1999 Nobel Prize in Physics
Reason for Award
for elucidating the quantum structure of electroweak interactions in physics (Nucl. Phys. B7 (1968) 637-650, B33 (1971) 173-199, B35 (1971) 167-188, B44 (1972) 189-213, B50 (1972) 318-353)
Laureates
Netherlands
Netherlands
Explanation
Our world has invisible forces like gravity or magnetism. Two of them—the electric force and the weak force—work together inside the tiny realm of atoms. Mr. ’t Hooft and Mr. Veltman proved with mathematics that these two forces come from the same rule book. Thanks to their work, scientists can calculate exactly how particles appear or disappear. This knowledge underpins technologies such as microwave ovens and medical radiation devices that support our daily life.
Related Keywords
electroweak interaction
The unified force comprising electromagnetic and weak interactions. It is mediated by the photon, W boson, and Z boson, and explained through SU(2)L×U(1)Y symmetry plus the Higgs mechanism, which separates massive and massless carriers. In the early universe the two forces were indistinguishable. It is essential for describing beta decay and solar fusion, and accelerator experiments probe symmetry restoration at high energies. Analyses of the cosmic microwave background and neutrino oscillations also rely on electroweak physics.
gauge theory
A theory whose fundamental principle is that physical laws remain unchanged under certain phase rotations or internal space transformations, known as symmetries. Electromagnetism is a U(1) gauge theory, while quantum chromodynamics is an SU(3) gauge theory. Gauge fields naturally emerge as force-carrying particles and determine the strength and structure of interactions. Mathematically they are described by fiber bundles and connections, linking the theory closely to differential geometry. The Nobel-winning work proved that even non-Abelian gauge theories with a mass-generation mechanism stay self-consistent.
renormalization
A procedure in quantum field theory that redefines the infinities appearing in calculations into finite, measurable quantities. It absorbs the difference between bare parameters and observed values, allowing the theory to make predictions. ’t Hooft and Veltman, using dimensional regularization and BRST invariance, showed that renormalization works even in non-Abelian gauge theories. Renormalization-group equations that track scale dependence are applied to critical phenomena and cosmological inflation. Modern high-energy experiments require careful choice of renormalization schemes to achieve NNLO or higher precision.
spontaneous symmetry breaking
A phenomenon in which the underlying physical laws are symmetric but the vacuum state is not. When the Higgs field acquires a non-zero value, gauge bosons gain mass while the symmetry remains hidden. Above a critical temperature the symmetry is restored, so the mechanism influences early-universe evolution after the Big Bang. It is mathematically analogous to the alignment of spins in a ferromagnet. The renormalizability proof of the electroweak theory ensured that quantum theory remains intact even with this mechanism included.
Standard Model
The theoretical framework that describes electromagnetic, weak, and strong forces together. It contains 17 elementary particles, three gauge interactions, and the Higgs mechanism. ’t Hooft and Veltman’s work made its calculations rigorous, accelerating discoveries of the W and Z bosons, gluons, and the Higgs particle. Unexplained phenomena such as gravity, dark matter, and neutrino masses remain future challenges. Precision tests of the Standard Model provide vital guidance on where new physics may emerge.