期刊
ASTROPHYSICS AND SPACE SCIENCE
卷 359, 期 1, 页码 -出版社
SPRINGER
DOI: 10.1007/s10509-015-2482-5
关键词
Hawking radiation; Gravitino; Quantum tunneling; Lorentzian wormhole; Spin-3/2 particles
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) ansatz 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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