Gravitinos tunneling from traversable Lorentzian wormholes

I. Sakalli, ALI OVGUN

Research output: Contribution to journalArticlepeer-review

32 Scopus citations

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$3/2$) 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.

Original languageEnglish
Article number32
JournalAstrophysics and Space Science
Volume359
Issue number1
DOIs
StatePublished - 2 Sep 2015

Keywords

  • Gravitino
  • Hawking radiation
  • Lorentzian wormhole
  • Quantum tunneling
  • Spin-3/2 particles

Fingerprint

Dive into the research topics of 'Gravitinos tunneling from traversable Lorentzian wormholes'. Together they form a unique fingerprint.

Cite this