INGENIA

ATM-33

Doppler width

Thermal broadening.

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AtomicDoppler

Governing equation

Δν/ν=2kTln2/mc2\Delta\nu/\nu=\sqrt{2kT\ln2/mc^2}

where

T
T (K)
m
Mass (u)
\Delta\nu/\nu
Fraction ()

Lecture brief

Historical brief

Balmer, Rydberg, Bohr (1913), fine structure, Zeeman and Stern–Gerlach built the spectrum of one atom. The lab computes levels, selection and magnetic splitting. This sheet (ATM-33 — Doppler width) is the form associated with Doppler. Working symbols: TT, mm \rightarrow Δν/ν\Delta\nu/\nu. Thermal broadening.

Purpose

Purpose: compute Δν/ν\Delta\nu/\nu from TT, mm in Atomic physics via Δν/ν=2kTln2/mc2\Delta\nu/\nu=\sqrt{2kT\ln2/mc^2} Thermal broadening. Use it when a real atomic physics question must be answered in SI before a code check.

Live realistic example

In symbols

Live case. Given T=5000.000KT = 5000.000\,\mathrm{K}, m=1.000um = 1.000\,\mathrm{u}, the governing relation Δν/ν=2kTln2/mc2\Delta\nu/\nu=\sqrt{2kT\ln2/mc^2} yields Δν/ν=2.532e5\Delta\nu/\nu = 2.532e-5\,\mathrm{—}. Thermal broadening. Move a slider: the numbers are this situation, not a canned story.

Calculator

Inputs

Outputs

  • Fraction \Delta\nu/\nu0.00002532
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ATM-33 · spectrum
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Narration of this film

Thermal broadening.

Thermal broadening.

Reading speed

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