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In and , the weak interaction, weak force or the weak nuclear force, is one of the four known fundamental interactions, with the others being , the strong interaction, and . It is the mechanism of interaction between subatomic particles that is responsible for the radioactive decay of atoms: The weak interaction participates in and . The theory describing its behaviour and effects is sometimes called quantum flavordynamics ( QFD); however, the term QFD is rarely used, because the weak force is better understood by electroweak theory (EWT).

(2025). 9783527406012, Wiley.

The effective range of the weak force is limited to subatomic distances and is less than the diameter of a proton.


Background
The of provides a uniform framework for understanding electromagnetic, weak, and strong interactions. An interaction occurs when two particles (typically, but not necessarily, spin ) exchange integer-spin, force-carrying . The fermions involved in such exchanges can be either electric (e.g., or ) or composite (e.g. or ), although at the deepest levels, all weak interactions ultimately are between elementary particles.

In the weak interaction, fermions can exchange three types of force carriers, namely , , and  bosons. The of these bosons are far greater than the mass of a proton or neutron, which is consistent with the short range of the weak force. In fact, the force is termed weak because its over any set distance is typically several orders of magnitude less than that of the electromagnetic force, which itself is further orders of magnitude less than the strong .

The weak interaction is the only fundamental interaction that breaks parity symmetry, and similarly, but far more rarely, the only interaction to break .

, which make up composite particles like neutrons and protons, come in six "flavours" up, down, charm, strange, top and bottom which give those composite particles their properties. The weak interaction is unique in that it allows quarks to swap their flavour for another. The swapping of those properties is mediated by the force carrier bosons. For example, during , a down quark within a neutron is changed into an up quark, thus converting the neutron to a proton and resulting in the emission of an electron and an electron antineutrino.

Weak interaction is important in the fusion of hydrogen into helium in a star. This is because it can convert a proton (hydrogen) into a neutron to form deuterium which is important for the continuation of nuclear fusion to form helium. The accumulation of neutrons facilitates the buildup of heavy nuclei in a star.

Most fermions decay by a weak interaction over time. Such decay makes radiocarbon dating possible, as carbon-14 decays through the weak interaction to nitrogen-14. It can also create radioluminescence, commonly used in tritium luminescence, and in the related field of (but not similar to ).

The electroweak force is believed to have separated into the electromagnetic and weak forces during the of the early universe.


History
In 1933, proposed the first theory of the weak interaction, known as Fermi's interaction. He suggested that could be explained by a four- interaction, involving a contact force with no range.

In the mid-1950s, and first suggested that the handedness of the spins of particles in weak interaction might violate the or symmetry. In 1957, the , carried out by Chien Shiung Wu and collaborators confirmed the symmetry violation.

In the 1960s, , and unified the electromagnetic force and the weak interaction by showing them to be two aspects of a single force, now termed the electroweak force.

The existence of the and  bosons was not directly confirmed until 1983.

(2025). 9780521657334, Cambridge University Press. .


Properties
The electrically charged weak interaction is unique in a number of respects:
  • It is the only interaction that can change the flavour of quarks and leptons (i.e., of changing one type of quark into another).
  • It is the only interaction that violates P, or parity symmetry. It is also the only one that violates .
  • Both the electrically charged and the electrically neutral interactions are mediated (propagated) by that have significant masses, an unusual feature which is explained in the by the .
  • Decay processes like governed by the weak interaction can only be observed when processes involving faster decays via electromagnetic or strong interaction are not competing.
    (1998). 9780471239734, Wiley. .

Due to their large mass (approximately 90 GeV/ c2) these carrier particles, called the and  bosons, are short-lived with a lifetime of under  seconds.

(1986). 9780521318754, Cambridge University Press. .
The weak interaction has a coupling constant (an indicator of how frequently interactions occur) between and , compared to the electromagnetic coupling constant of about and the strong interaction coupling constant of about 1; consequently the weak interaction is "weak" in terms of intensity. The weak interaction has a very short effective range (around to  m (0.01 to 0.1 fm)). At distances around  meters (0.001 fm), the weak interaction has an intensity of a similar magnitude to the electromagnetic force, but this starts to decrease with increasing distance. Scaled up by just one and a half orders of magnitude, at distances of around 3 m, the weak interaction becomes 10,000 times weaker.

The weak interaction affects all the of the , as well as the ; interact only through gravity and the weak interaction. The weak interaction does not produce , nor does it involve something that gravity does on an astronomical scale, the electromagnetic force does at the molecular and atomic levels, and the strong nuclear force does only at the subatomic level, inside of .

(2025). 9783540878421, Springer. .

Its most noticeable effect is due to its first unique feature: The charged weak interaction causes flavour change. For example, a is heavier than a (its partner ) and can decay into a proton by changing the flavour (type) of one of its two down quarks to an up quark. Neither the strong interaction nor permit flavour changing, so this can only proceed by weak decay; without weak decay, quark properties such as strangeness and charm (associated with the strange quark and charm quark, respectively) would also be conserved across all interactions.

All are unstable because of weak decay. In the process known as , a down quark in the can change into an up quark by emitting a  boson, which then decays into an and an electron . Another example is a common variant of radioactive decay wherein a proton and an electron within an atom interact and are changed to a neutron (an up quark is changed to a down quark), and an electron neutrino is emitted.

Due to the large masses of the W bosons, particle transformations or decays (e.g., flavour change) that depend on the weak interaction typically occur much more slowly than transformations or decays that depend only on the strong or electromagnetic forces. For example, a neutral decays electromagnetically, and so has a life of only about  seconds. In contrast, a charged pion can only decay through the weak interaction, and so lives about  seconds, or a hundred million times longer than a neutral pion. A particularly extreme example is the weak-force decay of a free neutron, which takes about 15 minutes.


Weak isospin and weak hypercharge
+ Left-handed fermions in the Standard Model

electron neutrino
tau
All of the above left-handed ( regular) particles have corresponding
right-handed anti-particles with equal and opposite weak isospin.
All right-handed (regular) particles and left-handed antiparticles have weak isospin of 0.

All particles have a property called (symbol ), which serves as an additive quantum number that restricts how the particle can interact with the of the weak force. Weak isospin plays the same role in the weak interaction with as does in , and in the strong interaction; a different number with a similar name, , discussed below, is used for interactions with the . All left-handed have a weak isospin value of either or ; all right-handed fermions have 0 isospin. For example, the up quark has and the down quark has . A quark never decays through the weak interaction into a quark of the same : Quarks with a of only decay into quarks with a of and conversely.

In any given strong, electromagnetic, or weak interaction, weak isospin is conserved: The sum of the weak isospin numbers of the particles entering the interaction equals the sum of the weak isospin numbers of the particles exiting that interaction. For example, a (left-handed) with a weak isospin of +1 normally decays into a (with ) and a (as a right-handed antiparticle, ).

For the development of the electroweak theory, another property, , was invented, defined as

Y_\text{W} = 2\,(Q - T_3),
where is the weak hypercharge of a particle with electrical charge (in elementary charge units) and weak isospin . is the generator of the U(1) component of the electroweak ; whereas some particles have a of zero, all known have a non-zero weak hypercharge.


Interaction types
There are two types of weak interaction (called ). The first type is called the "charged-current interaction" because the weakly interacting fermions form a current with total electric charge that is nonzero. The second type is called the "neutral-current interaction" because the weakly interacting fermions form a current with total electric charge of zero. It is responsible for the (rare) deflection of . The two types of interaction follow different . This naming convention is often misunderstood to label the electric charge of the and bosons, however the naming convention predates the concept of the mediator bosons, and clearly (at least in name) labels the charge of the current (formed from the fermions), not necessarily the bosons.


Charged-current interaction
In one type of charged current interaction, a charged (such as an or a , having a charge of −1) can absorb a (a particle with a charge of +1) and be thereby converted into a corresponding (with a charge of 0), where the type ("flavour") of neutrino (electron , muon , or tau ) is the same as the type of lepton in the interaction, for example:
\mu^- + \mathrm{W}^+ \to \nu_\mu
Similarly, a down-type (, , or , with a charge of ) can be converted into an up-type quark (, , or , with a charge of ), by emitting a  boson or by absorbing a  boson. More precisely, the down-type quark becomes a quantum superposition of up-type quarks: that is to say, it has a possibility of becoming any one of the three up-type quarks, with the probabilities given in the tables. Conversely, an up-type quark can emit a  boson, or absorb a  boson, and thereby be converted into a down-type quark, for example:
\begin{align}
                \mathrm{d} &\to \mathrm{u} + \mathrm{W}^- \\
 \mathrm{d} + \mathrm{W}^+ &\to \mathrm{u} \\
                \mathrm{c} &\to \mathrm{s} + \mathrm{W}^+ \\
 \mathrm{c} + \mathrm{W}^- &\to \mathrm{s}
     
\end{align}

The W boson is unstable so will rapidly decay, with a very short lifetime. For example:

\begin{align}
 \mathrm{W}^- &\to \mathrm{e}^- + \bar\nu_\mathrm{e} ~ \\
 \mathrm{W}^+ &\to \mathrm{e}^+ + \nu_\mathrm{e} ~
     
\end{align}

Decay of a W boson to other products can happen, with varying probabilities.

In the so-called of a neutron (see picture, above), a down quark within the neutron emits a boson and is thereby converted into an up quark, converting the neutron into a proton. Because of the limited energy involved in the process (i.e., the mass difference between the down quark and the up quark), the virtual boson can only carry sufficient energy to produce an electron and an electron-antineutrino – the two lowest-possible masses among its prospective decay products.

At the quark level, the process can be represented as:

\mathrm{d} \to \mathrm{u} + \mathrm{e}^- + \bar\nu_\mathrm{e} ~


Neutral-current interaction
In interactions, a or a (e.g., an or a ) emits or absorbs a neutral . For example:
\mathrm{e}^- \to \mathrm{e}^- + \mathrm{Z}^0

Like the  bosons, the  boson also decays rapidly, for example:

\mathrm{Z}^0 \to \mathrm{b} + \bar \mathrm{b}

Unlike the charged-current interaction, whose selection rules are strictly limited by chirality, electric charge, weak isospin, the neutral-current interaction can cause any two fermions in the standard model to deflect: Either particles or anti-particles, with any electric charge, and both left- and right-chirality, although the strength of the interaction differs.

The quantum number () serves the same role in the neutral current interaction with the that electric charge (, with no subscript) does in the electromagnetic interaction: It quantifies the vector part of the interaction. Its value is given by:

Q_\mathsf{w} = 2 \, T_3 - 4 \, Q \, \sin^2\theta_\mathsf{w} = 2 \, T_3 - Q + (1 - 4 \, \sin^2\theta_\mathsf{w}) \, Q ~.
Since the weak mixing angle , the parenthetic expression , with its value varying slightly with the momentum difference (called " running") between the particles involved. Hence
\ Q_\mathsf{w} \approx 2 \ T_3 - Q = \sgn(Q)\ \big(1 - |Q|\big)\ ,
since by convention , and for all fermions involved in the weak interaction . The weak charge of charged leptons is then close to zero, so these mostly interact with the  boson through the axial coupling.


Electroweak theory
The of particle physics describes the electromagnetic interaction and the weak interaction as two different aspects of a single electroweak interaction. This theory was developed around 1968 by , , and , and they were awarded the 1979 Nobel Prize in Physics for their work. The provides an explanation for the presence of three massive gauge bosons (, , , the three carriers of the weak interaction), and the (, the massless gauge boson that carries the electromagnetic interaction).

According to the electroweak theory, at very high energies, the universe has four components of the whose interactions are carried by four massless scalar forming a complex scalar Higgs field doublet. Likewise, there are four massless electroweak vector bosons, each similar to the . However, at low energies, this gauge symmetry is spontaneously broken down to the symmetry of electromagnetism, since one of the Higgs fields acquires a vacuum expectation value. Naïvely, the symmetry-breaking would be expected to produce three massless , but instead those "extra" three Higgs bosons become incorporated into the three weak bosons, which then acquire mass through the . These three composite bosons are the , , and  bosons actually observed in the weak interaction. The fourth electroweak gauge boson is the photon () of electromagnetism, which does not couple to any of the Higgs fields and so remains massless.

This theory has made a number of predictions, including a prediction of the masses of the and  bosons before their discovery and detection in 1983.

On 4 July 2012, the CMS and the ATLAS experimental teams at the Large Hadron Collider independently announced that they had confirmed the formal discovery of a previously unknown boson of mass between 125 and , whose behaviour so far was "consistent with" a Higgs boson, while adding a cautious note that further data and analysis were needed before positively identifying the new boson as being a Higgs boson of some type. By 14 March 2013, a Higgs boson was tentatively confirmed to exist.

In a speculative case where the scale were lowered, the unbroken interaction would eventually become confining. Alternative models where becomes confining above that scale appear quantitatively similar to the at lower energies, but dramatically different above symmetry breaking.


Violation of symmetry
The were long thought to remain the same under mirror reflection. The results of an experiment viewed via a mirror were expected to be identical to the results of a separately constructed, mirror-reflected copy of the experimental apparatus watched through the mirror. This so-called law of parity conservation was known to be respected by classical , and the strong interaction; it was assumed to be a universal law.
(2025). 9781438108070, Facts on File Inc..
However, in the mid-1950s and suggested that the weak interaction might violate this law. Chien Shiung Wu and collaborators in 1957 discovered that the weak interaction violates parity, earning Yang and Lee the 1957 Nobel Prize in Physics.

Although the weak interaction was once described by Fermi's theory, the discovery of parity violation and theory suggested that a new approach was needed. In 1957, and and, somewhat later, and proposed a V − A (vector minus or left-handed) Lagrangian for weak interactions. In this theory, the weak interaction acts only on left-handed particles (and right-handed antiparticles). Since the mirror reflection of a left-handed particle is right-handed, this explains the maximal violation of parity. The V − A theory was developed before the discovery of the Z boson, so it did not include the right-handed fields that enter in the neutral current interaction.

However, this theory allowed a compound symmetry to be conserved. CP combines parity P (switching left to right) with charge conjugation C (switching particles with antiparticles). Physicists were again surprised when in 1964, and provided clear evidence in decays that CP symmetry could be broken too, winning them the 1980 Nobel Prize in Physics.

In 1973, Makoto Kobayashi and Toshihide Maskawa showed that CP violation in the weak interaction required more than two generations of particles,

effectively predicting the existence of a then unknown third generation. This discovery earned them half of the 2008 Nobel Prize in Physics.

Unlike parity violation, CP violation occurs only in rare circumstances. Despite its limited occurrence under present conditions, it is widely believed to be the reason that there is much more matter than in the universe, and thus forms one of 's three conditions for .

(2025). 9789971505615, World Scientific Publishing Co.. .


See also
  • Weakless universe – the postulate that weak interactions are not anthropically necessary
  • Strong interaction


Footnotes

Sources

Technical


For general readers
  • (2025). 9780132366786, Plume. .
  • (2025). 080187971X, Johns Hopkins University Press. . 080187971X


External links

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