W particle, one of two massive electrically charged subatomic particles that are thought to transmit the weak force—that is, the force that governs radioactive decay in certain kinds of atomic nuclei. According to the Standard Model of particle physics that describes the fundamental particles and their interactions, the W particles and their electrically neutral partner, the Z particle, are the carrier particles (the gauge bosons) of the weak force. The discovery of the W and Z particles—also referred to as intermediate vector bosons—confirmed the electroweak theory, the joint framework describing the electromagnetic and weak forces.

The existence of intermediate vector bosons and their properties were predicted in the late 1960s by the physicists Sheldon Lee Glashow, Steven Weinberg, and Abdus Salam. Their theoretical efforts, now called the electroweak theory, explain that the electromagnetic force and the weak force, long considered separate entities, are actually manifestations of the same basic interaction. Just as the electromagnetic force is transmitted by means of carrier particles known as photons, the weak force is exchanged via three types of intermediate vector bosons. Two of these bosons bear either a positive or a negative electric charge and are designated W+ and W, respectively. The third type, called Z0, is electrically neutral. Unlike photons, each intermediate vector boson has a large mass, and this characteristic is responsible for the extremely short range of the weak force, whose influence is confined to a distance of only about 10−17 metre. (As established by quantum mechanics, the range of any given force tends to be inversely proportional to the mass of the particle transmitting it.)

In low-energy processes such as radioactive beta decay, the heavy W particles can be exchanged only because the uncertainty principle in quantum mechanics allows fluctuations in mass-energy over sufficiently short timescales. Such W particles can never be observed directly. However, detectable W particles can be produced in particle-accelerator experiments involving collisions between subatomic particles, provided that the collision energy is high enough. A W particle of this kind then decays into a charged lepton (e.g., electron, muon, or tau) and an associated neutrino or into a quark and an antiquark of different type (or “flavour”) but with a total charge of +1 or −1.

In 1983 two experiments at the European Organization for Nuclear Research (CERN) detected characteristics closely approximating those predicted for the formation and decay of W and Z particles. Their findings constituted the first direct evidence of weak bosons and provided strong support for the electroweak theory. The two teams observed numerous clear-cut instances of weak bosons in proton-antiproton collision experiments that were carried out in a 540-gigaelectron-volt (GeV; 109 eV) colliding-beam storage ring. All of the observed W particles had a mass of about 81 GeV, or approximately 80 times the mass of the proton, as had been predicted by the electroweak theory. The electrically neutral Z particles detected, with a rest mass of 93 GeV, were also consistent with prediction. The CERN physicist Carlo Rubbia and engineer Simon van der Meer were awarded the 1984 Nobel Prize for Physics in recognition of their role in the discovery of the W and Z particles.

Since the early work at CERN, W particles have been generated in much greater numbers in the 1,800-GeV Tevatron proton-antiproton collider at the Fermi National Accelerator Laboratory and in the Large Electron-Positron collider at CERN. These experiments have yielded more-precise measurements of the mass of the W particle, now known to be close to 80.4 GeV.

This article was most recently revised and updated by Robert Curley.

weak interaction, a fundamental force of nature that underlies some forms of radioactivity, governs the decay of unstable subatomic particles such as mesons, and initiates the nuclear fusion reaction that fuels the Sun. The weak interaction acts upon left-handed fermions—i.e., elementary particles with half-integer values of intrinsic angular momentum, or spin—and right-handed antifermions. Particles interact through the weak interaction by exchanging force-carrier particles known as the W and Z particles. These particles are heavy, with masses about 100 times the mass of a proton, and it is their heaviness that defines the extremely short-range nature of the weak interaction and that makes the weak interaction appear weak at the low energies associated with radioactivity.

The effectiveness of the weak interaction is confined to a distance range of 10−17 metre, about 1 percent of the diameter of a typical atomic nucleus. In radioactive decays the strength of the weak interaction is about 100,000 times less than the strength of the electromagnetic force. However, it is now known that the weak interaction has intrinsically the same strength as the electromagnetic force, and these two apparently distinct forces are believed to be different manifestations of a unified electroweak force.

Most subatomic particles are unstable and decay by the weak interaction, even if they cannot decay by the electromagnetic force or the strong force. The lifetimes for particles that decay via the weak interaction vary from as little as 10−13 second to 896 seconds, the mean life of the free neutron. Neutrons bound in atomic nuclei can be stable, as they are when they occur in the familiar chemical elements, but they can also give rise through weak decays to the type of radioactivity known as beta decay. In this case the lifetimes of the nuclei can vary from a thousandth of a second to millions of years. Although low-energy weak interactions are feeble, they occur frequently at the heart of the Sun and other stars where both the temperature and the density of matter are high. In the nuclear fusion process that is the source of stellar energy production, two protons interact via the weak interaction to form a deuterium nucleus, which reacts further to generate helium with the concomitant release of large amounts of energy.

Italian-born physicist Dr. Enrico Fermi draws a diagram at a blackboard with mathematical equations. circa 1950.
Britannica Quiz
Physics and Natural Law

The characteristics of the weak interaction, including its relative strength and effective range and the nature of the force-carrier particles, are summarized in the Standard Model of particle physics.

Christine Sutton