Energy ledger
Uniform acceleration adds energy, and every excitation subtracts the same quantum. There are no inelastic losses below threshold.
Q026 · Collisions / energy / current
Accelerate electrons through a gas and count those that reach the collector. Inspect a collision, scan the voltage, and measure the spacing between current dips.
02 / WHAT DID THE PARTICLES DO?
· Blue: active sample. Amber: last other saved sample. Drag to select the probe.
AT THE SELECTED PROBE
Recorded fraction equals normalized collector-current magnitude for a fixed injected flux. Whiskers are pointwise 95% Wilson intervals.
03 / MEASURE THE SPACING
Click a recorded scan point in the chart below. Choose neighboring valleys yourself; the cursors do not consult the excitation energy.
Only cursors on recorded scan voltages produce a spacing. This manual difference has grid and valley-selection uncertainty; it is not an automatic excitation-energy fit.
MODEL INSPECTION · DISTINCT FROM THE READOUT
· Last simulated flight at this voltage. Drops are actual collision events from its saved record; this diagnostic is not measured by the collector.
04 / KEEP THE EVIDENCE
Eight frozen samples. Restoring preserves the original settings and records. Acquiring again starts a new run. CSV also contains simulated collision or recoil diagnostics.
The 1D accelerating region has uniform field; x runs from cathode to grid. Emission energies follow an exponential flux distribution. Excitation has a constant hazard per unit forward distance above threshold; each event removes one energy quantum. The collector accepts energies above the retarding barrier. Below the contact offset we clamp the accelerating field to zero; we do not model reversed extraction. The ideal reference assumes vanishing excitation flight length, not the finite-hazard data model. Neither curve is calibrated mercury data. Gas density is controlled by optical depth, independently of the source energy scale.
Physics tutorial
BackgroundAccelerate electrons through a gas and count those that reach the collector. Inspect a collision, scan the voltage, and measure the spacing between current dips.
Why it mattersA particle exchanges energy with an atom or a photon. Count the consequences, then test a simpler explanation.
Start with the essentials
Uniform acceleration adds energy, and every excitation subtracts the same quantum. There are no inelastic losses below threshold.
Current magnitude is normalized to a fixed injected flux. Increasing the retarding barrier can only reject more electrons at fixed preparation.
The short-excitation-flight limit motivates the spacing estimate. Finite collision paths, source energy spread and a voltage grid move the observed minima.
Typical misconceptionThe collector measured every collision along the way.
Better mental modelThe collector gives a yes/no result. Collision locations and energies are explicitly exposed model diagnostics.
Typical misconceptionA successful simulation calibrates a physical instrument.
Better mental modelA one-dimensional forward-flight model with a single 4.9 eV excitation channel and a declared constant collision hazard above threshold. Counts are simulated. No elastic deflection, grid interception, ionization, space charge or calibrated mercury cross sections.
Before scanning, predict whether raising voltage always increases collected current.
What to observe: The data panel begins empty. Record a sample before interpreting it.Scan voltage, save, then repeat without gas. Inspect one electron at a valley and another after the current recovers.
What to observe: An electron can lose energy to excitation and then regain energy before the grid.Increase contact offset. Mark neighboring observed valleys before and after the shift. Then broaden the source.
What to observe: Absolute onset is not the same observable as spacing. Broad or poorly sampled valleys need careful selection.