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Collider

Professor Quark

Your guide at the accelerator. These are his lectures from the game, in the order you meet them.

Pixel-art portrait of Professor Quark

The story

PROF. QUARK

“Ah, there you are. Professor Quark, pleased to meet you. You've just seen how it all began – and a hundred metres beneath Geneva we bring that beginning back, in miniature: in my particle accelerator.”

PROF. QUARK

“For fifty years the Standard Model has explained almost everything: quarks, leptons, three forces. Almost. About 85% of the matter in the universe is dark, and nobody knows what it's made of.”

PROF. QUARK

“I'm certain the answer is waiting at energies nobody has reached yet. For that we need a bigger ring. And then, I'm afraid, another one.”

PROF. QUARK

“The principle: two bunches of particles race around the ring in opposite directions, near light speed. They cross inside the detector – there you make them collide. Motion becomes new particles: E = mc².”

PROF. QUARK

“Every collision delivers data, which pays for upgrades. The particles you find pay for magnets and detectors. And the higher the beam energy, the heavier the particles that can appear.”

PROF. QUARK

“The big goal: the Higgs boson. Five of them and the council approves the next ring. First the FCC, then across Europe, around the Earth, around the Moon … all the way out to the heliosphere.”

PROF. QUARK

“And somewhere out there, beyond everything we know, particles are waiting that officially don't exist. We'll find them. Together.”

How things work

PROF. QUARK

“Below is the timing bar. The dot moves in step with the particle bunches – the bright field is the moment they cross right inside the detector.”

PROF. QUARK

“Tap inside the bright field and it's a hit: full data and a chance at new particles. Miss it and the beam only hits leftover gas in the vacuum pipe: a few bytes, nothing more.”

PROF. QUARK

“A hit. At 1 MeV, though, you only get photons – massless quanta of light. Not enough energy for matter yet.”

PROF. QUARK

“An electron weighs 0.511 MeV, and it never appears alone, always with its antiparticle, the positron. That makes 1.02 MeV, the minimum the beam needs. Einstein, worked out: E = mc².”

PROF. QUARK

“One more thing: hit several crossings in a row and you build focus – more collisions per hit. One miss or a long pause and it's gone.”

PROF. QUARK

“An electron – your first piece of matter, made from pure energy. Its counterpart, the positron, was predicted by Paul Dirac and actually found in 1932.”

PROF. QUARK

“Particles are the second currency here. Data pays for the beam, particles pay for the machines – electrons, say, pay for luminosity.”

PROF. QUARK

“Luminosity means denser bunches, so more collisions – even without you, 0.2 per second per level. Your own hits stay better all the same: triple the chance at anything from uncommon up.”

PROF. QUARK

“Now the machine runs even while you fetch coffee. Time for the next goal: the pion at 140 MeV.”

PROF. QUARK

“The pion is the lightest hadron – a quark and an antiquark bound by the strong force. Hideki Yukawa predicted it in 1935 as the glue of atomic nuclei.”

PROF. QUARK

“Pions. And muons next – the electron's heavy cousins, 207 times as massive.”

PROF. QUARK

“Both pay for the magnetic field. Stronger dipole magnets keep more energetic beams on track – every level gives ×1.3 data per collision.”

PROF. QUARK

“A detector is built like an onion: layer upon layer, each one seeing different particles.”

PROF. QUARK

“Innermost the vertex detector for short-lived heavy particles, then the tracker for charged ones. The calorimeter measures energy, and outermost the muon chambers – only muons get that far.”

PROF. QUARK

“Each level of a layer makes its particle family 12% more frequent. Start with the tracker: its first levels cost just a few pions, and you'll see real tracks in the event display.”

PROF. QUARK

“Quite a collection already. Particles come in six tiers: common, uncommon, rare, epic, legendary – and mythic, the big ring goals. Every larger ring brings new, hypothetical particles.”

PROF. QUARK

“The codex tells you what each particle is and how it was discovered – and what you're still missing.”

PROF. QUARK

“At 125 GeV it gets serious: the Higgs boson. Peter Higgs predicted it in 1964; it was found in 2012 – right here at CERN.”

PROF. QUARK

“At the real LHC one appears per billion collisions. It's quicker with us, but it stays rare. The calorimeter helps: it sees the decay into two photons.”

PROF. QUARK

“Between us: when a bunch glows in colour, it carries something rare. Hit that crossing – or it's gone.”

PROF. QUARK

“Now it gets elegant: every particle oscillates at its own frequency, E = hν. In the upgrade menu, slide the beam wave exactly onto the J/ψ's and they come by the dozen. Its discovery in 1974 is still called the November Revolution.”

PROF. QUARK

“Cleanly measured. Good events get published, in four tiers: conference, paper, cover story, Nobel prize – every particle has a slot for each tier. Which tier an event reaches depends on its weakest measurement; better detectors and upgrades raise it. The codex shows what is already published.”

PROF. QUARK

“Every event you record is measured with seven values: mass, resolution, significance, √s, pile-up, rarity and trigger. You'll find them in the measurement log.”

PROF. QUARK

“Each value is compared with comparable events from the same phase of the game. “Better than 60%” means: better than 60 out of 100 comparable events.”

PROF. QUARK

“The weakest of the seven values decides: from 60% conference, from 80% paper, from 90% cover story, from 99.2% Nobel prize. One weak value holds back the whole event.”

PROF. QUARK

“Grey slots are still empty; they fill by themselves as soon as an event is good enough. For that, expand detector, resolution and trigger and keep pile-up low – tap a value to see which upgrade helps.”

At every new ring

Ring 2 · FCC ring

PROF. QUARK

“The FCC, the Future Circular Collider: 91 kilometres around, planned at CERN beneath Geneva and the lake, aiming at about 100 TeV – roughly seven times the LHC. A real plan, nothing made up.”

PROF. QUARK

“More energy means heavier particles. My colleagues suspect heavy partners of known particles, extra force carriers and signals from a dark sector that barely talks to us. None of it is proven – from here on we say “hypothetical”.”

PROF. QUARK

“New mechanic: luminosity starts at level 1 after the expansion, so the beam collides on its own from the start. Expanding resets data and upgrades; codex and mythic finds stay, and the yield rises permanently to ×1.6.”

Ring 3 · Continental ring

PROF. QUARK

“From here on we leave reality. The continental ring is fiction, nobody is planning this: 3,000 kilometres around, right across Europe, energies up to 2 PeV – more than a hundred times the LHC. Luckily, paper will put up with anything.”

PROF. QUARK

“What might turn up here? A bridge between quarks and leptons, single magnetic poles that Dirac thought possible as early as 1931, and an extremely light particle that would solve a puzzle of the strong force. All hypothetical, of course.”

PROF. QUARK

“New mechanic: double beam. Every 10th collision counts twice – double data and a second roll for new particles. The yield rises permanently to ×2.6.”

Ring 4 · Earth ring

PROF. QUARK

“The Earth ring: 40,000 kilometres, once around the equator. Fiction, but with a tradition: in 1954 Enrico Fermi worked out what an accelerator around the Earth could do. Here energies reach 200 PeV.”

PROF. QUARK

“What my colleagues suspect here: heavy siblings of the neutrinos – that would explain why the known ones are so tiny. And the quantum of gravity, the one piece quantum physics is still missing. Both hypothetical.”

PROF. QUARK

“New mechanic: the combo holds during automation. As long as luminosity runs it does not decay, and automatic collisions get the combo multiplier. Permanent yield ×4.1.”

Ring 5 · Lunar orbit ring

PROF. QUARK

“The lunar orbit ring: 2.4 million kilometres around, the Moon itself circling on the track. Fiction. 20 EeV sounds absurd, but nature does it already: cosmic rays reach even more – they just never aim.”

PROF. QUARK

“My colleagues suspect a strange transition in the weak-force field here. It might explain why matter was left over after the Big Bang instead of annihilating with antimatter. Never observed – hypothetical.”

PROF. QUARK

“New mechanic: anomalies. Every few minutes an anomaly appears on stage for 12 seconds. Tap it for a time boost (yield ×3) or a mass drop; missed ones expire without penalty. Yield ×6.6.”

Ring 6 · Solar orbit ring

PROF. QUARK

“The solar orbit ring: 940 million kilometres, Earth is just a dot on the track. Fiction, energies up to 2 ZeV. Building this takes a long breath – and a great deal of coffee.”

PROF. QUARK

“What my colleagues suspect here: heavy, long-lived particles that roll through the detector like hadrons, and the perennial favourite for dark matter – sluggish, heavy, almost never interacting. No detection so far, hypothetical.”

PROF. QUARK

“New mechanic: a second detector. As at ATLAS and CMS there are now two crossing points per lap; the beat halves, and twice as many hits are possible. Yield ×10.5.”

Ring 7 · Heliosphere ring

PROF. QUARK

“The heliosphere ring lies beyond the solar system, where the solar wind fades into interstellar gas. The Voyager probes have crossed that border – an accelerator there is fiction. Beam energy is unlimited here.”

PROF. QUARK

“Here my colleagues hope for hints about the nature of space and time: matter as tiny vibrating strings, and extra dimensions where gravity would be stronger than we think. Beautiful, but unproven – hypothetical.”

PROF. QUARK

“New mechanic: all resonances. Every particle with mass can now be produced as a resonance by tuning (±3%), the Higgs included. Yield ×16.8. And after that? After that, only the universe itself is left.”

PROF. QUARK

“The old ring (LHC ring) now serves as a pre-accelerator – like the SPS at CERN, which feeds the LHC at 450 GeV. So your beam starts at 375.8 GeV, about one fifteenth of what this ring can reach. You build the new ring up visibly with every beam level.”

When you find something hypothetical

  • Neutralino

    PROF. QUARK

    “A neutralino. The lightest partner in supersymmetry: neutral, heavy, nearly invisible – a dark matter candidate. In the detector it shows itself only as missing energy, the track that isn't there. Hypothetical, of course.”

  • Z′ boson

    PROF. QUARK

    “A Z′, the big brother of the Z boson. If there were another force, it would need another carrier. Its fingerprint: a muon pair with suspiciously high energy. The real experiments have found nothing so far – hence we build bigger.”

  • Dark photon

    PROF. QUARK

    “A dark photon – the light of a force only dark matter feels. We could see it at best because it mixes a little with the ordinary photon. Hypothetical, my colleagues say. Let's keep this between us.”

  • Leptoquark

    PROF. QUARK

    “A leptoquark – half quark, half lepton, as if two particle families had married. Grand unified theories predict it; hints in B decays have not been confirmed so far. But hope springs eternal. Hypothetical.”

  • Magnetic monopole

    PROF. QUARK

    “A magnetic monopole: a north pole without a south pole. Break a magnet and you just get two magnets. Dirac showed in 1931 that a single one would explain why electric charge comes in fixed portions. Nobody has ever seen one.”

  • Axion

    PROF. QUARK

    “An axion. Devised to explain why the neutron is so strikingly balanced electrically – and, on the side, a dark matter candidate. Very light, very shy, hypothetical. A particle that solves a problem you first had to notice.”

  • Heavy neutrino

    PROF. QUARK

    “A heavy neutrino. The known neutrinos are tiny – maybe because they have heavy siblings: the heavier the one, the lighter the others. A seesaw, and that is literally what the mechanism is called. Hypothetical.”

  • Graviton

    PROF. QUARK

    “A graviton, the quantum of gravity – the one force we still have no quantum theory for. Whoever detects a single one goes to Stockholm. In reality it is unimaginably hard to catch; hypothetical, naturally.”

  • Sphaleron

    PROF. QUARK

    “A sphaleron – not a particle but a transition in the weak-force field that treats matter and antimatter unequally. It may explain why anything was left at all. Greek: “ready to fall”. Hypothetical.”

  • R-hadron

    PROF. QUARK

    “An R-hadron: a heavy supersymmetric particle wrapped in ordinary quarks. So heavy and so long-lived that it crosses the whole detector – a lorry on the motorway. Hypothetical, my colleagues say.”

  • WIMP

    PROF. QUARK

    “A WIMP, a Weakly Interacting Massive Particle – the name says it all. For decades the favourite for dark matter, and every search so far has come up empty. Catching one is pure wishful thinking. Good thing that's allowed here.”

  • String ball

    PROF. QUARK

    “A string ball. If particles were tiny vibrating strings, enough energy could tangle a knot of them that decays into many particles. String theory is elegant but unproven. So don't take the result literally – but do take it with enthusiasm.”

  • Micro black hole

    PROF. QUARK

    “A micro black hole. Don't worry: hypothetical, and it would evaporate via Hawking radiation in a blink. If collisions could make one, cosmic rays would have done it for billions of years – and nothing happened. Did you see the light bend? Einstein's gravity.”