Skip to main content
Sandbox Physics

Neutrinos · D09 · Water and geometry

Cherenkov Light & Detector Rings

When does a cone of light become a ring? When it hits a surface lined with light sensors. The particle's speed sets the opening angle of the cone. Its direction and its distance from that surface then decide where the light lands, and so the shape and size of the ring you record.

Set a charged particle’s speed and tilt, then follow its light to a flat square detector. Move the emission point to see which parts of the pattern come from the cone’s geometry and which come from the detector’s finite size.

Interactive modelCherenkov Light & Detector Rings
Cherenkov half-angle—\text{—}
Speed threshold · fraction of vacuum light speed—\text{—}
Recorded rays—\text{—}
Outside the finite plane—\text{—}
Normal-incidence reference radius—\text{—}
Mean recorded optical path—\text{—}

Recorded data from a teaching simulation

Inspect the measurement

Preparing a reproducible teaching record…

Read a sample of the record

Physics tutorial

A cone meets a measurement plane

BackgroundThe detector plane faces along positive z; x is horizontal and y is vertical, all in metres. The charged particle moves in the plane spanned by x and z. Its small emission region sits at z equal to zero, shifted sideways by the chosen offset.

Why it mattersWhat changes the cone of light itself, and what only changes the pattern it leaves on the detector?

Start with the essentials

Focus question
What changes the cone of light itself, and what only changes the pattern it leaves on the detector?
One-sentence intuition
The particle’s speed sets the Cherenkov angle; the track’s tilt and the distance to the detector set the shape you record.

Core mathematical model

Cherenkov angle and speed threshold

cos⁡θC=1nβ,nβ>1\cos\theta_C=\frac{1}{n\beta},\qquad n\beta>1

The speed ratio here is the particle’s speed divided by the speed of light in vacuum. Below the threshold this model emits no light. The refractive index is taken to be the same at every wavelength.

Where each ray meets the plane, and the radius at normal incidence

rD=r0+zDkzk,Rα=0=zDtan⁡θC\mathbf r_D=\mathbf r_0+\frac{z_D}{k_z}\mathbf k,\qquad R_{\alpha=0}=z_D\tan\theta_C

The ray’s unit direction is k. Only rays that travel forward and land inside the square are recorded. The radius for a track perpendicular to the plane stays on screen as a reference even when the track is tilted; it is not fitted to the ring.

Common difficulties

A cone meets a measurement plane

Typical misconceptionThe ring is a picture of the neutrino itself.

Better mental modelThe ring is light from a charged particle that the neutrino produced. Working back to the neutrino also takes the kinematics of the interaction and the detector response.

Run the experiment

  1. 01

    Cross the threshold

    Choose Below threshold. Raise the speed until light appears.

    What to observe: The cone opens from zero angle. Above threshold the model always samples the same number of rays, so the brightness tells you nothing about how much light a real particle gives off.
  2. 02

    Tilt the cone

    Choose Tilted cone and compare the apparatus with the recorded plane.

    What to observe: A tilted cone leaves a shifted, stretched pattern, and the edge of the square can cut part of it off.
  3. 03

    Change distance only

    Return to Centered ring and double the emission-to-plane distance.

    What to observe: The ring’s radius doubles while the cone angle stays the same, until the ring runs past the edge of the square.

Related experiments and articles

Continue exploring

How detectors see a neutrino

A neutrino leaves only light, charge or a pair of signals close in time. How does each detector turn that into a direction, an energy or a source?

  1. LabReactor Antineutrino CoincidenceSelect prompt and delayed signals against accidental pairs.
  2. You are hereCherenkov Light & Detector RingsTurn charged-particle geometry into a recorded light pattern.
  3. LabLiquid Argon Time Projection ChamberTurn electron arrival times and wire projections into calibrated slice centroids.
  4. LabIceCube: From Sensor Hits to a TrackInfer a track direction from the recorded sensor times.
  5. LabSupernova Neutrino Burst ObservatoryScan a frozen burst record, then inspect one interaction at the optical timescale.
  6. LabNeutrino Sky Search ObservatorySearch frozen neutrino directions and compare a local hotspot with paired finite-grid background trials.

Neutrinos · Reading path

Make a source and test its journey

Articles on this path that use this experiment, followed by the other experiments they suggest.

  1. ArticleHow do you make a beam of particles you cannot steer?
  2. LabLong-Baseline CP Observatory
  3. LabNeutrino Flavor Propagation
  4. ArticleK2K and MINOS: test flavor change with a distance you choose
  5. ArticleT2K: why look slightly away from the beam axis?
  6. ArticleHyper-K: a larger target still needs a precise comparison

Neutrinos · Reading path

Start with the prize

Articles on this path that use this experiment, followed by the other experiments they suggest.

  1. Article2026 Nobel Prize in Physics: why look for neutrinos in Antarctic ice?
  2. LabIceCube: From Sensor Hits to a Track
  3. ArticleFive ways a neutrino headline can lead us astray
  4. ArticleWhy do neutrinos keep appearing in the Nobel Prize?
  5. LabReactor Antineutrino Coincidence
5 more groups

Neutrinos · Reading path

Build a new way to observe the sky

Articles on this path that use this experiment, followed by the other experiments they suggest.

  1. ArticleSN 1987A: a supernova seen from underground
  2. LabSupernova Neutrino Burst Observatory
  3. LabReactor Antineutrino Coincidence
  4. ArticleBefore IceCube: learning to build telescopes in water and ice
  5. LabIceCube: From Sensor Hits to a Track
  6. ArticleIceCube: how do you turn a cubic kilometre of ice into an instrument?

Neutrinos · Reading path

What happened to the Sun’s neutrinos?

Articles on this path that use this experiment, followed by the other experiments they suggest.

  1. ArticleHow do you know those neutrinos came from the Sun?
  2. LabSolar Neutrino Flavor Observatory
  3. ArticleSNO: where did the Sun’s missing neutrinos go?

Neutrinos · Reading path

Understand flavor change and mass

Articles on this path that use this experiment, followed by the other experiments they suggest.

  1. ArticleHow does the atmosphere make neutrinos all around us?
  2. LabAtmospheric Neutrino Zenith Experiment
  3. ArticleSuper-Kamiokande: the neutrinos that took the long way

Neutrinos · Reading path

Follow the measurement chain

Articles on this path that use this experiment, followed by the other experiments they suggest.

  1. ArticleWater, scintillator and argon: what does each detector see?
  2. LabLiquid Argon Time Projection Chamber
  3. LabReactor Antineutrino Coincidence

Particles and detectors · Reading path

Detecting a passing particle

Articles on this path that use this experiment, followed by the other experiments they suggest.

  1. ArticleCherenkov follows the blue light to a moving charge
FeedbackSomething broken, confusing, or missing on this page?Tell us
What kind of feedback?

Sent with this page’s address, its Lab ID, the site language and your device type. Please leave out personal details. Feedback is kept for up to 12 months.Privacy policy