Year: 2025
Type: article
Abstract: We present direct observational constraints on tachyons, particles with group velocity greater than $c$ 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 $M$ and tachyons of mass $m$ with $g$ degrees of freedom, the black hole lifetime is found to be ${t}_{\mathrm{BH}}\ensuremath{\approx}192\ensuremath{\pi}\ensuremath{\hbar}M/(g{c}^{2}{m}^{2})$ (or doubled for fermions). This implies that the observation of black holes of a few solar masses, with a lifetime of several billion years, rules out tachyons of mass $m\ensuremath{\gtrsim}3\ifmmode\times\else\texttimes\fi{}{10}^{9}\text{ }\text{ }\mathrm{GeV}$. 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.
Institutions: Tufts University, Harvard University
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W4410027181