For a while in the early twentieth century, the universe looked simple: protons and neutrons in the nucleus, electrons around it, photons for light. Then cosmic-ray detectors and particle accelerators began revealing new particles by the dozen. Physicists eventually organized them into a single framework, the Standard Model, which describes all known matter using a handful of truly fundamental particles and three of the four fundamental forces. It is one of the most thoroughly tested theories in science.
The four fundamental forces
| Force | Acts on | Range | Relative strength | Carrier particle |
|---|---|---|---|---|
| Strong nuclear | Quarks (and so protons and neutrons) | About the size of a nucleus, | Strongest | Gluon |
| Electromagnetic | Charged particles | Unlimited, weakening with distance | Second | Photon |
| Weak nuclear | All quarks and leptons | Much smaller than a nucleus | Third | W⁺, W⁻ and Z bosons |
| Gravity | Everything with mass or energy | Unlimited, weakening with distance | Weakest by far | Graviton (proposed, never detected; not part of the Standard Model) |
In the Standard Model a force is an exchange of force-carrying particles, called gauge bosons. Two electrons repel by exchanging photons; quarks are held together by exchanging gluons; the weak force, carried by the heavy W and Z bosons, is responsible for beta decay and lets one type of quark change into another. Gravity is so feeble between individual particles that it plays no role in particle physics: the electric repulsion between two protons is more than times their gravitational attraction.
Matter particles: quarks and leptons
| Generation | Quarks (charge +2/3) | Quarks (charge −1/3) | Charged leptons (charge −1) | Neutrinos (charge 0) |
|---|---|---|---|---|
| 1st | up (u) | down (d) | electron | electron neutrino |
| 2nd | charm (c) | strange (s) | muon | muon neutrino |
| 3rd | top (t) | bottom (b) | tau | tau neutrino |
There are twelve matter particles, in three generations. Each generation is a heavier copy of the one before, and the heavier particles quickly decay, so the ordinary matter around you is built almost entirely from the first: up quarks, down quarks and electrons. Quarks feel the strong force and carry fractional charges. They also carry a property called colour charge (nothing to do with visible colour), and they are confined: no one has ever isolated a single quark, because pulling two apart puts so much energy into the gluon field that new quark-antiquark pairs form instead. Leptons do not feel the strong force. Neutrinos are neutral and interact so rarely that most pass straight through Earth; the Sudbury Neutrino Observatory, deep in a mine near Sudbury, Ontario, helped show that neutrinos change type as they travel, which means they have mass, earning Arthur McDonald a share of the 2015 Nobel Prize in Physics. The final piece, the Higgs boson, is associated with the field that gives fundamental particles their mass; it was discovered at CERN in 2012.
Hadrons: baryons and mesons
- Proton: uud, charge
- Neutron: udd, charge
- Baryon number (each quark counts )
- The proton is the only one that is stable on its own
- Example: the positive pion is , charge
- Baryon number (quark , antiquark )
- All are unstable and decay quickly
- First found in cosmic rays and accelerator collisions
Hadrons are all the particles built from quarks held together by the strong force. The two families differ in their recipe. A baryon is three quarks; a meson is a quark bound to an antiquark. To find a hadron's charge, just add the charges of its quarks — an antiquark has the opposite charge of its quark, so an anti-down quark has charge . Every combination that actually exists adds up to a whole-number charge.
Antimatter, pair creation and annihilation
Every particle has an antiparticle with the same mass and the opposite charge. The antielectron, or positron (), was predicted by Paul Dirac's theory and found by Carl Anderson in cosmic rays in 1932. Relativity's lets energy and matter trade places. In pair creation, a high-energy gamma photon passing close to a nucleus turns into an electron and a positron; the nucleus is needed to absorb some momentum. In annihilation, a particle meets its antiparticle and both vanish, their mass-energy leaving as photons — for an electron and a positron at rest, two gamma photons flying off in opposite directions so that total momentum stays zero. PET medical scanners detect exactly these pairs of photons.