The Cast of Characters for the Big Bang

The primary cast of characters for the big bang includes:

  • Photons ("particles" of light)
  • Protons and neutrons
  • Electrons and their antiparticles the positrons
  • Neutrinos and their antiparticles the antineutrinos
  • At the very earliest times, there are other more fundamental particles such as quarks and gluons that participated, but by a fraction of a second after "the bang" (as astronomers call the big bang) the cast had been reduced to the above simple list. Let us now follow the approximate sequence of events that took place in the big bang in terms of the time since the expansion begins.

    Antiparticles and Antimatter

    Every elementary particle in the Universe appears to have a partner particle called its antiparticle that shares many of the same characteristics, but many other characteristics are the opposite of those for the particle. For example, the electron has as its antiparticle the antielectron (also called the positron). The electron and the antielectron have exactly the same masses, but they have exactly opposite electrical charges. A particle and its antiparticle are termed a pair. (Some particles are their own antiparticles. For example, the antiparticle of a photon is itself a photon.) The common stuff around us appears to be "matter" (matter composed of particles), but we produce small quantities of antimatter (matter composed of antiparticles) routinely in high energy accelerator experiments.

    Pair Annihilation
    When a matter particle meets its antimatter partner they destroy each other completely (the technical term is "pair annihilation"), releasing the equivalent of their rest masses in the form of pure energy (according to the Einstein energy-mass relation). For example, when an electron meets an antielectron, the two annihilate and produce a burst of light having the energy corresponding to the masses of the two particles.
    Pair Creation
    But the opposite reaction occurs also: two photons can give up their energy to form a particle-antiparticle pair. This process is called pair creation. Pair annihilation and pair creation are illustrated in the adjacent figure. These types of reactions play very important roles in the big bang. Because there was so much energy available, the very early universe was a seething inferno of pair creation reactions converting photons to particle-antiparticle pairs and of particle-antiparticle pairs annihilating to create photons.

    Matter and Antimatter Worlds
    Because the properties of matter and antimatter parallel each other, we believe that the physics and chemistry of a galaxy made entirely from antimatter would closely resemble that of a matter galaxy. Thus, it is conceivable that life built on antimatter could have evolved at other places in the Universe, just as life based on matter has evolved here. (But if your antimatter twin should show up some day, I would advise against shaking hands--remember that matter and antimatter annihilate each other!) However, we have no evidence thus far for large concentrations of antimatter anywhere in the Universe. Everything that we see so far on large scales seems to be matter, and we only see antimatter produced for short times in violent collisions. This is something of a mystery, because naively there are reasons from fundamental physics to believe that the Universe should have produced about as much matter as antimatter. We shall return to this mystery later.