boson Alkali 589.09.802352.40 3/21.772 First BEC (Ketterle 1995, Nobel 2001)
³⁹K 1939 Boson Alkali 767.06.041450.84 3/20.462 Feshbach res.; Fermi-Hubbard model
⁴⁰K 1940 Fermion Alkali 767.06.041450.82 41.286 Fermionic isotope; degenerate Fermi gas
⁴¹K 1941 Boson Alkali 767.06.041450.80 3/20.254 Less common; BEC demonstrated
⁸⁵Rb 3785 Boson Alkali 780.26.071460.36 5/23.036 Feshbach res. for tuneable interactions
⁸⁷Rb 3787 Boson Alkali 780.26.071460.36 3/26.835 Most popular qubit (6.8 GHz clock)
¹³³Cs 55133 Boson Alkali 852.35.231250.20 7/29.193 Defines the SI second; Li-Cs molecules
⁸⁸Sr 3888 Boson Alkaline Earth 461.032.07700.46 0— Narrow 689 nm line → T_D = 0.18 μK; optical clock
⁸⁷Sr 3887 Fermion Alkaline Earth 461.032.07700.46 9/2— 10 nuclear spin states; SU(N) physics
¹⁷⁴Yb 70174 Boson Alkaline Earth 399.028.06720.36 0— 556 nm narrow line → T_D = 4.4 μK; mHz clock transition
¹⁷¹Yb 70171 Fermion Alkaline Earth 399.028.06720.36 1/2— Effective spin-1/2 qubit; clock QC
¹⁶⁴Dy 66164 Boson Magnetic 421.0——— 0— Largest magnetic moment (10 μ_B); dipolar physics
¹⁶⁸Er 68168 Boson Magnetic 401.0——— 0— Large magnetic moment (7 μ_B); anisotropic interactions

T_D = Doppler temperature limit  |  2E_r/k_B = absorption-plus-emission recoil scale [single recoil is half this value]  |  HF = ground-state hyperfine splitting  | , = not applicable or varies by isotope. Broad-line T_D shown for all atoms; for alkaline-earth atoms the listed recoil scale is for the narrow intercombination line used for final cooling.

📈 Visual Comparison

Doppler Temperature T_D (μK), broad cooling line
Natural Linewidth Γ/2π (MHz), broad cooling line
Alkali Alkaline Earth
Note on alkaline-earth narrow lines: Sr-88 and Sr-87 have a narrow 689 nm intercombination line with Γ/2π = 7.6 kHz, giving a Doppler limit of T_D = 0.18 μK, far below the broad-line value shown above. Yb has a 556 nm intercombination line with Γ/2π = 182 kHz, giving T_D = 4.4 μK, far below the broad-line value shown in the table. These narrow lines enable sub-Doppler temperatures without requiring sub-Doppler stages (polarization-gradient cooling etc.).

📚 Essential Resources & Tools

Data compiled from Steck data sheets, NIST ASD, and primary literature · All links open in a new tab

See Also