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Conclusions

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Part of the book series: SpringerBriefs in Physics ((SpringerBriefs in Physics))

Abstract

This chapter contains a summary of important properties of the shadow of black holes and an outlook on upcoming extension.

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Notes

  1. 1.

    The conclusions in the first and fifth paragraph can be found in [1] while the last sentence of the second paragraph as well as the fourth paragraph are taken from [3].

References

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  • Grenzebach A (2015) Aberrational effects for shadows of black holes. In: Puetzfeld et al Proceedings of the 524th WE-Heraeus-Seminar “Equations of Motion in Relativistic Gravity”, held in Bad Honnef, Germany, 17–23 Feb 2013, pp 823–832. doi:10.1007/978-3-319-18335-0_25, arXiv:1502.02861

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  • Grenzebach A, Perlick V, Lämmerzahl C (2015) Photon regions and shadows of accelerated black holes. Int J Mod Phys D 24(9):1542,024(22). doi:10.1142/S0218271815420249 (“Special Issue Papers” of the “7th Black Holes Workshop”, Aveiro, Portugal, arXiv:1503.03036)

  • Penrose R (2002) Gravitational Collapse: The Role of General Relativity. Gen Relativ Gravit 34(7):1141–1165. 1st published: Rivista del Nuovo Cimento, Numero Speziale I, 252 (1969); reprint as “Golden Oldie”. doi:10.1023/A:1016578408204

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  • de Vries A (2000) The apparent shape of a rotating charged black hole, closed photon orbits and the bifurcation set \(A_{4}\). Class Quantum Gravity 17:123–144. doi:10.1088/0264-9381/17/1/309

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Correspondence to Arne Grenzebach .

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Grenzebach, A. (2016). Conclusions. In: The Shadow of Black Holes. SpringerBriefs in Physics. Springer, Cham. https://doi.org/10.1007/978-3-319-30066-5_5

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