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Particle Physics and Cosmology in Physics

This topic asks the smallest question and the largest one at the same time. What is matter made of, and how did it get here. The answers turn out to be connected, because the conditions in the first moments of the universe were energetic enough to produce every kind of particle, and the account of that early history is tested against the particles that exist today. Along the way physics had to give up on some comfortable ideas, since protons and neutrons are not fundamental, quarks cannot be pulled out on their own, and ordinary matter turns out to be a small minority of what the universe contains. The blocks give the four forces and how the carrier mass sets their range, the annihilation and pair production relations, the classification of particles with the conservation laws that govern them, the quark picture, and the cosmic results that follow from an expanding universe.

The Fundamental Forces in Nature
Range of a force from the mass of its exchange particle

Given

  • (J s)
  • (kg)
  • (m/s)

Constant used

Energy released when a particle and its antiparticle annihilate

Given

  • (kg)
  • (m/s)

Constant used

Minimum photon energy for pair production

Given

  • (kg)
  • (Hz)
  • (m/s)

Constant used

Positrons and Other Antiparticles
Mesons and the Beginning of Particle Physics
Classification of Particles
Conservation Laws
Charge of a hadron from its quark composition

Given

Strange Particles and Strangeness
Finding Patterns in the Particles
Quarks
Multicolored Quarks
The Standard Model
Hubble's law relating distance and recession speed

Given

  • (1/s)
  • (Mpc)

Constant used

Critical density of the universe

Given

  • (1/s)
  • (N m²/kg²)

Constants used

Age of the universe from the Hubble constant

Given

  • (1/s)

Constant used

The Cosmic Connection
Problems and Perspectives