Kinetic energy at the grid
The accelerating field adds energy at a steady rate, and each excitation takes away the same fixed quantum. Below threshold there are no inelastic losses.
Q026 · Electrons losing energy to atoms
Why can a higher voltage make the current drop? Once the electrons have enough energy to excite the gas atoms, they lose it in inelastic collisions. Too slow to climb the small retarding voltage in front of the collector, they no longer reach it, and the current drops. The dips repeat each time the voltage rises by one more excitation energy, about every 4.9 volts for mercury.
Accelerate electrons through a gas and count how many reach the collector. Look at a single collision, scan the voltage and measure the spacing between the dips in current.
02 / What did the particles do?
· Blue: current sample. Amber: the most recently saved other sample. Drag to choose the probe point.
At the selected probe point
For a fixed injected flux, the recorded fraction equals the size of the normalized collector current. 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.
Inside the model · separate 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 / Save the evidence
Up to eight saved samples. Restoring one brings back its original settings and records; acquiring again starts a new run. The CSV also holds the 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 how many reach the collector. Look at a single collision, scan the voltage and measure the spacing between the dips in current.
Why it mattersA particle trades energy with an atom or a photon. Count what happens, then check whether a simpler explanation would also fit.
Start with the essentials
The accelerating field adds energy at a steady rate, and each excitation takes away the same fixed quantum. Below threshold there are no inelastic losses.
The current is normalized to a fixed injected flux. With the source unchanged, raising the retarding barrier can only turn back more electrons.
The estimate assumes an electron excites an atom almost as soon as it reaches threshold. A finite path before each collision, the spread of source energies and the discrete voltage steps all shift the observed minima.
Typical misconceptionThe collector measured every collision along the way.
Better mental modelThe collector only records whether each electron arrived. Collision positions and energies are shown separately as model diagnostics.
Typical misconceptionIf the simulation works, a real instrument has been calibrated.
Better mental modelElectrons fly forward in one dimension, and the gas has a single excitation channel at 4.9 eV. Above that threshold, the chance of a collision per unit distance is a fixed constant. Counts are simulated. The model leaves out elastic deflection, electrons caught by the grid, ionization, space charge and calibrated mercury cross sections.
Before scanning, predict whether raising the voltage always increases the collected current.
What to observe: The data panel starts empty. Record some data before you interpret anything.Scan the voltage and save the result, then repeat with the gas removed. Look at one electron flight at a current dip and another where the current has recovered.
What to observe: An electron can lose energy exciting an atom and then pick up energy again before it reaches the grid.Increase the contact offset and mark neighboring valleys before and after the shift. Then broaden the source energy spread.
What to observe: The voltage where the dips begin and the spacing between them are different quantities. Choose broad or coarsely sampled valleys with care.Quantum evidence · Reading path
Articles on this path that use this experiment, followed by the other experiments they suggest.