English

Black Holes Rule Out Heavy Tachyons

General Relativity and Quantum Cosmology 2025-05-05 v2 Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology High Energy Physics - Theory

Abstract

We present direct observational constraints on tachyons; particles with group velocity greater than cc in vacuum in a Lorentz invariant theory. Since tachyons may have no direct couplings to Standard Model particles, the most robust and model independent constraints come from gravitational effects, especially black holes. We compute the Hawking radiation of tachyons from black holes, finding it to be significantly enhanced in the presence of heavy tachyons. For a black hole of mass MM and tachyons of mass mm with gg degrees of freedom, the black hole lifetime is found to be tbh192πM/(gc2m2)t_{bh} \approx 192 \pi \hbar M/(g c^2 m^2) (or doubled for fermions). This implies that the observation of black holes of a few solar masses, with lifetime of several billion years, rules out tachyons of mass m>3×109m > 3 \times 10^9 GeV. This means there cannot exist any tachyons associated with unification scales or quantum gravity. So while there already exists theoretical reasons to be skeptical of tachyons, our work provides a complementary direct observational constraint.

Keywords

Cite

@article{arxiv.2501.11606,
  title  = {Black Holes Rule Out Heavy Tachyons},
  author = {Mark P. Hertzberg and Abraham Loeb and Aidan Morehouse},
  journal= {arXiv preprint arXiv:2501.11606},
  year   = {2025}
}

Comments

7 pages in double column format, 2 figures. Accepted for publication in Phys. Rev. D