English

Horizon wave-function for single localized particles: GUP and quantum black hole decay

General Relativity and Quantum Cosmology 2015-06-16 v2 High Energy Physics - Theory Quantum Physics

Abstract

A localised particle in Quantum Mechanics is described by a wave packet in position space, regardless of its energy. However, from the point of view of General Relativity, if the particle's energy density exceeds a certain threshold, it should be a black hole. In order to combine these two pictures, we introduce a horizon wave-function determined by the particle wave-function in position space, which eventually yields the probability that the particle is a black hole. The existence of a minimum mass for black holes naturally follows, albeit not in the form of a sharp value around the Planck scale, but rather like a vanishing probability that a particle much lighter than the Planck mass be a black hole. We also show that our construction entails an effective Generalised Uncertainty Principle (GUP), simply obtained by adding the uncertainties coming from the two wave-functions associated to a particle. Finally, the decay of microscopic (quantum) black holes is also described in agreement with what the GUP predicts.

Keywords

Cite

@article{arxiv.1306.5298,
  title  = {Horizon wave-function for single localized particles: GUP and quantum black hole decay},
  author = {R. Casadio and F. Scardigli},
  journal= {arXiv preprint arXiv:1306.5298},
  year   = {2015}
}

Comments

8 pages, 5 figures, extended version of arXiv:1305.3195 with new results about the GUP and black hole decay, clarifications about black hole decay added

R2 v1 2026-06-22T00:38:30.196Z