Abstract
Recent research shows that Hawking radiation (HR) is also possible around the trapping horizon of a wormhole. In this article, we show that the HR of gravitino (spin-\(3/2\)) particles from the traversable Lorentzian wormholes (TLWH) reveals a negative Hawking temperature (HT). We first introduce the TLWH in the past outer trapping horizon geometry (POTHG). Next, we derive the Rarita-Schwinger equations (RSEs) for that geometry. Then, using both the Hamilton-Jacobi (HJ) ansätz and the WKB approximation in the quantum tunneling method, we obtain the probabilities of the emission/absorption modes. Finally, we derive the tunneling rate of the emitted gravitino particles, and succeed to read the HT of the TLWH.
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Sakalli, I., Ovgun, A. Gravitinos tunneling from traversable Lorentzian wormholes. Astrophys Space Sci 359, 32 (2015). https://doi.org/10.1007/s10509-015-2482-5
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DOI: https://doi.org/10.1007/s10509-015-2482-5