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Quasi-normal modes and absorption probabilities of spin-3/2 fields in $D$-dimensional Reissner-Nordstr\'om black hole spacetimes

Autor: Chen, C. -H., Cho, H. T., Cornell, A. S., Harmsen, G., Ngcobo, X.

Publikováno v: Phys. Rev. D 97, 024038 (2018)

In this paper we consider spin-3/2 fields in a $D$-dimensional Reissner-Nordstr\"om black hole spacetime. As these spacetimes are not Ricci-flat, it is necessary to modify the covariant derivative to the supercovariant derivative, by including terms

Externí odkaz: http://arxiv.org/abs/1710.08024

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Spin-3/2 fields in $D$-dimensional Schwarzschild black hole space-times

Autor: Chen, C. -H., Cho, H. T., Cornell, A. S., Harmsen, G.

Publikováno v: Phys. Rev. D 94, 044052 (2016)

In previous works we have studied spin-3/2 fields near 4-dimensional Schwarzschild black holes. The techniques we developed in that case have now been extended here to show that it is possible to determine the potential of spin-3/2 fields near $D$-di

Externí odkaz: http://arxiv.org/abs/1605.05263

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Absorption probabilities associated with spin-3/2 particles near $N$-dimensional Schwarzschild black holes

Autor: Harmsen, G. E., Chen, C. H., Cho, H. T., Cornell, A. S.

In June 2015 the Large Hadron Collider was able to produce collisions with an energy of 13TeV, where collisions at these energy levels may allow for the formation of higher dimensional black holes. In order to detect these higher dimensional black ho

Externí odkaz: http://arxiv.org/abs/1602.07434

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Gravitino fields in Schwarzschild black hole spacetimes

Autor: Chen, C. -H., Cho, H. T., Cornell, A. S., Harmsen, G., Naylor, Wade

The analysis of gravitino fields in curved spacetimes is usually carried out using the Newman-Penrose formalism. In this paper we consider a more direct approach with eigenspinor-vectors on spheres, to separate out the angular parts of the fields in

Externí odkaz: http://arxiv.org/abs/1504.02579

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