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Sandbox Physics

E34 · Electron spectroscopy

EELS: Energy Loss & Thin-Specimen Signals

Move a probe across a carbon-rich inclusion, collect transmitted electrons and read two spectrum windows. Separate the zero-loss peak, repeated plasmon losses and a carbon core edge. Balance collection, energy sampling, resolution and exposure before accepting a thin-specimen result.

Interactive modelEELS: Energy Loss & Thin-Specimen Signals
Assumed relative thickness—\text{—}
Recorded-window log ratio—\text{—}
Two or more low-loss events0 %0\,\mathrm{\%}
Core counts minus known background—\text{—}
Expected edge SNR · known background—\text{—}
Expected low-loss window coverage0 %0\,\mathrm{\%}
Experiment target—\text{—}

Physics tutorial

Read a spectrum before naming a material

BackgroundA transmitted electron can reach the detector without measurable loss, lose energy to a collective excitation, or excite an inner-shell electron. A spectrometer sorts those outcomes by energy.

Why it mattersAn edge is useful only if collection, energy response, sampling and specimen thickness support its interpretation.

Start with the essentials

Focus question
What did the transmitted electrons lose?
One-sentence intuition
Zero loss does not mean no elastic scattering. Repeated low-loss events shift and broaden core-edge information, while detector dispersion and energy resolution describe different limits.

Core mathematical model

Repeated loss orders

Pn=μne−μn!,μ=tλP_n=\frac{\mu^n e^{-\mu}}{n!},\qquad \mu=\frac{t}{\lambda}

Independent inelastic events give a zero-loss fraction and a plural-loss population. The mean free path here is an assumed teaching input.

Relative thickness from counts

(tλ) ⁣app=ln⁡IwindowIZLP\left(\frac{t}{\lambda}\right)_{\!\mathrm{app}}=\ln\frac{I_{\mathrm{window}}}{I_{\mathrm{ZLP}}}

Both integrals use the recorded low-loss bins. The finite spectral window and finite zero-loss integration can bias the result, especially with broad response or thick specimens. Absolute thickness also needs a calibrated mean free path.

The instrument broadens, pixels integrate

σE=ΔEFWHM8ln⁡2,Cj=Ninc∫Ej−Ej+p(E) dE\sigma_E=\frac{\Delta E_{\mathrm{FWHM}}}{\sqrt{8\ln2}},\qquad C_j=N_{\mathrm{inc}}\int_{E_j^-}^{E_j^+}p(E)\,\mathrm dE

Resolution and dispersion differ: narrowing detector bins does not undo an already broad energy response. Every bin integrates probability before counting noise is drawn.

A core event can be followed by low losses

Score(E)∝∑n=0∞Pn [S1∗Gn](E−16n eV)S_{\mathrm{core}}(E)\propto\sum_{n=0}^{\infty}P_n\,[S_1*G_n](E-16n\,\mathrm{eV})

This rare-core-event teaching approximation redistributes an edge toward higher loss. The synthetic onset and feature can be shifted, but no actual oxidation state is inferred. Known model-background subtraction gives an optimistic SNR reference.

Common difficulties

An edge shift is not a diagnosis

Typical misconceptionAny shifted edge names a unique oxidation state.

Better mental modelThese are invented near-edge shapes. Chemical identification requires references, calibration and a suitable scattering model.

Run the experiment

  1. 01

    Thin, then thicken

    Compare Thin · resolved with Plural scattering. Watch the low-loss orders and compare assumed thickness with the recorded-window estimate.

    What to observe: Multiple losses grow and redistribute the core signal. A finite low-loss window can lose part of the tail.
  2. 02

    Separate sampling from response

    Keep the specimen thin; compare 0.25 and 2 eV per pixel, then change the energy response from 1 to 6 eV.

    What to observe: Fine bins preserve a narrow feature only if the instrument response is already narrow.
  3. 03

    Locate the signal

    Move the probe out of the C-rich region, then restore it. Try the synthetic shift preset.

    What to observe: The core edge weakens outside the inclusion. The low-loss mean stays fixed because this toy specimen shares the same mean free path.
  4. 04

    Complete the target

    Achieve the stated thinness, sampling, response and expected SNR requirements, then check.

    What to observe: Known-background SNR is an optimistic reference. Real fitting, detector response and material cross sections need additional evidence.