Polarization spin-tensors in two-spinor formalism and Behrends-Fronsdal spin projection operator for $D$-dimensional case
Mikhail Podoinitsyn

TL;DR
This paper derives differential relations linking polarization spin-tensors of free massive particles of arbitrary spin in four dimensions and introduces a new formula for the Behrends-Fronsdal spin projection operator in arbitrary dimensions.
Contribution
It presents novel recurrent differential relations and a new formula for the Behrends-Fronsdal spin projection operator in D-dimensional space.
Findings
Derived differential relations for polarization spin-tensors in 4D.
Formulated a new D-dimensional Behrends-Fronsdal spin projection operator.
Enhanced understanding of spin projection in higher-dimensional theories.
Abstract
In the work, the recurrent differential relations that connecting the polarization spin-tensor of the wave function of a free massive particle of an arbitrary spin for and new formula of the -dimensional Behrends-Fronsdal spin projection operator are found.
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Polarization spin-tensors in two-spinor formalism
and Behrends-Fronsdal spin projection operator
for -dimensional case.
M.A. Podoinitsyn 111e-mail: [email protected]
Bogoliubov Laboratory of Theoretical Physics, JINR, Dubna 141980, Russia
Abstract
In the work, the recurrent differential relations that connecting the polarization spin-tensor of the wave function of a free massive particle of an arbitrary spin for and new formula of the -dimensional Behrends-Fronsdal spin projection operator are found.
1 Introduction
This work is a continuation of the article [1]. The [1] is devoted to a two-spinor description of free massive particles of arbitrary spin and to the Berends-Fronsdal projection operators – a projector onto irreducible completely symmetric representations of the -dimensional Poincaré group. Each of these two sections received a small addition in the present work.
We briefly recall the main results of the [1]. We use the Wigner unitary representations of the group , which covers the Poincaré group. These representations are irreducible and one can reformulate them in such a way that these irreps act in the space of spin-tensor wave functions of a special type. The construction of the functions is carried out with the help of Wigner operators, which translate the unitary massive representation of the group (induced from the irreducible representation of the stability subgroup ) acting in the space of Wigner wave functions to a representation of the group , acting in the space of special spin-tensor fields of massive particles. In addition, the generalization on arbitrary dimension of the four-dimensional Behrends-Fronsdal spin projection operator was found.
In the first section of this article, for fixing the notation and material consistency, we present the definitions of the spin-tensor wave function the polarization spin-tensors and the expansion formula for to the sum over the polarization spin-tensors. Further, using a special parametrization of Wigner operators in terms of two Weyl spinors, we prove the main Proposition 1** ** of the first section. On the existence of differential recurrence relations connecting various polarization spin-tensors . These relations allow us to write out explicit expressions for the polarization spin-tensors in terms of two spinors.
In the second part of the paper, we describe a new method for constructing of the Berends-Fronsdal spin projection operator for -dimensional case.
2 Polarization spin-tensors for the field of arbitrary spin.
Based on the Wigner construction of massive unitary and irreducible representations of the covering Poincare group , one can show (see [1]) that the space of the unitary representation of the group with spin is transformed to the space of the spin-tensor wave functions of - type depending on four-momentum :
[TABLE]
Here , – is an arbitrary symmetric tensor of rank (the Wigner wave function), – are components of the test four-momentum :
[TABLE]
parameter is the mass, and – are Pauli matrices while – is the unit matrix. Matrices , used in (2.1), are solutions of the equations
[TABLE]
The matrix parametrizes coset space . The upper index of the spin-tensors in (2.1) distinguishes these spin-tensors with respect to the number of dotted indices. In eq. (2.1) we use operators A_{(k)}^{\otimes p}\otimes\bigl{(}A^{\dagger-1}_{(k)}(q\tilde{\sigma})\bigr{)}^{\otimes r} to translate the Wigner wave functions into spin-tensor functions of -type, These operators are called the Wigner operators.
According to [1], the spin-tensor wave functions can be represented as the following sum over the polarization spin-tensors .
[TABLE]
The explicit form of the coefficients is not needed here (you can see it in [1]), if the test momentum is fixed as polarizations are given by
[TABLE]
where we introduced
[TABLE]
where the componets of the auxiliary Weyl Spinor.
Proposition 1
The spin-tensors , defined in (2.4) satisfy the relations:
[TABLE]
[TABLE]
[TABLE]
where - Weyl spinors.
Proof. The proof is based on the use the representation of matrices in terms of Weyl spinors
[TABLE]
[TABLE]
proposed in paper [1]. Let us show, for example, how one can prove of relation (2.7). The proofs of relations (2.6), (2.8) are similar. First of all we consider the obvious identity which follows from definitions (2.5):
[TABLE]
Now we expand the numerator of the right-hand side of the formula (2.11)
[TABLE]
Then we substitute (2.11) into (2.4) and use (2.12)
[TABLE]
here we have divided the sum over in two parts (it will be needed for further consideration). We also need the following identities
[TABLE]
which follow from (2.9) and (2.10). Note that the relations are holds
[TABLE]
From the identities (2.14) and the relations (2.15) we can get formulas
[TABLE]
Using first identities (2.14) and then (2.16), the right-hand side of formula (2.13) (without numeric factor and monomial ) can be rewritten as follows
[TABLE]
Now we add to (2.17) the following zero terms
[TABLE]
And as a result the sum of (2.17) and (2.18) has the form
[TABLE]
where to obtain equality we used the product rule. Further, substituting the right-hand side (2.19) in (2.13), we are convinced of the validity of the relation (2.7).
Remark 1. Formulas from Proposition 1 can be used to construct tensors of arbitrary polarization , expressed in terms of Weyl spinors . We first construct the polarization tensor for , using the parametrization of the Wigner operators (2.4) in terms of parameterization (2.9) of operators
[TABLE]
Now, using recurrence formula (2.7) we can write the polarization tensor for
[TABLE]
Further, applying the formula (2.7), one can obtain all the polarization tensors.
3 Behrends-Fronsdal operator for -dimensional case.
Defenition 1 *The Behrends-Fronsdal projection operator uniquely determined by the following conditions
*1) projective property and reality: ;
*2) symmetry: ;
*3) transversality: , ;
*4) tracelessness: .
For the four-dimensional space-time , the Behrends-Fronsdal projection operator for any spin was explicitly constructed in [2], [3]. In [1], [4], [5] the generalization of the Behrends-Fronsdal operator to the case of an arbitrary number of dimensions was found. The construction was based on the properties of this operator, which are listed in Defenition 1.
Instead of the tensor symmetrized in the upper and lower indices, was considered the generating function
[TABLE]
For concreteness, we assume that the tensor with components is defined in the pseudo-Euclidean -dimensional space with an arbitrary metric , having the signature . Indices and in (3.1) run through values and , .
Proposition 2
(See [1]) The generating function (3.1) of the covariant projection operator (in -dimensional space-time), satisfying properties 1)-4), in Defenition 1, has the form
[TABLE]
where – integer part of , the coefficients satisfy recurrent relation
[TABLE]
The solution of equation (3.3) has the form
[TABLE]
, and the function is defined as follows ( – the metric of space ):
[TABLE]
Now we will prove some new statement about the generation fuction of the operator .
Proposition 3
For the generation function (3.1) the following recurrence formula is hold
[TABLE]
Here we defined element
[TABLE]
where and element have the form 222Here the operator really plays the role of a unit, since it trivially acts on all covariant combinations constructed from on (3.5) and space-time metric .
[TABLE]
where .
Proof. First we simplify the formula (3.6). Note, we will need it later, that the following formula is hold.
[TABLE]
Consider the differential operator
[TABLE]
from the right hand-side (3.6). Next we show, that (3.10) reduces to the following sum of two simple terms
[TABLE]
Then using (3.11) we can rewrite the formula (3.6)
[TABLE]
here we immediately differentiated by the variable .
We now show that the formula (3.11) is equivalent to (3.10). We carry out the proof by induction on . For the formula (3.7) is represented as
[TABLE]
We make a contraction similar to (3.10) for , using the formula (3.13) and the definition of the generating function из (3.5), as a result we have
[TABLE]
it follows that the formulas (3.11) and (3.10) is equivalent for . Now we consider the sequence of the transformations for the (3.10) in case any
[TABLE]
here in the first equality we used the recurrence relation (3.9), in the second equality we used the induction hypothesis (equivalence of formulas (3.11) and (3.10) for ), in the third equation we applied differentiation with respect to the auxiliary -vector .
We now show that the formula (3.12) is valid for the generating function (3.2). We act with the differential operator from the right-hand side (3.12) on the generating function , taken as a series (3.2)
[TABLE]
were the coefficients define by formula (3.4).
The result of the action will be the following components
[TABLE]
In the proof, we will consider the case when is an even number, the proof for odd is carried out in a similar way. Let’s make in each line (3.17) some transformations
[TABLE]
In the first line we excluded the first term from the total sum and we took into account the fact that for even the relation is hold. In the second line, we again used the equality and eliminated the obviously zero first term. In the third line, we eliminated the last term, then made a shift of the summation parameter , and used . Now we add all terms (3.18) as a result we get
[TABLE]
where the coefficient is determined by the following chain of equalities
[TABLE]
here we used the recurrence relation (3.3) for the coefficients . Substituting now the explicit expression for , we see that exactly coincides with . As a result, we can write
[TABLE]
4 Conclusion
We hope that the formalism considered in this paper for describing massive particles of arbitrary spin will be useful in the construction of scattering amplitudes of massive particles in a similar way to the construction of spinor-helicity scattering amplitudes for massless particles [7], [8]. Some steps in this direction have already been done in papers [9],[10],[11] where the analogous formalism and its special generalization were used. We also think that using the methods from [6] the formulas (3.6) - (3.8) can be generalized for projection operators of any type of symmetry (corresponding to arbitrary Young diagrams).
The first part of this work was supported by RFBR, grant 18-52-05002 Арм_а; the second part was supported by RFBR, grant 19-01-00726А.
The author is grateful to A.P. Isaev for formulation of the problem and helpful discussions.
The reference list from the paper itself. Each links out to its DOI / PubMed record.
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