Helicity (particle physics)

<h2 id="overview">Overview</h2>
The angular momentum J is the sum of an <a href="/facts/Angular_momentum_operator/d55sXn5u">orbital angular momentum</a> L and a <a href="/facts/Spin_(physics)/4Jvp7e8P">spin</a> S. The relationship between orbital angular momentum L, the position operator r and the linear momentum (orbit part) p is

L
        
        =
        
          r
        
        ×
        
          p
        
      
    
    {\displaystyle \mathbf {L} =\mathbf {r} \times \mathbf {p} }

so L's component in the direction of p is zero. Thus, helicity is just the projection of the spin onto the direction of linear momentum. The helicity of a particle is positive (" right-handed") if the direction of its spin is the same as the direction of its motion and negative ("left-handed") if opposite.
Helicity is <a href="/facts/Conservation_law/6g1Ay2FR">conserved</a>.<a class="footnote-ref" id="fnref:1" href="#fn:1">1</a> That is, the helicity commutes with the <a href="/facts/Hamiltonian_(quantum_mechanics)/5XwK2HmD">Hamiltonian</a>, and thus, in the absence of external forces, is time-invariant. It is also rotationally invariant, in that a rotation applied to the system leaves the helicity unchanged. Helicity, however, is not <a href="/facts/Lorentz_invariant/K5AEuGKg">Lorentz invariant</a>; under the action of a <a href="/facts/Lorentz_boost/jotJL06G">Lorentz boost</a>, the helicity may change sign. Consider, for example, a baseball, pitched as a <a href="/facts/Gyroball/nIyXPYXe">gyroball</a>, so that its spin axis is aligned with the direction of the pitch. It will have one helicity with respect to the point of view of the players on the field, but would appear to have a flipped helicity in any frame moving faster than the ball.

<h3>Comparison with chirality</h3>
In this sense, helicity can be contrasted to <a href="/facts/Chirality_(physics)/H8Xbcvzt">chirality</a>, which is Lorentz invariant, but is not a constant of motion for massive particles. For massless particles, the two coincide: The helicity is equal to the chirality, both are Lorentz invariant, and both are constants of motion.
In <a href="/facts/Quantum_mechanics/BRc3Mzgr">quantum mechanics</a>, angular momentum is quantized, and thus helicity is quantized as well. Because the <a href="/facts/Eigenvalues/8TjEoT8u">eigenvalues</a> of spin with respect to an axis have discrete values, the eigenvalues of helicity are also discrete. For a massive particle of spin S, the eigenvalues of helicity are S, S − 1, S − 2, ..., −S.<a class="footnote-ref" id="fnref:2" href="#fn:2">2</a>: 12 
For massless particles, not all of spin eigenvalues correspond to physically meaningful degrees of freedom: For example, the <a href="/facts/Photon/mFNhAEzA">photon</a> is a massless spin 1 particle with helicity eigenvalues −1 and +1, but the eigenvalue 0 is not physically present.<a class="footnote-ref" id="fnref:3" href="#fn:3">3</a>
All known <a href="/facts/Spin-1/2/3I929M4X">spin ⁠1/2⁠ particles</a> have non-zero mass; however, for hypothetical massless spin ⁠1/2⁠ particles (the <a href="/facts/Weyl_spinor/8KhWTFaM">Weyl spinors</a>), helicity is equivalent to the <a href="/facts/Chirality_(physics)/H8Xbcvzt">chirality operator</a> multiplied by ⁠1/2⁠ħ. By contrast, for massive particles, distinct chirality states (e.g., as occur in the <a href="/facts/Weak_interaction/f6upmKMs">weak interaction</a> charges) have both positive and negative helicity components, in ratios proportional to the mass of the particle.
A treatment of the helicity of gravitational waves can be found in Weinberg.<a class="footnote-ref" id="fnref:4" href="#fn:4">4</a>
In summary, they come in only two forms: +2 and −2, while the +1, 0 and −1 helicities are "non-dynamical" (they can be removed by a gauge transformation).

<h2 id="little-group">Little group</h2>
In 3 + 1 dimensions, the <a href="/facts/Little_group/Vh9VtUUw">little group</a> for a <a href="/facts/Massless_particle/65Xng6Vx">massless particle</a> is the <a href="/facts/Double_covering_group/IrRjtTL2">double cover</a> of <a href="/facts/Euclidean_group/VdTSdwzl">SE(2)</a>. This has <a href="/facts/Unitary_representation/W1XRatG8">unitary representations</a> which are invariant under the SE(2) "translations" and transform as eihθ under a SE(2) rotation by θ. This is the helicity h representation. There is also another unitary representation which transforms non-trivially under the SE(2) translations. This is the continuous spin representation.
In d + 1 dimensions, the little group is the double cover of SE(d − 1) (the case where d ≤ 2 is more complicated because of <a href="/facts/Anyon/hfgpCFjf">anyons</a>, etc.). As before, there are unitary representations which don't transform under the SE(d − 1) "translations" (the "standard" representations) and <a href="/facts/Pauli%E2%80%93Lubanski_pseudovector/r8Tnsnbc">"continuous spin" representations</a>.

<h2 id="see-also">See also</h2>
This article is about helicity in physics. For other uses, see <a href="/facts/Helicity_(disambiguation)/0c4s8UKI">Helicity (disambiguation)</a>.
<ul><li><a href="/facts/Chirality_(physics)/H8Xbcvzt">Chirality (physics)</a></li>
<li><a href="/facts/Helicity_basis/cmjB3ssE">Helicity basis</a></li>
<li><a href="/facts/Gyroball/nIyXPYXe">Gyroball</a>, a macroscopic object (specifically a baseball) exhibiting an analogous phenomenon</li>
<li><a href="/facts/Wigner%27s_classification/1c9PCW2r">Wigner's classification</a></li>
<li><a href="/facts/Pauli%E2%80%93Lubanski_pseudovector/r8Tnsnbc">Pauli–Lubanski pseudovector</a></li></ul>

<h2 id="other-sources">Other sources</h2>

<ul><li>Povh, Bogdan; Lavelle, Martin; Rith, Klaus; Scholz, Christoph; Zetsche, Frank (2008). Particles and Nuclei: An introduction to the physical concepts (6th ed.). Berlin, DE: Springer. <a href="/facts/ISBN_(identifier)/15AdSPa9">ISBN</a> 9783540793687.</li>
<li>Schwartz, Matthew D. (2014). "Chirality, helicity, and spin". Quantum Field Theory and the Standard Model. Cambridge, UK: Cambridge University Press. pp. 185–187. <a href="/facts/ISBN_(identifier)/15AdSPa9">ISBN</a> 9781107034730.</li>
<li>Taylor, John (1992). "Gauge theories in particle physics". In Davies, Paul (ed.). The New Physics (1st pbk. ed.). Cambridge, UK: Cambridge University Press. pp. 458–480. <a href="/facts/ISBN_(identifier)/15AdSPa9">ISBN</a> 9780521438315.</li></ul>

<h2 id="references">References</h2>

<ol>
<li id="fn:1">Landau, L.D.; Lifshitz, E.M. (2013). Quantum mechanics. A shorter course of theoretical physics. Vol. 2. Elsevier. pp. 273–274. ISBN 9781483187228. <a href="9781483187228" target="_blank">9781483187228</a> <a href="#fnref:1" class="footnote-back-ref">↩</a></li>
<li id="fn:2">Troshin, S.M.; Tyurin, N.E. (1994). Spin Phenomena in Particle Interactions. Singapore: World Scientific. ISBN 9789810216924. <a href="9789810216924" target="_blank">9789810216924</a> <a href="#fnref:2" class="footnote-back-ref">↩</a></li>
<li id="fn:3">Thomson, Mark (Fall 2011) [Michaelmas Term, 2011]. "Electroweak unification and the W and Z bosons" (PDF). High Energy Physics. Particle Physics / Part III: Particles. Cambridge, UK: Cambridge University. Retrieved 2022-10-15. <a href="https://www.hep.phy.cam.ac.uk/~thomson/partIIIparticles/handouts/Handout_13_2011.pdf" target="_blank">https://www.hep.phy.cam.ac.uk/~thomson/partIIIparticles/handouts/Handout_13_2011.pdf</a> <a href="#fnref:3" class="footnote-back-ref">↩</a></li>
<li id="fn:4">Weinberg, Steven (1972). Gravitation and Cosmology: Principles and application of the General Theory of Relativity. Wiley & Sons. chapter 10. <a href="#fnref:4" class="footnote-back-ref">↩</a></li>
</ol>

Helicity (particle physics) open-in-new

Helicity (particle physics)