
arXiv:2210.02423v1 [gr-qc] 5 Oct 2022
A SPACE-TIME CALCULUS BASED ON SYMMETRIC 2-SPINORS
STEFFEN AKSTEINER AND THOMAS B ¨
ACKDAHL
Abstract. In this paper we present a space-time calculus for symmetric spinors, including a
product with a number of index contractions followed by symmetrization. As all operations
stay within the class of symmetric spinors, no involved index manipulations are needed. In fact
spinor indices are not needed in the formalism. It is also general because any covariant tensor
expression in a 4-dimensional Lorentzian spacetime can be translated to this formalism. The
computer algebra implementation SymSpin as part of xAct for Mathematica is also presented.
1. Introduction
When working with tensorial expressions, one usually encounters difficulties handling index
manipulations due to complicated symmetries. Techniques including group theoretical calcula-
tions and Young tableaux have been introduced to try to tackle these problems. However, their
complexity grows quickly with the size of the problem. The purpose of this paper is to present
a formalism based on 2-spinors that aims to simplify the situation by utilizing the symmetry
properties of irreducible spinors.
Let (M, gab) be a 4-dimensional manifold with metric gab of Lorentzian signature and admitting
a spin structure with spin metric ǫAB . It is well known that any tensor field on Mcan be expressed
in terms of 2-spinors, which in turn can be decomposed into irreducible symmetric spinors [9,
Prop 3.3.54]. For instance a valence (3,0) spinor can be decomposed as
TABC =T(ABC)+1
3TDD(BǫC)A−1
3ǫA(BTDC)D−1
2TADDǫBC .(1)
Therefore, it is sufficient to work with with symmetric spinors. To fully establish this perspective,
a symmetric product for symmetric spinors with a number of contractions is needed. It is the
intention of this work to introduce the corresponding algebra and to derive its basic properties.
In particular, with these operations we stay within the algebra of symmetric spinors. This offers
great simplifications, and speeds up the calculations. Furtheremore, no relevant information is
left in the indices, and we therefore get an index-free compact formalism.
We have previously described the decomposition of the covariant derivative [4], leading to four
fundamental spinor operators, which can be viewed as a special case. Also, the symmetric product
is a generalization of some special operators, like the Kioperators defined in [1, Definition II.4].
Therefore, all properties of such operators can easily be derived from the corresponding properties
of the symmetric product described in this paper.
The formalism has many potential applications, see [2],[3]. As a simple example, consider a
condition of the form
0 = KAB F H LFCϕHC +M(ACϕB)C,(2)
for symmetric spinors K, L, M, ϕ. For arbitrary ϕa systematic computation, using the techniques
of this paper, shows that the conditions on K, L, M are of the form
KG(ABC L|G|F)= 0, MAB =1
2KCF AB LCF ,(3)
see Section 3.2 for details. The same techniques have been used in [7] to derive conditions on the
spacetime for the existence of second order symmetry operators for the massive Dirac equation.
The formalism is implemented in the SymSpin [5] package for xAct [8] for Mathematica.
In Section 2we introduce the symmetric product and state basic properties in Theorem 3.
The expansion of a product into symmetric products is discussed in Lemma 6. The irreducible
parts of the Levi-Civita connection, its commutators, curvature and Leibniz rules are discussed
in Section 2.4. A concise form the the dyad components of such symmetric spinors is given
1