Abstract
In this paper we calculate the Bondi mass of asymptotically flat spacetimes with interacting electromagnetic and scalar fields. The system of coupled Einstein–Maxwell–Klein–Gordon equations is investigated and corresponding field equations are written in the spinor form and in the Newman–Penrose formalism. Asymptotically flat solution of the resulting system is found near null infinity. Finally we use the asymptotic twistor equation to find the Bondi mass of the spacetime and derive the Bondi mass-loss formula. We compare the results with our previous work (Bičák et al. in Class Quantum Gravity 27(17):175011, 2010) and show that, unlike the conformal scalar field, the (Maxwell–)Klein–Gordon field has negatively semi-definite mass-loss formula.
Similar content being viewed by others
Notes
In order to calculate the Bondi mass, the analyticity is not necessary and weaker assumptions on the differentiability of the solution could be imposed. In what follows we use the analyticity to argue that the mass of the Klein–Gordon field must be zero.
This depends on the conventions used. What is convention-independent is the behaviour of the Weyl tensor \(C_{abcd}=\varPsi _{ABCD}\varepsilon _{A'B'}\varepsilon _{C'D'}\). In the non-abstract index formalism, components of tensors are related to components of spinors via van der Waerden symbols \(\sigma _a^{AA'}\) which can have a conformal weight and thus they affect the conformal weight of \(\varPsi _{ABCD}\), as in, e.g. [22].
By the Newman–Penrose quantities we mean five components \(\varPsi _m,\,m=0,\dots 4\), six independent components \(\varPhi _{mn},\,m,n=0,1,2\), twelve spin coefficients, three electromagnetic components \(\phi _m,\,m=0,1,2\), four components of the potential \(A_m,\,m=0,1,\overline{1},2\), and the scalar field \(\phi \).
References
Bičák, J., Scholtz, M., Tod, P.: On asymptotically flat solutions of Einstein’s equations periodic in time: II. Spacetimes with scalar-field sources. Class. Quantum Gravity 27(17), 175011 (2010). doi:10.1088/0264-9381/27/17/175011
Penrose, R.: Quasi-local mass and angular momentum in general relativity. R Soc Lond Proc. Ser. A 381, 53–63 (1982). doi:10.1098/rspa.1982.0058
Hawking, S.W.: Gravitational radiation in an expanding universe. J. Math. Phys. 9(4), 598–604 (1968)
Dougan, A.J., Mason, L.J.: Quasilocal mass constructions with positive energy. Phys. Rev. Lett. 67, 2119–2122 (1991)
Brown, J.D., York Jr, J.W.: Quasilocal energy and conserved charges derived from the gravitational action. Phys. Rev. D 47, 1407–1419 (1993)
Szabados, L.B.: Quasi-local energy-momentum and angular momentum in GR: a review article. Living Rev. Relativ. 7 (2004)
Jaramillo, J.L., Gourgoulhon, E.: Mass and angular momentum in general relativity. In: Blanchet, L., pallicci, A., Whiting, B. (eds.) Mass and Motion in General Relativity. Springer, Berlin (2011)
Arnowitt, R., Deser, S., Misner, C.W.: Republication of: the dynamics of general relativity. Gen. Relativ. Gravit. 40, 1997–2027 (2008)
Bondi, H., van der Burg, M.G.J., Metzner, A.W.K.: Gravitational waves in general relativity. VII. Waves from axi-symmetric isolated systems. R Soc. Lond. Proc. Ser. A 269, 21–52 (1962)
Geroch, R., Held, A., Penrose, R.: A space-time calculus based on pairs of null directions. J. Math. Phys. 14, 874–881 (1973)
Chrusciel, P.T., Jezierski, J., Kijowski, J.: A Hamiltonian field theory in the radiating regime. Springer, NewYork (2002)
Huang, C.: Bondi Mass in Scalar Fields. In: The 28th International Cosmic Ray Conference in Tsukuba, pp. 3145–3148. Universal Academy Press Inc, Tokyo (2013)
Tod, K.P.: Penrose’s quasi-local mass. In: Bailey, T.N., Baston, R.J. (eds.) Twistors in Mathematics and Physics. Cambridge University Press, Cambridge (1990)
Tod, K.P.: Some examples of Penrose’s quasi-local mass construction. R. Soc. Lond. Proc. Ser. A 388, 457–477 (1983)
Tod, K.P.: More on Penrose’s quasi-local mass. Class. Quantum Gravity 3, 1169–1189 (1986). doi:10.1088/0264-9381/3/6/016
Gegenberg, J.D., Das, A.: An exact stationary solution of the combined Einstein–Maxwell–Klein–Gordon equations. J. Math Phys. 22, 1736–1739 (1981)
Hawking, S.W., Ellis, G.F.R.: The Large Scale Structure of Space-Time. Cambridge University Press, Cambridge (1975)
Penrose, R., Rindler, W.: Spinors and Space-Time. Vol. 1: Two-Spinor Calculus and Relativistic Fields. Cambridge University Press, Cambridge (1984)
Stewart, J.: Advanced General Relativity. Cambridge University Press, Cambridge (1993)
Bičák, J., Scholtz, M., Tod, P.: On asymptotically flat solutions of Einstein’s equations periodic in time: I. Vacuum and electrovacuum solutions. Class. Quantum Gravity 27(5), 055007 (2010). doi:10.1088/0264-9381/27/5/055007
Penrose, R., Rindler, W.: Spinors and Space-Time. Volume 2: Spinor and Twistor Methods in Space-Time Geometry. Cambridge University Press, Cambridge (1986)
Penrose, R.: Zero rest-mass fields including gravitation: asymptotic behaviour. R. Soc. Lond. Proc. Ser. A 284, 159–203 (1965). doi:10.1098/rspa.1965.0058
Adamo, T.M., Kozameh, C., Newman, E.T.: Null geodesic congruences, asymptotically-flat spacetimes and their physical interpretation. Living Rev. Relativ. 12, 6 (2009)
Newman, E.T., Penrose, R.: An approach to gravitational radiation by a method of spin coefficients. J. Math. Phys. 3(3), 566–578 (1962)
Winicour, J.: Massive fields at null infinity. J. Math. Phys. 29, 2117–2121 (1988)
Helfer, A.D.: Null infinity does not carry massive fields. J. Math. Phys. 34, 3478–3480 (1993)
Huggett, S.A., Tod, K.P.: An Introduction to Twistor Theory. Cambridge University Press, Cambridge (1994)
Szabados, L.B.: Two-dimensional Sen connections in general relativity. Class. Quantum Gravity 11, 1833–1846 (1994). doi:10.1088/0264-9381/11/7/019
Szabados, L.B.: Two-dimensional Sen connections and quasi-local energy-momentum. Class. Quantum Gravity 11, 1847–1866 (1994). doi:10.1088/0264-9381/11/7/020
Acknowledgments
This work was supported by the grant GAUK 606412 of the Charles University of Prague, Czech Republic and the grant GAČR 202/09/0772 of the Czech science foundation. The authors acknowledge useful discussions with Paul Tod and Szabados László. In particular, we are grateful to Paul Tod for his comments on the original manuscript.
Author information
Authors and Affiliations
Corresponding author
Appendix 1: Field equations in the Newman–Penrose formalism
Appendix 1: Field equations in the Newman–Penrose formalism
Four-potential \(A_a = A_{AA'}\) is a real vector field and its components with respect to the spin basis will be denoted by
Similarly we introduce the Newman–Penrose components of electromagnetic spinor \(\phi _{AB}\) by
Potential \(A_a\) is governed by Eq. (8),
Projections of this equation onto the spin basis are
The Lorenz condition \(\nabla ^a A_a = 0\) in the Newman–Penrose formalism acquires the form
Projections of the gradient \(\varphi _{AA'}=\nabla _{AA'}\phi \) will be denoted by
Now we can complete equations for electromagnetic field. Equation (9),
is the spinor version of Maxwell’s equations with four-current \(j^a\) on the right hand side. Projections of this equation onto the spin basis follow:
Dynamical equation for the gradient \(\varphi _{AA'}\) is provided by Eq. (12)
Projected on the spin basis, this equation is equivalent to any of the following four scalar equations:
The Ricci spinor is related to the electro-scalar fields by Einstein’s equations (16) and is given by formula (18). The Newman–Penrose components of the Ricci spinor read:
The Ricci identities in the tetrad introduced in Sect. 3 simplify to the following set of equations.
Rights and permissions
About this article
Cite this article
Scholtz, M., Holka, L. On the Bondi mass of Maxwell–Klein–Gordon spacetimes. Gen Relativ Gravit 46, 1665 (2014). https://doi.org/10.1007/s10714-014-1665-7
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s10714-014-1665-7