Gravitational Cherenkov losses in MOND theories

TL;DR

This paper shows that high-energy cosmic rays do not impose strong constraints on MOND theories compatible with general relativity, due to the significantly reduced gravitational Cherenkov losses when considering the correct cutoff scale.

Contribution

It demonstrates that gravitational Cherenkov losses are much smaller than previously thought in MOND theories that match GR at high accelerations, relaxing constraints on such theories.

Findings

Cherenkov losses are many orders smaller than earlier estimates.

The relevant cutoff scale is the MOND radius, not the de Broglie wavelength.

Survival of high-energy cosmic rays does not strongly constrain GR-compatible MOND theories.

Abstract

Survival of high-energy cosmic rays (HECRs) against gravitational Cherenkov losses is shown not to cast strong constraints on MOND theories that are compatible with general relativity (GR): theories that coincide with GR in the high-acceleration limit. The energy-loss rate, L, is shown to be many orders smaller than those derived in the literature for theories with no extra scale. The gravitational acceleration produced by a HECR in its vicinity is much higher than the MOND acceleration a0. So, modification to GR, which underlies L, enters only beyond the MOND radius of the particle, within which GR holds sway: r_M=sqrt(Gp/c a0). The spectral cutoff, which enters L quadratically, is thus 1/r_M, not the particle's, much larger, de Broglie wavenumber: k_{dB}= p/hbar. Thus, L is smaller than published rates, which use k_{dB}, by a factor (r_M k_{dB})^2~10^{39}(cp/3.10^{11}Gev)^3. With 1/r_M as cutoff, the distance a HECR can travel without major losses is q l_M, where l_M=c^2/a0 is the MOND length, and q is a dimensionless function of parameters of the problem. Since l_M is ~2 pi times the Hubble distance, survival of HECRs does not strongly constrain GR-compatible, MOND theories. Such theories also easily satisfy existing preferred-frame limits, inasmuch as these limits are gotten in high-acceleration systems. I exemplify the results with MOND adaptations of Einstein-Aether theories.