Abstract
We study the “shear-free” part of the Goldberg–Sachs theorem for type II and D six-dimensional Einstein spacetimes. A spacetime is of the type II or D if it admits a double Weyl aligned null direction (WAND). The Goldberg–Sachs theorem then restricts geometric properties of double WANDs. This restriction can be expressed in terms of constraints on the form of the “optical matrix” defining the expansion, rotation, and shear of the double WAND. We show that a rank-four and rank-three optical matrix is orthogonally similar to one of three canonical forms, reducing the number of free parameters of the optical matrix from ten to five.
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Notes
Making further assumptions about the r-dependence of various quantities—see footnote 7 therein.
Genuine Weyl types II and D do not include the more special Weyl types III, N, and O.
In fact, the polynomial order is even constant across each row of \(\varvec{M}\).
The two identities are contained in the Fadeev–LeVerrier algorithm: the first one is an intermediate result of the algorithm, whereas the second one is an application of the theorem itself.
Here we use the fact that \(\varvec{Q}\) is of rank 3: \(\delta _{2} = \delta _{3} = 0\) implies that at least one of \(\delta _{4}\), \(\delta _{5}\) is non-vanishing, and thus either columns 2, 3, 4 or columns 2, 3, 5 are linearly independent, leaving collinearity of columns 4, 5 the only possibility.
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Acknowledgements
This work has been supported by research plan RVO: 67985840. V. P. has been supported by the Czech Science Foundation Grant No GAČR 19-09659S. The work was done under the auspices of the Albert Einstein Center for Gravitation and Astrophysics, Czech Republic.
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A Solution to \(\mu = 0\)
A Solution to \(\mu = 0\)
We define \(\mu \) as in (79a)
where
Let us discuss solutions of the equation
Note that
Proposition 4
For each solution of the equation \(\mu = 0\), at least one of the following conditions is fulfilled
Proof
Let us suppose that none of (93a)–(93d) holds. We will show that then (93e) must hold.
It is straightforward to see that \(\mu = 0\) implies
Therefore, under the given assumptions,
Treating \(\mu \) as a quadratic polynomial in \(\alpha \) and \(\gamma \), we see that each time, the discriminant is non-positive, so we complete the square
where
As both \(\beta \gamma \) and \(\alpha \beta \) are strictly positive, four equalities follow from \(\mu = 0\)
Choosing an appropriate combination of \( h_{1}\) and \( h_{2} \) gives
The first factor is strictly positive due to (95) and thus
Hence, considering (95) again,
Considering \(k_{1} = 0\), \(k_{2} = 0\), one of the following two conditions must hold
However, it can be seen from (89) and (95) that it is impossible to achieve (102a). \(\square \)
Corollary 1
The equation
has the following set of roots, parametrized by real x, y, z,
Proof
To see that (104) solves \(\mu = 0\), one can substitute into (89)
It is obvious that cases (93b)–(93d) can be parametrized according to (104). In order to complete the proof, it suffices to show that this parametrization can be also applied to the case (93e).
Let us assume (93e)
Hence
The determinant necessarily vanishes
Thus one can introduce x and y such that
By substituting this parametrization into (107), we get
which implies
Finally, one can introduce z such that
\(\square \)
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Tintěra, T., Pravda, V. On the Goldberg–Sachs theorem in six dimensions. Gen Relativ Gravit 51, 111 (2019). https://doi.org/10.1007/s10714-019-2592-4
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DOI: https://doi.org/10.1007/s10714-019-2592-4