- Electroweak force
- The unified force combining electromagnetism and the weak nuclear force, shown by Weinberg, Glashow, and Salam in 1967 to be a single force that appears as two distinct forces at low energies.
- Higgs field
- A quantum field filling all of space whose non-zero vacuum value gives mass to particles that interact with it (like W and Z bosons) while leaving the photon massless.
- Higgs boson
- The particle associated with excitations (ripples) of the Higgs field, discovered at CERN on July 4, 2012; has spin-0 and mass of ~125 GeV.
- Baryogenesis
- The hypothetical set of physical processes in the early universe that produced a slight excess of matter (baryons) over antimatter, explaining why the universe is not empty.
- WIMP
- Weakly Interacting Massive Particle — the leading class of dark matter candidate; a heavy particle that interacts only via gravity and the weak force, making it very hard to detect.
- QCD (Quantum Chromodynamics)
- The currently accepted quantum field theory of the strong nuclear force, describing how quarks are bound together by gluons inside protons and neutrons.
- Quantum field theory (QFT)
- The theoretical framework combining quantum mechanics and special relativity; it treats every particle type as an excitation of an underlying field that permeates all of space.
- Casimir effect
- A measurable attractive force between two uncharged metal plates placed very close together in a vacuum, caused by the difference in virtual particle density inside versus outside the gap.
- Electroweak symmetry breaking
- The process at 10^-12 seconds after the Big Bang when the Higgs field switched on, giving mass to the W and Z bosons while leaving the photon massless, splitting the electroweak force into electromagnetism and the weak force.
- Grand Unified Theory (GUT)
- A hypothetical theory that would merge the electroweak force and the strong nuclear force into a single unified force, a step below the full Theory of Everything.
- Planck scale / Planck energy
- The energy scale (~10^19 GeV) at which quantum gravitational effects are expected to become important; roughly 10^15 times beyond the reach of current accelerators.
- Neutrino oscillation
- The phenomenon where a neutrino created as one of three 'flavors' (electron, muon, tau) spontaneously changes into another flavor as it travels; confirmed since 1998 and implies neutrinos have mass.
- Leptogenesis
- A proposed mechanism for the matter-antimatter asymmetry in which differences in the oscillation behavior of neutrinos and antineutrinos in the early universe led to a surplus of matter.
- Cosmological constant (Λ)
- A term Einstein added — then removed — from his general relativity equations to represent a repulsive energy of space; reintroduced in 1998 after observational evidence for accelerating cosmic expansion.
- Baryonic matter
- Ordinary matter made of protons and neutrons (baryons), as opposed to dark matter; constitutes only about 5% of the total energy content of the universe.
- Microlensing
- A gravitational lensing effect where a massive foreground object causes a background star to temporarily brighten; used to search for dark compact objects like rogue black holes.
- Bullet Cluster
- A system of two colliding galaxy clusters where gravitational lensing maps the mass at the location of the galaxies rather than the gas clouds, providing strong evidence for dark matter.
- Loop quantum gravity (LQG)
- A theory that attempts to quantize space itself — treating spacetime as composed of discrete fundamental units — without attempting to unify all forces; developed by Carlo Rovelli and colleagues.
- Prodigious
- Remarkably large or impressive in extent; used by Lincoln to describe the rate of collisions at the LHC (~1 billion per second).
- Supersymmetry (SUSY)
- A theoretical framework postulating that every known particle has a heavier 'superpartner'; predicts five Higgs bosons rather than one, and was a leading dark matter candidate theory that has not been confirmed at the LHC.