Journal
EUROPEAN PHYSICAL JOURNAL PLUS
Volume 130, Issue 6, Pages 1-4Publisher
SPRINGER HEIDELBERG
DOI: 10.1140/epjp/i2015-15110-9
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In this article, we consider the Hawking radiation (HR) of vector (massive spin-1) particles from the traversable Lorentzian wormholes (TLWH) in 3+1 dimensions. We start by providing the Proca equations for the TLWH. Using the Hamilton-Jacobi (HJ) ansatz with the WKB approximation in the quantum tunneling method, we obtain the probabilities of the emission/absorption modes. Then, we derive the tunneling rate of the emitted vector particles and manage to read the standard Hawking temperature of the TLWH. The result obtained represents a negative temperature, which is also discussed.
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