In physics, the Majorana equation is a relativistic wave equation. It is named after the Italian physicist Ettore Majorana, who proposed it in 1937 as a means of describing fermions that are their own antiparticle.[1] Particles corresponding to this equation are termed Majorana particles, although that term now has a more expansive meaning, referring to any (possibly non-relativistic) fermionic particle that is its own anti-particle (and is therefore electrically neutral).
There have been proposals that massive neutrinos are described by Majorana particles; there are various extensions to the Standard Model that enable this. The article on Majorana particles presents status for the experimental searches, including details about neutrinos. This article focuses primarily on the mathematical development of the theory, with attention to its discrete and continuous symmetries. The discrete symmetries are charge conjugation, parity transformation and time reversal; the continuous symmetry is Lorentz invariance.
Charge conjugation plays an outsize role, as it is the key symmetry that allows the Majorana particles to be described as electrically neutral. A particularly remarkable aspect is that electrical neutrality allows several global phases to be freely chosen, one each for the left and right chiral fields. This implies that, without explicit constraints on these phases, the Majorana fields are naturally CP violating. Another aspect of electric neutrality is that the left and right chiral fields can be given distinct masses. That is, electric charge is a Lorentz invariant, and also a constant of motion; whereas chirality is a Lorentz invariant, but is not a constant of motion for massive fields. Electrically neutral fields are thus less constrained than charged fields. Under charge conjugation, the two free global phases appear in the mass terms (as they are Lorentz invariant), and so the Majorana mass is described by a complex matrix, rather than a single number. In short, the discrete symmetries of the Majorana equation are considerably more complicated than those for the Dirac equation, where the electrical charge
U(1)
The Majorana equation can be written in several distinct forms:
These three forms are equivalent, and can be derived from one-another. Each offers slightly different insight into the nature of the equation. The first form emphasises that purely real solutions can be found. The second form clarifies the role of charge conjugation. The third form provides the most direct contact with the representation theory of the Lorentz group.
The conventional starting point is to state that "the Dirac equation can be written in Hermitian form", when the gamma matrices are taken in the Majorana representation. The Dirac equation is then written as[6]
\left(-i
\partial | |
\partialt |
-i\hat\alpha ⋅ \nabla+\betam\right)\psi=0
\hat\alpha
\beta
The Majorana equation is
i{\partial /}\psi-m\psic=0~
{\partial /}
\psic=ηcC{\overline\psi}T~
( ⋅ )T
ηc
|ηc|=1,
ηc=1,
C
C
\overline\psi=\psi\dagger\gamma0~.
A number of algebraic identities follow from the charge conjugation matrix
C.
C\gamma\mu=
TC | |
-\gamma | |
\mu |
\psic=-ηc\gamma0C\psi*~
\psi*
\psi.
C
C-1=C\dagger=CT=-C
i{\partial /}\psic-m\psi=0
A detailed discussion of the physical interpretation of matrix
C
\psic
\psi,
The Majorana operator,
DL,
DL\equivi
\mu\partial | |
\overline{\sigma} | |
\mu |
+ηm\omegaK
\overline{\sigma}\mu=\begin{bmatrix}\sigma0&-\sigma1&-\sigma2&-\sigma3\end{bmatrix}=\begin{bmatrix}I2&-\sigmax&-\sigmay&-\sigmaz\end{bmatrix}
I2
\mu=0
\mu\in\{1,2,3\}.
η
|η|=1,
η=1.
\omega
\operatorname{Sp}(2,C),
\omega=i\sigma2=\begin{bmatrix}0&1\ -1&0\end{bmatrix}~,
\omega2=-I
aI+b\omega\conga+bi\inC
a,b\inR
Finally, the
K
\psiL
DL\psiL=0
i\overline{\sigma}\mu\partial\mu\psiL(x)+ηm\omega
* | |
\psi | |
L(x) |
=0
with
* | |
\psi | |
L(x) |
\psiL(x).
Some of the properties of the Majorana equation, its solution and its Lagrangian formulation are summarized here.
\psi=\psic.
The Majorana equation can be written both in terms of a real four-component spinor, and as a complex two-component spinor. Both can be constructed from the Weyl equation, with the addition of a properly Lorentz-covariant mass term.[7] This section provides an explicit construction and articulation.
The Weyl equation describes the time evolution of a massless complex-valued two-component spinor. It is conventionally written as[8] [9] [10]
\mu\partial | |
\sigma | |
\mu |
\psi=0
Written out explicitly, it is
I2
\partial\psi | |
\partialt |
+
\sigma | ||||
|
+
\sigma | ||||
|
+
\sigma | ||||
|
=0
The Pauli four-vector is
\sigma\mu=\begin{pmatrix}\sigma0&\sigma1&\sigma2&\sigma3\end{pmatrix}=\begin{pmatrix}I2&\sigmax&\sigmay&\sigmaz\end{pmatrix}
I2
\vecx\to{\vecx}\prime=-\vecx
\mu\partial | |
\bar{\sigma} | |
\mu |
\psi=0
where
\bar{\sigma}\mu=\begin{pmatrix}I2&-\sigmax&-\sigmay&-\sigmaz\end{pmatrix}
\mu\partial | |
\sigma | |
\mu |
\psi\rm=0
\mu\partial | |
\bar{\sigma} | |
\mu |
\psi\rm=0~.
\operatorname{SL}(2,C)
\operatorname{Sp}(2,C).
\operatorname{SO}(1,3).
\operatorname{SL}(2,C)
The double-covering of the Lorentz group is given by
\overline{\sigma}\mu
\mu} | |
{Λ | |
\nu |
=S\overline{\sigma}\nuS\dagger
where
Λ\in\operatorname{SO}(1,3)
S\in\operatorname{SL}(2,C)
S\dagger
x\mapstox\prime=Λx
The symplectic group
\operatorname{Sp}(2,C)
S
\omega-1Ssf{T}\omega=S-1
where
\omega=i\sigma2=\begin{bmatrix}0&1\ -1&0\end{bmatrix}
is a skew-symmetric matrix. It is used to define a symplectic bilinear form on
C2.
u,v\inC2
u=\begin{pmatrix}u1\ u2\end{pmatrix} v=\begin{pmatrix}v1\ v2\end{pmatrix}
the symplectic product is
\langleu,v\rangle=-\langlev,u\rangle=u1v2-u2v1=usf{T}\omegav
usf{T}
u~.
\langleu,v\rangle=\langleSu,Sv\rangle
The skew matrix takes the Pauli matrices to minus their transpose:
\omega\sigmak\omega-1=
sf{T} | |
-\sigma | |
k |
for
k=1,2,3.
\sigma\mu
\mu} | |
{Λ | |
\nu |
=\left(S-1\right)\dagger\sigma\nuS-1
These two variants describe the covariance properties of the differentials acting on the left and right spinors, respectively.
x\mapstox\prime=Λx
| ||||
\sigma |
\psi\rm(x)\mapsto
| ||||
\sigma |
\psi\rm(x\prime) =\left(S-1\right)\dagger
| ||||
\sigma |
\psi\rm(x)
provided that the right-handed field transforms as
\psi\rm(x)\mapsto
\prime | |
\psi | |
\rmR |
(x\prime)=S\psi\rm(x)
Similarly, the left-handed differential transforms as
| ||||
\overline{\sigma} |
\psi\rm(x)\mapsto
| ||||
\overline{\sigma} |
\psi\rm(x\prime) =S
| ||||
\overline{\sigma} |
\psi\rm(x)
\psi\rm(x)\mapsto
\prime | |
\psi | |
\rmL |
(x\prime)=\left(S\dagger\right)-1\psi\rm(x)
The complex conjugate of the right handed spinor field transforms as
* | |
\psi | |
\rmR |
(x)\mapsto
\prime* | |
\psi | |
\rmR |
(x\prime)=S*\psi
* | |
\rmR |
(x)
The defining relationship for
\operatorname{Sp}(2,C)
\omegaS*=\left(S\dagger\right)-1\omega.
* | |
m\omega\psi | |
\rmR |
(x)\mapsto
\prime* | |
m\omega\psi | |
\rmR |
(x\prime)=\left(S\dagger\right)-1
* | |
m\omega\psi | |
\rmR |
(x)
This is fully compatible with the covariance property of the differential. Taking
η=ei\phi
i\sigma\mu\partial\mu\psi\rm(x)+η
* | |
m\omega\psi | |
\rmR |
(x)
transforms in a covariant fashion. Setting this to zero gives the complex two-component Majorana equation for the right-handed field. Similarly, the left-chiral Majorana equation (including an arbitrary phase factor
\zeta
i\overline{\sigma}\mu\partial\mu\psi\rm(x)+\zeta
* | |
m\omega\psi | |
\rmL |
(x)=0
The left and right chiral versions are related by a parity transformation. As shown below, these square to the Klein–Gordon operator only if
η=\zeta.
\omega\psi*=i\sigma2\psi
\psi~;
Define a pair of operators, the Majorana operators,
\begin{align} D\rm&=i\overline{\sigma}\mu\partial\mu+\zetam\omegaK& D\rm&=i\sigma\mu\partial\mu+ηm\omegaK \end{align}
K
\begin{align} D\rm\mapsto
\prime | |
D | |
\rmL |
&=SD\rmS\dagger& D\rm\mapsto
\prime | |
D | |
\rmR |
&=\left(S\dagger\right)-1D\rmS-1\end{align}
\begin{align} \psi\rm\mapsto
\prime | |
\psi | |
\rmL |
&=\left(S\dagger\right)-1\psi\rm& \psi\rm\mapsto
\prime | |
\psi | |
\rmR |
&=S\psi\rm\end{align}
\begin{align} D\rm\psi\rm&=0& D\rm\psi\rm&=0 \end{align}
The products
D\rmD\rm
D\rmD\rm
D\rmD\rm=\left(i\sigma\mu\partial\mu+ηm\omegaK\right)\left(i\overline{\sigma}\mu\partial\mu+\zetam\omegaK\right) =-
2 | |
\left(\partial | |
t |
-\vec\nabla ⋅ \vec\nabla+η\zeta*m2\right) =-\left(\square+η\zeta*m2\right)
\omega2=-1
Ki=-iK~.
η\zeta*=1
η=\zeta~.
The real four-component version of the Majorana equation can be constructed from the complex two-component equation as follows. Given the complex field
\psi\rm
D\rm\psi\rm=0
\chi\rm\equiv-η\omega
* | |
\psi | |
\rmL |
Using the algebraic machinery given above, it is not hard to show that
\left(i\sigma\mu\partial\mu-ηm\omegaK\right)\chi\rm=0
Defining a conjugate operator
\delta\rm=i\sigma\mu\partial\mu-ηm\omegaK
The four-component Majorana equation is then
\left(D\rm ⊕ \delta\rm\right)\left(\psi\rm ⊕ \chi\rm\right)=0
Writing this out in detail, one has
D\rm ⊕ \delta\rm=\begin{bmatrix}D\rm&0\ 0&\delta\rm\end{bmatrix}= i\begin{bmatrix}I&0\ 0&I\end{bmatrix}\partialt +i\begin{bmatrix}-\sigmak&0\ 0&\sigmak\end{bmatrix}\nablak +m\begin{bmatrix}η\omegaK&0\ 0&-η\omegaK\end{bmatrix}
Multiplying on the left by
\beta=\gamma0=\begin{bmatrix}0&I\ I&0\end{bmatrix}
\beta\left(D\rm ⊕ \delta\rm\right)=\begin{bmatrix}0&\delta\rm\ D\rm&0\end{bmatrix}= i\beta\partialt+ i\begin{bmatrix}0&\sigmak\ -\sigmak&0\end{bmatrix}\nablak- m\begin{bmatrix}0&η\omegaK\ -η\omegaK&0\end{bmatrix}
That is,
\beta\left(D\rm ⊕ \delta\rm\right)=i\gamma\mu\partial\mu-m\begin{bmatrix}0&η\omegaK\ -η\omegaK&0\end{bmatrix}
Applying this to the 4-spinor
\psi\rm ⊕ \chi\rm=\begin{pmatrix}\psi\rm\ \chi\rm\end{pmatrix} =\begin{pmatrix}\psi\rm
* | |
\ -η\omega\psi | |
\rmL |
\end{pmatrix}
\omega2=-1
\begin{bmatrix}0&η\omegaK\ -η\omegaK&0\end{bmatrix} \begin{pmatrix}\psi\rm
* | |
\ -η\omega\psi | |
\rmL |
\end{pmatrix}= \begin{pmatrix}\psi\rm
* | |
\ -η\omega\psi | |
\rmL |
\end{pmatrix}
\left(i\gamma\mu\partial\mu-m\right)\begin{pmatrix} \psi\rm\\
* | |
-η\omega\psi | |
\rmL |
\end{pmatrix}=0
The skew matrix can be identified with the charge conjugation operator (in the Weyl basis). Explicitly, this is
C=\begin{bmatrix}0&η\omegaK\ -η\omegaK&0\end{bmatrix}
Given an arbitrary four-component spinor
\psi~,
C\psi=\psic=ηC\overline{\psi}sf{T}
with
C
\begin{align} 0&=\left(i\gamma\mu\partial\mu-mC\right)\psi\\ &=i\gamma\mu\partial\mu\psi-m\psic\end{align}
The charge conjugation operator appears directly in the 4-component version of the Majorana equation. When the spinor field is a charge conjugate of itself, that is, when
\psic=\psi,
The charge conjugation operator
C
C\psi=\psic=ηC\left(\overline\psi\right)sf{T}
A general discussion of the physical interpretation of this operator in terms of electrical charge is given in the article on charge conjugation. Additional discussions are provided by Bjorken & Drell[11] or Itzykson & Zuber. In more abstract terms, it is the spinorial equivalent of complex conjugation of the
U(1)
U(1)
*:U(1)\toU(1) ei\phi\mapsto e-i\phi
U(1).
U(1).
In the above,
C
C
\psi
\psi
K
K(x+iy)=x-iy,
C=-η\gamma0CK
It is not hard to show that
C2=1
C\gamma\muC=-\gamma\mu~.
C
C\psi(\pm)=\pm\psi(\pm)
The eigenvectors are readily found in the Weyl basis. From the above, in this basis,
C
C=\begin{bmatrix}0&η\omegaK\ -η\omegaK&0\end{bmatrix}
and thus
(\pm) | |
\psi | |
Weyl |
=\begin{pmatrix}\psi\rm\ \mpη
* | |
\omega\psi | |
\rmL |
\end{pmatrix}
Both eigenvectors are clearly solutions to the Majorana equation. However, only the positive eigenvector is a solution to the Dirac equation:
0=\left(i\gamma\mu\partial\mu-mC\right)\psi(+)=\left(i\gamma\mu\partial\mu-m\right)\psi(+)
The negative eigenvector "doesn't work", it has the incorrect sign on the Dirac mass term. It still solves the Klein–Gordon equation, however. The negative eigenvector is termed the ELKO spinor.
Under parity, the left-handed spinors transform to right-handed spinors. The two eigenvectors of the charge conjugation operator, again in the Weyl basis, are
(\pm) | |
\psi | |
\rm{R |
,Weyl
As before, both solve the four-component Majorana equation, but only one also solves the Dirac equation. This can be shown by constructing the parity-dual four-component equation. This takes the form
\beta\left(\delta\rm ⊕ D\rm\right)=i\gamma\mu\partial\mu+mC
\delta\rm=i\overline{\sigma}\mu\partial\mu-ηm\omegaK
Given the two-component spinor
\psi\rm
\chi\rm=-η
* | |
\omega\psi | |
\rmR |
.
D\rm\psi\rm=-η\omega(\delta\rm\chi\rm)
D\rm\psi\rm=0
\delta\rm\chi\rm=0
0=\left(\delta\rm ⊕ D\rm\right)\left(\chi\rm ⊕ \psi\rm\right)
0=(i\gamma\mu\partial\mu+mC)\begin{pmatrix}\chi\rm\ \psi\rm\end{pmatrix}
C(\chi\rm ⊕ \psi\rm)=-(\chi\rm ⊕ \psi\rm)
(-) | |
\psi | |
{\rmR |
,Weyl
To conclude, and reiterate, the Majorana equation is
0=\left(i\gamma\mu\partial\mu-mC\right)\psi=i\gamma\mu\partial\mu\psi-m\psic
It has four inequivalent, linearly independent solutions,
(\pm) | |
\psi | |
\rmL,R |
.
(+) | |
\psi | |
\rmL |
(-) | |
\psi | |
\rmR |
~.
One convenient starting point for writing the solutions is to work in the rest frame way of the spinors. Writing the quantum Hamiltonian with the conventional sign convention
H=i\partialt
i\partialt\psi=-i\vec\alpha ⋅ \nabla\psi+m\beta\psic
In the chiral (Weyl) basis, one has that
\gamma0=\beta=\begin{pmatrix}0&I\ I&0\end{pmatrix}, \vec\alpha=\begin{pmatrix}\vec\sigma&0\ 0&-\vec\sigma\end{pmatrix}
\vec\sigma
(+) | |
\psi | |
Weyl |
i\partialt\psi\rm=-i\vec\sigma ⋅ \nabla\psi\rm+m(i\sigma2
*) | |
\psi | |
\rmL |
i\partialt(i\sigma2
*) | |
\psi | |
\rmL |
=+i\vec\sigma ⋅ \nabla(i\sigma2
*) | |
\psi | |
\rmL |
+m\psi\rm
\sigma2
\sigma2\left(\veck ⋅ \vec\sigma\right)\sigma2=-\veck ⋅ \vec\sigma*.
The plane wave solutions can be developed for the energy-momentum
\left(k0,\veck\right)
(u) | |
\psi | |
\rmL |
=\begin{pmatrix}e-imt\ eimt\end{pmatrix}
(d) | |
\psi | |
\rmL |
=\begin{pmatrix}eimt\ -e-imt\end{pmatrix}
That these are being correctly interpreted can be seen by re-expressing them in the Dirac basis, as Dirac spinors. In this case, they take the form
(u) | |
\psi | |
Dirac |
=\begin{bmatrix}e-imt\ 0\ 0\ -eimt\end{bmatrix}
(d) | |
\psi | |
Dirac |
=\begin{bmatrix}0\ e-imt\ -eimt\ 0\end{bmatrix}
In a general momentum frame, the Majorana spinor can be written as
The appearance of both and in the Majorana equation means that the field cannot be coupled to a charged electromagnetic field without violating charge conservation, since particles have the opposite charge to their own antiparticles. To satisfy this restriction, must be taken to be electrically neutral. This can be articulated in greater detail.
The Dirac equation can be written in a purely real form, when the gamma matrices are taken in the Majorana representation. The Dirac equation can then be written as
\left(-i | \partial |
\partialt |
-i\hat\alpha ⋅ \nabla+\betam\right)\psi=0
\hat\alpha
\beta
\operatorname{Spin}(1,3).
\operatorname{Spin}C(1,3).
This can also be stated in a different way: the Dirac equation, and the Dirac spinors contain a sufficient amount of gauge freedom to naturally encode electromagnetic interactions. This can be seen by noting that the electromagnetic potential can very simply be added to the Dirac equation without requiring any additional modifications or extensions to either the equation or the spinor. The location of this extra degree of freedom is pin-pointed by the charge conjugation operator, and the imposition of the Majorana constraint removes this extra degree of freedom. Once removed, there cannot be any coupling to the electromagnetic potential, ergo, the Majorana spinor is necessarily electrically neutral. An electromagnetic coupling can only be obtained by adding back in a complex-number-valued phase factor, and coupling this phase factor to the electromagnetic potential.
The above can be further sharpened by examining the situation in
(p,q)
\operatorname{Spin}C(p,q)
\operatorname{SO}(p,q) x S1
S1\congU(1)
\operatorname{SO}(p,q)
U(1)
d+A.
A
A
R
F=dA.
(p,q)=(1,3)
The quanta of the Majorana equation allow for two classes of particles, a neutral particle and its neutral antiparticle. The frequently applied supplemental condition corresponds to the Majorana spinor.
See main article: Majorana particle.
Particles corresponding to Majorana spinors are known as Majorana particles, due to the above self-conjugacy constraint. All the fermions included in the Standard Model have been excluded as Majorana fermions (since they have non-zero electric charge they cannot be antiparticles of themselves) with the exception of the neutrino (which is neutral).
Theoretically, the neutrino is a possible exception to this pattern. If so, neutrinoless double-beta decay, as well as a range of lepton-number violating meson and charged lepton decays, are possible. A number of experiments probing whether the neutrino is a Majorana particle are currently underway.[14]