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arXiv · 1203.1729

Hawking tunneling and boomerang behaviour of massive particles with E < m

Gil Jannes·Thomas G. Philbin·Germain Rousseaux
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Abstract

Massive particles are radiated from black holes through the Hawking mechanism together with the more familiar radiation of massless particles. For $E >= m$, the emission rate is identical to the massless case. But $E < m$ particles can also tunnel across the horizon. A study of the dispersion relation and wave packet simulations show that their classical trajectory is similar to that of a boomerang. The tunneling formalism is used to calculate the probability for detecting such $E < m$ particles, for a Schwarzschild black hole of astrophysical size or in an analogue gravity experiment, as a function of the distance from the horizon and the energy of the particle.

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Gil Jannes, Thomas G. Philbin, Germain Rousseaux. 2012-03-08. Hawking tunneling and boomerang behaviour of massive particles with E < m. https://doi.org/10.1063/1.4734453

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