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Parity (physics)

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Symmetry of spatially mirrored systems

Inphysics, aparity transformation (also calledparity inversion) is the flip in the sign ofonespatialcoordinate. In three dimensions, it can also refer to the simultaneous flip in the sign of all three spatial coordinates (apoint reflection):

P:(xyz)(xyz).{\displaystyle \mathbf {P} :{\begin{pmatrix}x\\y\\z\end{pmatrix}}\mapsto {\begin{pmatrix}-x\\-y\\-z\end{pmatrix}}.}

It can also be thought of as a test forchirality of a physical phenomenon, in that a parity inversion transforms a phenomenon into its mirror image.

All fundamental interactions ofelementary particles, with the exception of theweak interaction, are symmetric under parity transformation. As established by theWu experiment conducted at the USNational Bureau of Standards by Chinese-American scientistChien-Shiung Wu, the weak interaction is chiral and thus provides a means for probing chirality in physics. In her experiment, Wu took advantage of the controlling role of weak interactions inradioactive decay of atomic isotopes to establish the chirality of the weak force.

By contrast, in interactions that are symmetric under parity, such as electromagnetism in atomic and molecular physics, parity serves as a powerful controlling principle underlying quantum transitions.

A matrix representation ofP (in any number of dimensions) hasdeterminant equal to −1, and hence is distinct from arotation, which has a determinant equal to 1. In a two-dimensional plane, a simultaneous flip of all coordinates in sign isnot a parity transformation; it is the same as a180° rotation.

In quantum mechanics, wave functions that are unchanged by a parity transformation are described aseven functions, while those that change sign under a parity transformation are odd functions.

Simple symmetry relations

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See also:Representation theory of SU(2)

Underrotations, classical geometrical objects can be classified intoscalars,vectors, andtensors of higher rank. Inclassical physics, physical configurations need to transform underrepresentations of every symmetry group.

Quantum theory predicts that states in aHilbert space do not need to transform under representations of thegroup of rotations, but only underprojective representations. The wordprojective refers to the fact that if one projects out the phase of each state, where we recall that the overall phase of a quantum state is not observable, then a projective representation reduces to an ordinary representation. All representations are also projective representations, but the converse is not true, therefore the projective representation condition on quantum states is weaker than the representation condition on classical states.

The projective representations of any group are isomorphic to the ordinary representations of acentral extension of the group. For example, projective representations of the 3-dimensional rotation group, which is thespecial orthogonal group SO(3), are ordinary representations of thespecial unitary group SU(2). Projective representations of the rotation group that are not representations are calledspinors and so quantum states may transform not only as tensors but also as spinors.

If one adds to this a classification by parity, these can be extended, for example, into notions of

  • scalars (P = +1) andpseudoscalars (P = −1) which are rotationally invariant.
  • vectors (P = −1) andaxial vectors (also calledpseudovectors) (P = +1) which both transform as vectors under rotation.

One can definereflections such as

Vx:(xyz)(xyz),{\displaystyle V_{x}:{\begin{pmatrix}x\\y\\z\end{pmatrix}}\mapsto {\begin{pmatrix}-x\\y\\z\end{pmatrix}},}

which also have negative determinant and form a valid parity transformation. Then, combining them with rotations (or successively performingx-,y-, andz-reflections) one can recover the particular parity transformation defined earlier. The first parity transformation given does not work in an even number of dimensions, though, because it results in a positive determinant. In even dimensions only the latter example of a parity transformation (or any reflection of an odd number of coordinates) can be used.

Parity forms theabelian groupZ2{\displaystyle \mathbb {Z} _{2}} due to the relationP^2=1^{\displaystyle {\hat {\mathcal {P}}}^{2}={\hat {1}}}. All Abelian groups have only one-dimensionalirreducible representations. ForZ2{\displaystyle \mathbb {Z} _{2}}, there are two irreducible representations: one is even under parity,P^ϕ=+ϕ{\displaystyle {\hat {\mathcal {P}}}\phi =+\phi }, the other is odd,P^ϕ=ϕ{\displaystyle {\hat {\mathcal {P}}}\phi =-\phi }. These are useful in quantum mechanics. However, as is elaborated below, in quantum mechanics states need not transform under actual representations of parity but only under projective representations and so in principle a parity transformation may rotate a state by anyphase.

Representations of O(3)

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An alternative way to write the above classification of scalars, pseudoscalars, vectors and pseudovectors is in terms of the representation space that each object transforms in. This can be given in terms of thegroup homomorphismρ{\displaystyle \rho } which defines the representation. For a matrixRO(3),{\displaystyle R\in {\text{O}}(3),}

When the representation is restricted toSO(3){\displaystyle {\text{SO}}(3)}, scalars and pseudoscalars transform identically, as do vectors and pseudovectors.

Classical mechanics

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Newton's equation of motionF=ma{\displaystyle \mathbf {F} =m\mathbf {a} } (if the mass is constant) equates two vectors, and hence is invariant under parity. The law of gravity also involves only vectors and is also, therefore, invariant under parity.

However, angular momentumL{\displaystyle \mathbf {L} } is anaxial vector,L=r×pP^(L)=(r)×(p)=L.{\displaystyle {\begin{aligned}\mathbf {L} &=\mathbf {r} \times \mathbf {p} \\{\hat {P}}\left(\mathbf {L} \right)&=(-\mathbf {r} )\times (-\mathbf {p} )=\mathbf {L} .\end{aligned}}}

In classicalelectrodynamics, the charge densityρ{\displaystyle \rho } is a scalar, the electric field,E{\displaystyle \mathbf {E} }, and currentj{\displaystyle \mathbf {j} } are vectors, but the magnetic field,B{\displaystyle \mathbf {B} } is an axial vector. However,Maxwell's equations are invariant under parity because thecurl of an axial vector is a vector.

Effect of spatial inversion on some variables of classical physics

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The two major divisions of classical physical variables have either even or odd parity. The way into which particular variables and vectors sort out into either category depends on whether thenumber of dimensions of space is either an odd or even number. The categories ofodd oreven given below for theparity transformation is a different, but intimately related issue.

The answers given below are correct for 3 spatial dimensions. In a 2 dimensional space, for example, when constrained to remain on the surface of a planet, some of the variables switch sides.

Odd

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Classical variables whose signs flip under space inversion are predominantly vectors. They include:

Even

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Classical variables, predominantly scalar quantities, which do not change upon spatial inversion include:

Quantum mechanics

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Possible eigenvalues

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Two dimensional representations of parity are given by a pair of quantum states which go into each other under parity. However, this representation can always be reduced to linear combinations of states, each of which is either even or odd under parity. One says that allirreducible representations of parity are one-dimensional.

In quantum mechanics, spacetime transformations act onquantum states. The parity transformation,P^{\displaystyle {\hat {\mathcal {P}}}}, is aunitary operator, in general acting on a stateψ{\displaystyle \psi } as follows:P^ψ(r)=eiϕ/2ψ(r){\displaystyle {\hat {\mathcal {P}}}\,\psi {\left(r\right)}=e^{{i\phi }/{2}}\psi {\left(-r\right)}}.

One must then haveP^2ψ(r)=eiϕψ(r){\displaystyle {\hat {\mathcal {P}}}^{2}\,\psi {\left(r\right)}=e^{i\phi }\psi {\left(r\right)}}, since an overall phase is unobservable. The operatorP^2{\displaystyle {\hat {\mathcal {P}}}^{2}}, which reverses the parity of a state twice, leaves the spacetime invariant, and so is an internal symmetry which rotates its eigenstates by phaseseiϕ{\displaystyle e^{i\phi }}. IfP^2{\displaystyle {\hat {\mathcal {P}}}^{2}} is an elementeiQ{\displaystyle e^{iQ}} of a continuous U(1) symmetry group of phase rotations, theneiQ{\displaystyle e^{-iQ}} is part of this U(1) and so is also a symmetry. In particular, we can defineP^P^eiQ/2{\displaystyle {\hat {\mathcal {P}}}'\equiv {\hat {\mathcal {P}}}\,e^{-{iQ}/{2}}}, which is also a symmetry, and so we can choose to callP^{\displaystyle {\hat {\mathcal {P}}}'} our parity operator, instead ofP^{\displaystyle {\hat {\mathcal {P}}}}. Note thatP^2=1{\displaystyle {{\hat {\mathcal {P}}}'}^{2}=1} and soP^{\displaystyle {\hat {\mathcal {P}}}'} has eigenvalues±1{\displaystyle \pm 1}. Wave functions with eigenvalue+1{\displaystyle +1} under a parity transformation areeven functions, while eigenvalue1{\displaystyle -1} corresponds to odd functions.[1] However, when no such symmetry group exists, it may be that all parity transformations have some eigenvalues which are phases other than±1{\displaystyle \pm 1}.

For electronic wavefunctions, even states are usually indicated by a subscript g forgerade (German: even) and odd states by a subscript u forungerade (German: odd). For example, the lowest energy level of the hydrogen molecule ion (H2+) is labelled1σg{\displaystyle 1\sigma _{g}} and the next-closest (higher) energy level is labelled1σu{\displaystyle 1\sigma _{u}}.[2]

The wave functions of a particle moving into an external potential, which iscentrosymmetric (potential energy invariant with respect to a space inversion, symmetric to the origin), either remain invariable or change signs: these two possible states are called the even state or odd state of the wave functions.[3]

The law of conservation of parity of particles states that, if an isolated ensemble of particles has a definite parity, then the parity remains invariable in the process of ensemble evolution. However this is not true for thebeta decay of nuclei, because theweak nuclear interaction violates parity.[4]

The parity of the states of a particle moving in a spherically symmetric external field is determined by theangular momentum, and the particle state is defined by three quantum numbers: total energy, angular momentum and the projection of angular momentum.[3]

Consequences of parity symmetry

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When parity generates theAbelian groupZ2{\displaystyle \mathbb {Z} _{2}}, one can always take linear combinations of quantum states such that they are either even or odd under parity (see the figure). Thus the parity of such states is ±1. The parity of a multiparticle state is the product of the parities of each state; in other words parity is a multiplicative quantum number.

In quantum mechanics,Hamiltonians areinvariant (symmetric) under a parity transformation ifP^{\displaystyle {\hat {\mathcal {P}}}}commutes with the Hamiltonian. In non-relativistic quantum mechanics, this happens for any scalar potential, i.e.,V=V(r){\displaystyle V=V{\left(r\right)}}, hence the potential is spherically symmetric. The following facts can be easily proven:

Some of the non-degenerate eigenfunctions ofH^{\displaystyle {\hat {H}}} are unaffected (invariant) by parityP^{\displaystyle {\hat {\mathcal {P}}}} and the others are merely reversed in sign when the Hamiltonian operator and the parity operator commute:P^|ψ=c|ψ,{\displaystyle {\hat {\mathcal {P}}}|\psi \rangle =c\left|\psi \right\rangle ,}

wherec{\displaystyle c} is a constant, theeigenvalue ofP^{\displaystyle {\hat {\mathcal {P}}}},P^2|ψ=cP^|ψ.{\displaystyle {\hat {\mathcal {P}}}^{2}\left|\psi \right\rangle =c\,{\hat {\mathcal {P}}}\left|\psi \right\rangle .}

Many-particle systems: atoms, molecules, nuclei

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The overall parity of a many-particle system is the product of the parities of the one-particle states. It is −1 if an odd number of particles are in odd-parity states, and +1 otherwise. Different notations are in use to denote the parity of nuclei, atoms, and molecules.

Atoms

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Atomic orbitals have parity (−1), where the exponent ℓ is theazimuthal quantum number. The parity is odd for orbitals p, f, ... with ℓ = 1, 3, ..., and an atomic state has odd parity if an odd number of electrons occupy these orbitals. For example, the ground state of the nitrogen atom has the electron configuration 1s22s22p3, and is identified by the term symbol4So, where the superscript o denotes odd parity. However the third excited term at about 83,300 cm−1 above the ground state has electron configuration 1s22s22p23s has even parity since there are only two 2p electrons, and its term symbol is4P (without an o superscript).[6]

Molecules

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The complete (rotational-vibrational-electronic-nuclear spin) electromagnetic Hamiltonian of any molecule commutes with (or is invariant to) the parity operation P (or E*, in the notation introduced byLonguet-Higgins[7]) and its eigenvalues can be given the parity symmetry label+ or as they are even or odd, respectively. The parity operation involves the inversion of electronic and nuclear spatial coordinates at the molecular center of mass.

Centrosymmetric molecules at equilibrium have a centre of symmetry at their midpoint (the nuclear center of mass). This includes all homonucleardiatomic molecules as well as certain symmetric molecules such asethylene,benzene,xenon tetrafluoride andsulphur hexafluoride. For centrosymmetric molecules, the point group contains the operationi which is not to be confused with the parity operation. The operationi involves the inversion of the electronic and vibrational displacement coordinates at the nuclear centre of mass. For centrosymmetric molecules the operationi commutes with the rovibronic (rotation-vibration-electronic) Hamiltonian and can be used to label such states. Electronic and vibrational states of centrosymmetric molecules are either unchanged by the operationi, or they are changed in sign byi. The former are denoted by the subscriptg and are calledgerade,while the latter are denoted by the subscriptu and are calledungerade. The complete electromagnetic Hamiltonian of a centrosymmetric moleculedoes not commute with the point group inversion operationi because of the effect of the nuclear hyperfine Hamiltonian. The nuclear hyperfine Hamiltonian can mix the rotational levels ofg andu vibronic states (calledortho-para mixing) and give rise toortho-para transitions[8][9]

Nuclei

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In atomic nuclei, the state of each nucleon (proton or neutron) has even or odd parity, and nucleon configurations can be predicted using thenuclear shell model. As for electrons in atoms, the nucleon state has odd overall parity if and only if the number of nucleons in odd-parity states is odd. The parity is usually written as a + (even) or − (odd) following the nuclear spin value. For example, theisotopes of oxygen include17O(5/2+), meaning that the spin is 5/2 and the parity is even. The shell model explains this because the first 16 nucleons are paired so that each pair has spin zero and even parity, and the last nucleon is in the 1d5/2 shell, which has even parity since ℓ = 2 for a d orbital.[10]

Quantum field theory

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If one can show that thevacuum state is invariant under parity,P^|0=|0{\displaystyle {\hat {\mathcal {P}}}\left|0\right\rangle =\left|0\right\rangle }, the Hamiltonian is parity invariant[H^,P^]{\displaystyle \left[{\hat {H}},{\hat {\mathcal {P}}}\right]} and the quantization conditions remain unchanged under parity, then it follows that every state hasgood parity, and this parity is conserved in any reaction.

To show thatquantum electrodynamics is invariant under parity, we have to prove that the action is invariant and the quantization is also invariant. For simplicity we will assume thatcanonical quantization is used; the vacuum state is then invariant under parity by construction. The invariance of the action follows from the classical invariance of Maxwell's equations. The invariance of the canonical quantization procedure can be worked out, and turns out to depend on the transformation of the annihilation operator:[citation needed]Pa(p,±)P+=a(p,±){\displaystyle \mathbf {Pa} (\mathbf {p} ,\pm )\mathbf {P} ^{+}=\mathbf {a} (-\mathbf {p} ,\pm )}wherep{\displaystyle \mathbf {p} } denotes the momentum of a photon and±{\displaystyle \pm } refers to its polarization state. This is equivalent to the statement that the photon has oddintrinsic parity. Similarly allvector bosons can be shown to have odd intrinsic parity, and allaxial-vectors to have even intrinsic parity.

A straightforward extension of these arguments to scalar field theories shows that scalars have even parity. That is,Pϕ(x,t)P1=ϕ(x,t){\displaystyle {\mathsf {P}}\phi (-\mathbf {x} ,t){\mathsf {P}}^{-1}=\phi (\mathbf {x} ,t)}, sincePa(p)P+=a(p){\displaystyle \mathbf {Pa} (\mathbf {p} )\mathbf {P} ^{+}=\mathbf {a} (-\mathbf {p} )}This is true even for a complex scalar field. (Details ofspinors are dealt with in the article on theDirac equation, where it is shown thatfermions and antifermions have opposite intrinsic parity.)

Withfermions, there is a slight complication because there is more than onespin group.

Parity in the Standard Model

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Fixing the global symmetries

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See also:(−1)F

Applying the parity operator twice leaves the coordinates unchanged, meaning thatP2 must act as one of the internal symmetries of the theory, at most changing the phase of a state.[11] For example, theStandard Model has three globalU(1) symmetries with charges equal to thebaryon numberB, thelepton numberL, and theelectric chargeQ. Therefore, the parity operator satisfiesP2 =eiαB+iβL+iγQ for some choice ofα,β, andγ. This operator is also not unique in that a new parity operatorP' can always be constructed by multiplying it by an internal symmetry such asP' =PeiαB for someα.

To see if the parity operator can always be defined to satisfyP2 = 1, consider the general case whenP2 =Q for some internal symmetry Q present in the theory. The desired parity operator would beP' =PQ−1/2. IfQ is part of a continuous symmetry group thenQ−1/2 exists, but if it is part of adiscrete symmetry then this element need not exist and such a redefinition may not be possible.[12]

The Standard Model exhibits a(−1)F symmetry, whereF is thefermionnumber operator counting how many fermions are in a state. Since all particles in the Standard Model satisfyF =B +L, the discrete symmetry is also part of thee(B +L) continuous symmetry group. If the parity operator satisfiedP2 = (−1)F, then it can be redefined to give a new parity operator satisfyingP2 = 1. But if the Standard Model is extended by incorporatingMajorananeutrinos, which haveF = 1 andB +L = 0, then the discrete symmetry(−1)F is no longer part of the continuous symmetry group and the desired redefinition of the parity operator cannot be performed. Instead it satisfiesP4 = 1 so the Majorana neutrinos would have intrinsic parities of±i.

Parity of the pion

[edit]

In 1954, a paper byWilliam Chinowsky andJack Steinberger demonstrated that thepion has negative parity.[13]They studied the decay of an "atom" made from adeuteron (2
1
H+
) and a negatively charged pion (π
) in a state with zero orbitalangular momentum L=0 {\displaystyle ~\mathbf {L} ={\boldsymbol {0}}~} into twoneutrons (n{\displaystyle n}).

Neutrons arefermions and so obeyFermi–Dirac statistics, which implies that the final state is antisymmetric. Using the fact that the deuteron has spin one and the pion spin zero together with the antisymmetry of the final state they concluded that the two neutrons must have orbital angular momentum L=1 .{\displaystyle ~L=1~.} The total parity is the product of the intrinsic parities of the particles and the extrinsic parity of the spherical harmonic function (1)L .{\displaystyle ~\left(-1\right)^{L}~.} Since the orbital momentum changes from zero to one in this process, if the process is to conserve the total parity then the products of the intrinsic parities of the initial and final particles must have opposite sign. A deuteron nucleus is made from a proton and a neutron, and so using the aforementioned convention that protons and neutrons have intrinsic parities equal to +1 {\displaystyle ~+1~} they argued that the parity of the pion is equal to minus the product of the parities of the two neutrons divided by that of the proton and neutron in the deuteron, explicitly(1)(1)2(1)2=1 ,{\textstyle {\frac {(-1)(1)^{2}}{(1)^{2}}}=-1~,} from which they concluded that the pion is apseudoscalar particle.

Parity violation

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See also:Wu experiment
P-symmetry: A clock built like its mirrored image behaves like the mirrored image of the original clock.
P-asymmetry: A clock built like its mirrored image that doesnot behave like a mirrored image of the original clock.

Although parity is conserved inelectromagnetism andgravity, it is violated in weak interactions, and perhaps, to some degree, instrong interactions.[14][15] The Standard Model incorporatesparity violation by expressing the weak interaction as achiral gauge interaction. Only the left-handed components of particles and right-handed components of antiparticles participate in charged weak interactions in the Standard Model. This implies that parity is not a symmetry of our universe, unless ahidden mirror sector exists in which parity is violated in the opposite way.

An obscure 1928 experiment, undertaken byR. T. Cox, G. C. McIlwraith, and B. Kurrelmeyer, had in effect reported parity violation inweak decays, but, since the appropriate concepts had not yet been developed, those results had no impact.[16] In 1929,Hermann Weyl explored, without any evidence, the existence of a two-component massless particle of spin one-half. This idea was rejected byPauli, because it implied parity violation.[17]

By the mid-20th century, it had been suggested by several scientists that parity might not be conserved (in different contexts), but without solid evidence these suggestions were not considered important. Then, in 1956, a careful review and analysis by theoretical physicistsTsung-Dao Lee andChen-Ning Yang[18] went further, showing that while parity conservation had been verified in decays by the strong orelectromagnetic interactions, it was untested in theweak interaction. They proposed several possible direct experimental tests. They were mostly ignored,[citation needed] but Lee was able to convince his Columbia colleagueChien-Shiung Wu to try it.[citation needed] She needed specialcryogenic facilities and expertise, so the experiment was done at theNational Bureau of Standards.

Wu,Ambler, Hayward, Hoppes, and Hudson (1957) found a clear violation of parity conservation in the beta decay ofcobalt-60.[19] As the experiment was winding down, with double-checking in progress, Wu informed Lee and Yang of their positive results, and saying the results need further examination, she asked them not to publicize the results first. However, Lee revealed the results to his Columbia colleagues on 4 January 1957 at a "Friday lunch" gathering of the Physics Department of Columbia.[20] Three of them,R. L. Garwin,L. M. Lederman, and R. M. Weinrich, modified an existing cyclotron experiment, and immediately verified the parity violation.[21] They delayed publication of their results until after Wu's group was ready, and the two papers appeared back-to-back in the same physics journal.

The discovery of parity violation explained the outstandingτ–θ puzzle in the physics ofkaons.

In 2010, it was reported that physicists working with theRelativistic Heavy Ion Collider had created a short-lived parity symmetry-breaking bubble inquark–gluon plasmas. An experiment conducted by several physicists in theSTAR collaboration, suggested that parity may also be violated in the strong interaction.[15] It is predicted that this local parity violation manifests itself bychiral magnetic effect.[22][23]

Intrinsic parity of hadrons

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To every particle one can assign an intrinsic parity as long as nature preserves parity. Although weak interactions do not, one can still assign a parity to anyhadron by examining the strong interaction reaction that produces it, or through decays not involving the weak interaction, such asrho meson decay topions.

See also

[edit]

References

[edit]

Footnotes

  1. ^An example of a mass flow rate would the direction and rate, by weight, at which a river moves sediment. It is a composite form oflinear momentum, and is closely related to the flow ofsound oscillations through a medium.

Citations

  1. ^Levine, Ira N. (1991).Quantum Chemistry (4th ed.). Prentice-Hall. p. 163.ISBN 0-205-12770-3.
  2. ^Levine, Ira N. (1991).Quantum Chemistry (4th ed.). Prentice-Hall. p. 355.ISBN 0-205-12770-3.
  3. ^abAndrew, A. V. (2006). "2.Schrödinger equation".Atomic spectroscopy. Introduction of theory to Hyperfine Structure. Springer. p. 274.ISBN 978-0-387-25573-6.
  4. ^Mladen Georgiev (20 November 2008). "Parity non-conservation in β-decay of nuclei: revisiting experiment and theory fifty years after. IV. Parity breaking models". p. 26.arXiv:0811.3403 [physics.hist-ph].
  5. ^Bransden, B. H.; Joachain, C. J. (2003).Physics of Atoms and Molecules (2nd ed.).Prentice Hall. p. 204.ISBN 978-0-582-35692-4.
  6. ^NIST Atomic Spectrum Database To read the nitrogen atom energy levels, type "N I" in the Spectrum box and click on Retrieve data.
  7. ^Longuet-Higgins, H.C. (1963)."The symmetry groups of non-rigid molecules".Molecular Physics.6 (5):445–460.Bibcode:1963MolPh...6..445L.doi:10.1080/00268976300100501.
  8. ^Pique, J. P.; et al. (1984). "Hyperfine-Induced Ungerade-Gerade Symmetry Breaking in a Homonuclear Diatomic Molecule near a Dissociation Limit:127{\displaystyle ^{127}}I2{\displaystyle _{2}} at the2P3/2{\displaystyle ^{2}P_{3/2}}2P1/2{\displaystyle ^{2}P_{1/2}} Limit".Phys. Rev. Lett.52 (4):267–269.Bibcode:1984PhRvL..52..267P.doi:10.1103/PhysRevLett.52.267.
  9. ^Critchley, A. D. J.; et al. (2001). "Direct Measurement of a Pure Rotation Transition in H2+{\displaystyle _{2}^{+}}".Phys. Rev. Lett.86 (9):1725–1728.Bibcode:2001PhRvL..86.1725C.doi:10.1103/PhysRevLett.86.1725.PMID 11290233.
  10. ^Cottingham, W.N.; Greenwood, D.A. (1986).An introduction to nuclear physics. Cambridge University Press. p. 57.ISBN 0-521-31960-9.
  11. ^Weinberg, Steven (1995). "16".The Quantum Theory of Fields Volume 1. Vol. 4. Cambridge University Press. pp. 124–126.ISBN 9780521670531.
  12. ^Feinberg, G.;Weinberg, S. (1959). "On the phase factors in inversions".Il Nuovo Cimento.14 (3):571–592.Bibcode:1959NCim...14..571F.doi:10.1007/BF02726388.S2CID 120498009.
  13. ^Chinowsky, W.; Steinberger, J. (1954). "Absorption of Negative Pions in Deuterium: Parity of the Pion".Physical Review.95 (6):1561–1564.Bibcode:1954PhRv...95.1561C.doi:10.1103/PhysRev.95.1561.
  14. ^Gardner, Martin (1969) [1964].The Ambidextrous Universe; Left, Right, and the Fall of Parity (rev. ed.). New York:New American Library. p. 213.
  15. ^abMuzzin, S.T. (19 March 2010)."For one tiny instant, physicists may have broken a law of nature".PhysOrg. Retrieved5 August 2011.
  16. ^Roy, A. (2005). "Discovery of parity violation".Resonance.10 (12):164–175.doi:10.1007/BF02835140.S2CID 124880732.
  17. ^Wu, Chien-Shiung (2008),"The Discovery of the Parity Violation in Weak Interactions and Its Recent Developments",Nishina Memorial Lectures, Lecture Notes in Physics, vol. 746, Tokyo: Springer Japan, pp. 43–70,doi:10.1007/978-4-431-77056-5_4,ISBN 978-4-431-77055-8, retrieved29 August 2021
  18. ^Lee, T.D.;Yang, C.N. (1956)."Question of Parity Conservation in Weak Interactions".Physical Review.104 (1):254–258.Bibcode:1956PhRv..104..254L.doi:10.1103/PhysRev.104.254.
  19. ^Wu, C.S.;Ambler, E; Hayward, R.W.; Hoppes, D.D.; Hudson, R.P. (1957)."Experimental test of parity conservation in beta decay".Physical Review.105 (4):1413–1415.Bibcode:1957PhRv..105.1413W.doi:10.1103/PhysRev.105.1413.
  20. ^Caijian, Jiang (1 August 1996).Wu jian xiong-wu li ke xue de si yi fu ren吳健雄: 物理科學的第一夫人 [Wu Jianxiong: The first lady of physical sciences] (in Chinese). 江才健 (author/biographer). 時報文化出版企業股份有限公司 (Times Culture Publishing Enterprise). p. 216.ISBN 978-957132110-3.{{cite book}}: CS1 maint: ignored ISBN errors (link)ISBN 957-13-2110-9
  21. ^Garwin, R.L.;Lederman, L.M.; Weinrich, R.M. (1957)."Observations of the failure of conservation of parity and charge conjugation in meson decays: The magnetic moment of the free muon".Physical Review.105 (4):1415–1417.Bibcode:1957PhRv..105.1415G.doi:10.1103/PhysRev.105.1415.
  22. ^Kharzeev, D.E.; Liao, J. (2 January 2019). "Isobar collisions at RHIC to test local parity violation in strong interactions".Nuclear Physics News.29 (1):26–31.Bibcode:2019NPNew..29...26K.doi:10.1080/10619127.2018.1495479.ISSN 1061-9127.S2CID 133308325.
  23. ^Zhao, Jie; Wang, Fuqiang (July 2019). "Experimental searches for the chiral magnetic effect in heavy-ion collisions".Progress in Particle and Nuclear Physics.107:200–236.arXiv:1906.11413.Bibcode:2019PrPNP.107..200Z.doi:10.1016/j.ppnp.2019.05.001.S2CID 181517015.

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