Abstract
We investigate the features of the non-corrected thermal (non-thermal) spectrum and the quantum corrected thermal (non-thermal) spectrum. We find that: (1) using the quantum corrected non-thermal spectra, the black hole radiation as tunneling is an entropy conservation process, and thus black hole evaporation process is unitary; (2) there are no obvious differences between all spectra except for near the Planck mass scale by comparing their average emission energies, average numbers of emissions and average emission energy fluctuations; (3) the energy covariances of Hawking radiations for all the thermal spectra are exactly zero, while they are nontrivial for all the non-thermal spectra. Especially, there are distinctly different maximums of energy covariances for the temperature-corrected and energy-corrected non-thermal spectra. Consequently, these differences provide a possible way towards experimentally analyzing whether the radiation spectrum of black hole is thermal or non-thermal with or without high order quantum corrections.
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Notes
For \(D\) dimensional Schwarzschild black hole, the fundamental Planck scale is reduced depending on the compact space of volume \(V_{D-4}\), e.g., the reduced Planck scale \(M_P\sim 1\,\mathrm {TeV}\) with \(D=10\) and \(V_6\sim fm^6\) [40].
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Acknowledgments
This work was supported by the National Natural Science Foundation of China under Grant Nos. 11175065, 10935013; the National Basic Research of China under Grant No. 2010CB833004; the Hunan Provincial Natural Science Foundation of China under Grant No. 11JJ7001; Hunan Provincial Innovation Foundation For Postgraduate under Grant No. CX2012B202; the Construct Program of the National Key Discipline
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Tian, Z., Jing, J. Towards experimentally studying some puzzles of Hawking radiation. Gen Relativ Gravit 46, 1779 (2014). https://doi.org/10.1007/s10714-014-1779-y
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DOI: https://doi.org/10.1007/s10714-014-1779-y