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Optical Tweezers

Radiation pressure on a sphere from exact Mie theory — asymmetry parameter, pressure cross-section, scattering force — plus trap stiffness and depth for a focused Gaussian beam in the Rayleigh regime.

v0.1.0·Updated 2026-07-18
Model & Assumptions Beta
Model
Exact Mie: σpr = σext − gσsca with g = ⟨cosθ⟩ from the Mie coefficients (Bohren & Huffman §4.5); F = nhostσprI/c. Trap: Rayleigh (dipole) gradient force in a TEM₀₀ Gaussian focus — U = −βI with β = (2πnhosta³/c)·Re[(m²−1)/(m²+2)]; κr = 4βI₀/w₀², κz = 2βI₀/zR².
Assumptions
Homogeneous sphere; paraxial Gaussian beam (peak irradiance 2P/πw₀²); Minkowski photon momentum in the host medium. Trap numbers use the dipole approximation — trusted for 2a ≲ λ/(5nhost), flagged otherwise.
Limitations
No generalized Lorenz–Mie (beam-shape) coefficients: outside the dipole regime, stiffness and depth are indicative only. Gradient force uses Re(n) of absorbing particles; heating of absorbing particles is the Photothermal tool's job.
Parameters

Trapping criterion. A trap is usually considered stable when the depth exceeds ~10 kBT, so Brownian kicks rarely eject the particle. The radius chart marks that line.

κr pN/μm
κz pN/μm
Depth kBT
Fscat fN
Radiation pressure spectrum — Qpr and g
Trap depth vs radius at λtrap
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