arXiv:gr-qc/9911055·v1·General Relativity and Quantum Cosmology
Gravitational-Recoil Effects on Fermion Propagation in Space-Time Foam
J. Ellis (CERN)🇨🇭 · N.E. Mavromatos (King's College London)🇬🇧 · D.V. Nanopoulos (Texas A&M, HARC, Academy of Athens)🇺🇸 · G. Volkov (IHEP, Protvino)🇨🇭
Abstract
Motivated by the possible experimental opportunities to test quantum gravity via its effects on high-energy neutrinos propagating through space-time foam, we discuss how to incorporate spin structures in our D-brane description of gravitational recoil effects in vacuo. We also point to an interesting analogous condensed-matter system. We use a suitable supersymmetrization of the Born-Infeld action for excited D-brane gravitational backgrounds to argue that energetic fermions may travel slower than the low-energy velocity of light: \delta c / c \sim -E/M. It has been suggested that Gamma-Ray Bursters may emit pulses of neutrinos at energies approaching 10^{19} eV: these would be observable only if M \gsim 10^{27} GeV.
Comments: 18 pages LaTeX