NEUPLAY

Play, visualize and learn real physics — neutrino oscillations, sky surveys, particle colliders and relativity. No install, works on desktop and mobile.

Games

Each game is built around a real piece of physics.

Visualize

Interactive plots: move the sliders and watch the physics change.

Learn

The physics behind each game, in a few minutes.

Neutrino oscillations

Neutrinos come in three flavours — electron, muon and tau. Each flavour is a quantum mixture of three mass states, which travel with slightly different phases. As a neutrino flies, the mixture drifts, so a neutrino born as one flavour can be detected as another. The chance depends on distance L and energy E through sin²(1.27 Δm² L / E). The discovery earned the 2015 Nobel Prize and proved neutrinos have mass.

Telescopes, sources and transients

A telescope only sees a small patch of sky — its field of view. Faint steady sources need long exposures to build up enough signal, while transients such as gamma-ray bursts, supernovae and fast radio bursts flash for seconds to days. Survey astronomers trade off a wide field (find more) against depth (see fainter), exactly the choice you make with the field-of-view control.

How the LHC works
  • Dipole magnets (1232 of them, at 8.3 tesla) bend the protons around the 27 km ring.
  • Quadrupole magnets squeeze the beam like lenses so it doesn't spread out.
  • RF cavities give the protons a kick on every lap, up to 6.8 TeV per beam.
  • Protons arrive pre-accelerated from a chain of smaller machines ending with the SPS at 450 GeV.
  • Two beams counter-rotate and collide inside ATLAS, CMS, ALICE and LHCb.
Special relativity near light speed

Nothing with mass reaches the speed of light c. As speed v grows, the Lorentz factor γ = 1/√(1 − v²/c²) grows without limit. Moving objects are measured shorter along their motion by 1/γ (length contraction), moving clocks run slow by γ (time dilation), and starlight bunches up ahead and shifts blue (aberration and Doppler shift). At 99.5% of c, γ ≈ 10: a 10-light-year trip lasts only about a year on board.

Cosmic-ray air showers

Cosmic rays are protons and atomic nuclei from space, some carrying more energy than any particle accelerator can reach. When one hits a nucleus high in the atmosphere, around 15–30 km up, it makes a spray of pions. Neutral pions decay at once into two photons, which start an electromagnetic cascade: photons turn into electron–positron pairs, and electrons radiate new photons, doubling the number of particles roughly every radiation length (37 g/cm² of air). Charged pions either hit another nucleus or decay into muons, which reach the ground. The shower grows until the particles' energy drops to about 85 MeV, the depth of shower maximum Xmax, then dies away. A 1 PeV proton makes about a million particles at its maximum. Iron nuclei start their showers higher, reaching Xmax sooner and making more muons, which is how observatories such as Pierre Auger and LHAASO work out what cosmic rays are made of.

Careers in science, maths and medicine

A science and maths background opens many doors. After high school, a bachelor's degree (B.Sc., B.Tech or MBBS) can lead straight to work as an engineer, developer, analyst or doctor. A master's or medical residency leads to specialist roles such as data scientist, chip designer, cardiologist or surgeon. A Ph.D. and postdoc lead to research and professorships, and an MBA moves scientists and engineers into management.

Wormholes in Lightspeed are science fiction: they are allowed by general relativity's equations, but none has ever been observed.

Create

Make your own physics graphics and download them.

Connect

Questions, ideas for new games, or found a bug? Send a message.

Career tree

Where can science and maths take you? Start at high school and click to follow a path through bachelor's, master's and Ph.D. to the jobs at the end. The number on each step counts the careers reachable from it.

Paths are typical examples, not the only routes: many people switch fields, and degree names vary by country.