Greybody factor of scalar fields from black strings
arXiv:1712.07574 · doi:10.1140/epjc/s10052-017-5449-6
Abstract
The greybody factor of massless, uncharged scalar fields is studied in the background of cylindrically symmetric spacetimes, in the low-energy approximation. We discuss two cases. In the first case we derive analytical expression for the absorption probability when the spacetime is kinetically coupled with the Einstein tensor. In the second case we do the analysis in the absence of the coupling constant. For this purpose we analyze the wave equation which is obtained from Klein-Gordon equation. The radial part of the wave equation is solved in the form of the hypergeometric function in the near horizon region, whereas in the far region the solution is of the form of Bessel's function. Finally, considering continuity of the wave function we smoothly match the two solutions in the low energy approximation to get the formula for the absorption probability.
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- Greybody Factors of Holographic Superconductors with Lifshitz Scaling
- Quantum fields in the background spacetime of a loop quantum gravity black hole
- Rotating black string in dRGT massive gravity
- Absorption Cross-Section and Decay Rate of Dilatonic Black Strings
- Greybody Factor for a Rotating Bardeen Black Hole by Perfect Fluid Dark Matter
- Thermodynamics of Black String from Rényi entropy in de Rham-Gabadadze-Tolley Massive Gravity Theory