Hawking radiation as tunnelling from the trapping horizon of a general non-static spherically symmetric space-time
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🌀 gr-qc
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hawkinghorizontunnellinggeneralnon-staticradiationsphericallysymmetric
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Using tunnelling approach, Hawking radiation is derived for a general class of non-static spherically symmetric space time. The standard tunnelling rate formula is obtained using the unified first law of thermodynamics on the trapping horizon and Hawking temperature is measured by an Kodama observer inside the horizon.
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