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2018•AIP conference proceedingsRequires access

Fermions emission of linear dilaton black hole

Seyedeh Fatemeh Mirekhtiary, Akbar Abbasi

Open publisher page 2 citations

Abstract

We apply tunnelling method to the general class of static, spherically symmetric space time for the geometry of LDBH, we extend the Dirac equation and WKB approximation to read the tunnelling probability of fermions emission for incoming and outgoing particles from event horizon of LDBH and exhibit that the hawking temperature is truly recovered. (we eliminated any change in the angular momentum of the black hole due to the spin of the emitted particle)

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What this paper is about

We apply tunnelling method to the general class of static, spherically symmetric space time for the geometry of LDBH, we extend the Dirac equation and WKB approximation to read the tunnelling probability of fermions emission for incoming and outgoing particles from event horizon of LDBH and exhibit that the hawking temperature is truly recovered. (we eliminated any change in the angular momentum of the black hole due to the spin of the emitted particle)

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Available abstract

We apply tunnelling method to the general class of static, spherically symmetric space time for the geometry of LDBH, we extend the Dirac equation and WKB approximation to read the tunnelling probability of fermions emission for incoming and outgoing particles from event horizon of LDBH and exhibit that the hawking temperature is truly recovered. (we eliminated any change in the angular momentum of the black hole due to the spin of the emitted particle)

Key concepts: WKB approximation, Physics, Event horizon, Quantum tunnelling, Fermion, Dilaton, Black hole (networking), Angular momentum

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