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Observation of thermal Hawking radiation and its temperature in an analogue black hole

Abstract

The entropy of a black hole1 and Hawking radiation2 should have the same temperature given by the surface gravity, within a numerical factor of the order of unity. In addition, Hawking radiation should have a thermal spectrum, which creates an information paradox3,4. However, the thermality should be limited by greybody factors5, at the very least6. It has been proposed that the physics of Hawking radiation could be verified in an analogue system7, an idea that has been carefully studied and developed theoretically8,9,10,11,12,13,14,15,16,17,18. Classical white-hole analogues have been investigated experimentally19,20,21, and other analogue systems have been presented22,23. The theoretical works and our long-term study of this subject15,24,25,26,27 enabled us to observe spontaneous Hawking radiation in an analogue black hole28. The observed correlation spectrum showed thermality at the lowest and highest energies, but the overall spectrum was not of the thermal form, and no temperature could be ascribed to it. Theoretical studies of our observation made predictions about the thermality and Hawking temperature29,30,31,32,33. Here we construct an analogue black hole with improvements compared with our previous setup, such as reduced magnetic field noise, enhanced mechanical and thermal stability and redesigned optics. We find that the correlation spectrum of Hawking radiation agrees well with a thermal spectrum, and its temperature is given by the surface gravity, confirming the predictions of Hawking’s theory. The Hawking radiation observed is in the regime of linear dispersion, in analogy with a real black hole, and the radiation inside the black hole is composed of negative-energy partner modes only, as predicted.

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Fig. 1: Hawking and partner modes.
Fig. 2: Profile of the analogue black hole.
Fig. 3: Measured Hawking radiation.
Fig. 4: Spectrum of the Hawking radiation.

Data availability

The data that support the plots within this paper and other findings of this study are available from the corresponding author upon reasonable request.

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Acknowledgements

We thank the participants of the LITP Analogue Gravity Workshop for their conversations. We thank I. Carusotto, R. Parentani, D. Marolf and F. Michel for comments. This work was supported by the Israel Science Foundation.

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Authors

Contributions

J.R.M.d.N. and J.S. designed and built the experimental apparatus. J.R.M.d.N., K.G. and V.I.K. performed theoretical calculations. J.S. acquired the data. K.G., V.I.K. and J.S. analysed the data. J.R.M.d.N. performed the numerical simulations. J.R.M.d.N. and J.S. wrote the manuscript with input from all authors.

Corresponding author

Correspondence to Jeff Steinhauer.

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The authors declare no competing interests.

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Muñoz de Nova, J.R., Golubkov, K., Kolobov, V.I. et al. Observation of thermal Hawking radiation and its temperature in an analogue black hole. Nature 569, 688–691 (2019). https://doi.org/10.1038/s41586-019-1241-0

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