Abstract
Important early calculations in (\(3+1\)) cosmological spacetimes were carried out by Audretsch, and Schäfer [1, 2]. Several solutions in a non-cosmological context are [3,4,5,6,7,8,9,10]. In our first example we shall calculate the Fock-Ivanenkocoefficients and the resulting Dirac equations for the Schwarzschild metric (with signature (\(+2\))). The \(\gamma \) matrices are in the standard representation, however because of our signature choice, we have to multiply each of the matrices (B.8), with a factor of \(+i\). Then Eq. (B.9) change sign and Eq. (B.3) holds with \(\varepsilon =+1\).
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
J. Audretsch, G. Schäfer, Quantum mechanics of electromagnetically bounded spin-\(\frac{1}{2}\) particles in an expanding universe: I. Influence of the expansion. Gen. Relativ. Gravit. 9, 243–255 (1978)
J. Audretsch, G. Schäfer, Quantum mechanics of electromagnetically bounded spin-\(\frac{1}{2}\) particles in expanding universes: II. Energy spectrum of the hydrogen atom. Gen. Relativ. Gravit. 9, 489–500 (1978)
S. Chandrasekhar, The solution of Dirac’s equation in Kerr geometry. Proc. R. Soc. Lond. A. 349, 571–575 (1976)
D.N. Page, Dirac equation around a charged, rotating black hole. Phys. Rev. D 14, 1509–1510 (1976)
V.M. Villalba, Exact solution to Dirac equation in a reducible Einstein space. J. Math Phys. 31, 1483–1486 (1990)
D.-Y. Chen, Q.-Q. Jiang, X.-T. Zu, Hawking radiation of Dirac particles via tunnelling from rotating black holes in de Sitter spaces. Phys. Lett. B 665, 106–110 (2008)
H. Cebeci, N. Özdemir, Dirac equation in Kerr-Taub NUT spacetime. Class. Quantum Grav. 30, 175005 (2013)
O.V. Veko, E.M. Ovsiyuk, V.M. Red’kov, Dirac particle in the presence of a magnetic charge in de Sitter universe: exact solutions and transparency of the cosmological horizon. Nonlinear Phenom. Complex Syst. 17, 461–463 (2014)
L. Anderson, C. Bär, Wave and Dirac equations manifolds, pp. 1–21. 17 April 2018, arXiv:1710.04512v2
J.F. García, C. Sabín, Dirac equation in exotic space-times, pp. 1–7. 11 Nov 2018, arXiv:1811.00385v2
S. Chandrasekhar, The Mathematical Theory of Black Holes, (Clarendon Press, Oxford, 1992)
M.N. Hounkonnou, J.E.B. Mendy, Exact solutions of the Dirac equation in a nonfactorizable metric. J. Math. Phys. 40, 3827–3842 (1999)
L. Parker, One-electron atom as a probe of spacetime curvature. Phys. Rev. D 22, 1922–1934 (1980)
P. Collas, D. Klein, Dirac particles in a gravitational shock wave. Class. Quantum Grav. 35, 125006 (2018), https://doi.org/10.1088/1361-6382/aac144
C. Chicone, B. Mashhoon, Explicit Fermi coordinates and tidal dynamics in de Sitter and Gödel spacetimes. Phys. Rev. D 74, 064019 (2006)
D. Klein, P. Collas, General transformation formulas for Fermi-Walker coordinates. Class. Quantum Grav. 25, 145019 (2008), arXiv:0712.3838
D. Klein, P. Collas, Exact Fermi coordinates for a class of space-times. J. Math. Phys. 51, 022501 (2010)
D. Klein, E. Randles, Fermi coordinates, simultaneity, and expanding space in Robertson-Walker cosmologies. Ann. Henri Poincaré 12, 303–328 (2011)
D. Bini, A. Geralico, R.T. Jantzen, Fermi coordinates in Schwarzschild spacetime: closed form expressions. Gen. Relativ. Gravit. 43, 1837–1853 (2011)
D. Klein, Maximal Fermi charts and geometry of inflationary universes. Ann Henri Poincaré (2012). https://doi.org/10.1007/s00023-012-0227-3
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
Copyright information
© 2019 The Author(s), under exclusive license to Springer Nature Switzerland AG
About this chapter
Cite this chapter
Collas, P., Klein, D. (2019). Examples in (\(3+1\)) GR. In: The Dirac Equation in Curved Spacetime. SpringerBriefs in Physics. Springer, Cham. https://doi.org/10.1007/978-3-030-14825-6_4
Download citation
DOI: https://doi.org/10.1007/978-3-030-14825-6_4
Published:
Publisher Name: Springer, Cham
Print ISBN: 978-3-030-14824-9
Online ISBN: 978-3-030-14825-6
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)