Skip to main content

The Gravity of Light

  • Chapter
  • First Online:
Modified and Quantum Gravity

Part of the book series: Lecture Notes in Physics ((LNP,volume 1017))

  • 497 Accesses

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.

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Chapter
USD 29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD 79.99
Price excludes VAT (USA)
  • Available as EPUB and PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD 99.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Institutional subscriptions

Notes

  1. 1.

    For a discussion of the role of the universal constant c characterizing the relations between inertial frames, see ref. [1].

References

  1. G. Koekoek, J.W. van Holten and U. Wyder, The path to special relativity. Preprint (2022). https://arxiv.org/abs/2109.11925

  2. F. Dyson, A. Eddington, C. Davidson, A determination of the deflection of light by the sun’s gravitational field. Phil. Trans. R. Soc. A 220, 571 (1920)

    Google Scholar 

  3. K. Akiyama, et al., (Event Horizon Telescope Collaboration), First M87 event horizon telescope results. I. The shadow of the supermassive black hole. Astrophys. J. Lett. 875, L1 (2019)

    Google Scholar 

  4. B. Abbott, et al., (LIGO Scientific Collaboration and Virgo Collaboration), Observation of gravitational waves from a binary black-hole merger. Phys. Rev. Lett. 116, 061102 (2016)

    Google Scholar 

  5. H.W. Brinkmann, Proc. Natl. Acad. Sci. 9, 1 (1923)

    Article  ADS  Google Scholar 

  6. O. Baldwin, G. Jeffery, The relativity theory of plane waves. Proc. R. Soc. A 111, 95 (1926)

    ADS  MATH  Google Scholar 

  7. W. Rindler, Essential Relativity (Springer, Berlin, 1977)

    Book  MATH  Google Scholar 

  8. H. Stephani, D. Kramer, M. MacCallum, C. Hoenselaers, E. Herlt, Exact Solutions of Einstein’s Field Equations (Cambridge University Press, Cambridge, 2003)

    Book  MATH  Google Scholar 

  9. J.W. van Holten, Gravitational waves and masless particle fields, in Proceedings of the XXXVth Karpacz Winterschool of Theor. Physics, ed. by J. Kowalski-Glikman (Springer, Berlin, 1999), p. 365

    Google Scholar 

  10. J.W. van Holten, The gravitational field of a light wave. Fortschr. Phys. 59, 284 (2011)

    Article  MathSciNet  MATH  Google Scholar 

  11. J.W. van Holten, The gravity of light-waves. Universe 4, 110 (2018)

    Article  ADS  Google Scholar 

Download references

Acknowledgements

Discussions with Ernst Traanberg of the Lorentz Institute in Leiden on solving field equations in the plane-wave background are gratefully acknowledged.

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Jan W. van Holten .

Editor information

Editors and Affiliations

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:

(15.56)

such that for \(a = (0,1,2,3)\)

(15.57)

The generators of the Lorentz transformations on spinors are defined by

$$\displaystyle \begin{aligned} \sigma _{ab} = \frac{1}{4} \left[ \gamma _a, \gamma _b \right], {} \end{aligned} $$
(15.58)

with commutation relations

$$\displaystyle \begin{aligned} \left[ \sigma _{ab}, \sigma _{cd} \right] = \eta_{ad} \sigma _{bc} - \eta_{ac} \sigma _{bd} - \eta_{bd} \sigma _{ac} + \eta_{bc} \sigma _{ad}. {} \end{aligned} $$
(15.59)

Hermitean conjugation is achieved by

$$\displaystyle \begin{aligned} \gamma _a^{\dagger} = \gamma _0 \gamma _a \gamma _0. {} \end{aligned} $$
(15.60)

The charge conjugation operator C is defined by

$$\displaystyle \begin{aligned} C = C^{\dagger} = C^{-1} = - C^T = \gamma _2 \gamma _0 = \left( \begin{array}{cc} \sigma _2 & 0 \\ 0 & - \sigma _2 \end{array} \right), {} \end{aligned} $$
(15.61)

such that

$$\displaystyle \begin{aligned} C^{-1} \gamma _a C = - \gamma _a^T. {} \end{aligned} $$
(15.62)

If the spinor \(\Psi \) is a solution of the Dirac equation in Minkowski space

$$\displaystyle \begin{aligned} \left( \gamma \cdot \partial + m \right) \Psi = 0, {} \end{aligned} $$
(15.63)

then this is also true for the charge-conjugate:

(15.64)

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

(15.65)

Rights and permissions

Reprints and permissions

Copyright information

© 2023 The Author(s), under exclusive license to Springer Nature Switzerland AG

About this chapter

Check for updates. Verify currency and authenticity via CrossMark

Cite this chapter

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

Download citation

Publish with us

Policies and ethics