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- W2904312028 abstract "This paper is devoted to study charged fermion particles tunneling through the horizon of Kerr-Newman-AdS black hole surrounded by quintessence by using Hamilton-Jacobi ansatz. In our analysis, we investigate Hawking temperature as well as quantum corrected Hawking temperature on account of generalized uncertainty principle. Moreover, we discuss the effects of correction parameter <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M1><mml:mrow><mml:mi>β</mml:mi></mml:mrow></mml:math> on the corrected Hawking temperature <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M2><mml:mrow><mml:msub><mml:mrow><mml:mi>T</mml:mi></mml:mrow><mml:mrow><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mi>H</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math>, graphically. We conclude that the temperature <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M3><mml:mrow><mml:msub><mml:mrow><mml:mi>T</mml:mi></mml:mrow><mml:mrow><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mi>H</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math> vanishes when <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M4><mml:mi>β</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant=normal>100</mml:mn></mml:math>, whereas for <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M5><mml:mi>β</mml:mi><mml:mo><</mml:mo><mml:mn mathvariant=normal>100</mml:mn></mml:math> and <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M6><mml:mi>β</mml:mi><mml:mo>></mml:mo><mml:mn mathvariant=normal>100</mml:mn></mml:math>, the temperature turns out to be positive and negative, respectively. We observe that the graphs of <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M7><mml:mrow><mml:msub><mml:mrow><mml:mi>T</mml:mi></mml:mrow><mml:mrow><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mi>H</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math> w.r.t. quintessence parameter <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M8><mml:mrow><mml:mi>α</mml:mi></mml:mrow></mml:math> exhibit behavior only for the particular ranges, i.e., <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M9><mml:mn mathvariant=normal>0</mml:mn><mml:mo><</mml:mo><mml:mi>α</mml:mi><mml:mo><</mml:mo><mml:mn mathvariant=normal>1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant=normal>6</mml:mn></mml:math>, charge <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M10><mml:mn mathvariant=normal>0</mml:mn><mml:mo><</mml:mo><mml:mi>Q</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant=normal>1</mml:mn></mml:math>, and rotation parameter <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M11><mml:mn mathvariant=normal>0</mml:mn><mml:mo><</mml:mo><mml:mi>a</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant=normal>1</mml:mn></mml:math>. For smaller and larger values of negative <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M12><mml:mrow><mml:mi mathvariant=normal>Λ</mml:mi></mml:mrow></mml:math>, as horizon increases, the temperature decreases and increases, respectively." @default.
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- W2904312028 date "2019-01-14" @default.
- W2904312028 modified "2023-10-02" @default.
- W2904312028 title "Fermions Tunneling and Quantum Corrections for Quintessential Kerr-Newman-AdS Black Hole" @default.
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