Abstract
The gravitational field of an idealized plane-wave solution of the Maxwell equations can be described in closed form. After discussing this particular solution of the Einstein-Maxwell equations, the motion of neutral test particles, which are sensitive only to the gravitational background field, is analyzed. This is followed by a corresponding analysis of the dynamics of neutral fields in the particular Einstein-Maxwell background, considering scalars, Majorana spinors and abelian vector fields, respectively.
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Notes
- 1.
For a discussion of the role of the universal constant c characterizing the relations between inertial frames, see ref. [1].
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Acknowledgements
Discussions with Ernst Traanberg of the Lorentz Institute in Leiden on solving field equations in the plane-wave background are gratefully acknowledged.
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Appendix: Spinors and the Dirac Algebra
Appendix: Spinors and the Dirac Algebra
Spinor fields in curved space-time are most easily described in the tangent Minkowski space, using the vierbein formulation to translate the results to the curved space-time manifold. We use the flat-space representation of the Dirac algebra in which \(\gamma _5\) is diagonal:
such that for \(a = (0,1,2,3)\)
The generators of the Lorentz transformations on spinors are defined by
with commutation relations
Hermitean conjugation is achieved by
The charge conjugation operator C is defined by
such that
If the spinor \(\Psi \) is a solution of the Dirac equation in Minkowski space
then this is also true for the charge-conjugate:
The Majorana constraint \(\Psi ^c = \Psi \) reduces the number of independent spinor components from 4 to 2 complex ones. This makes it easy to work in terms of 2-component spinors \((\chi , \eta )\) which are eigenspinors of \(\gamma _5\), by the decomposition
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Holten, J.W.v. (2023). The Gravity of Light. In: Pfeifer, C., Lämmerzahl, C. (eds) Modified and Quantum Gravity. Lecture Notes in Physics, vol 1017. Springer, Cham. https://doi.org/10.1007/978-3-031-31520-6_15
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