# Can the Cosmic Neutrino Background be detected from a lab moving near the speed of light?

If I've understood it correctly, the energy of an object depends on the reference frame, so when you accelerate, the CMB and CNB appear to gain energy (relative to your rest frame).

So if you are inside a lab that moves at 99.999% of the speed of light, will the CNB (Cosmic Neutrino Background) gain enough energy to be detectable?

• Acronym guessing is no fun...what are CMB and CNB? Commented Apr 20, 2015 at 17:51
• Edited. Cosmic Microwave Background and Cosmic Neutrino Background. Commented Apr 20, 2015 at 18:07
• Often the CNB is abbreviated as C$\nu$B. Commented Apr 20, 2015 at 23:21

The current energies of neutrinos in the cooled cosmic neutrino background are expected to be of order $10^{-4}$ to $10^{-3}$ eV (depending a little bit on what the neutrino masses are) and are almost certainly moving at a small fraction of the speed of light.
Whilst there are experiments under way to try detecting these very low energy neutrinos (for example the Ptolemy experiment), the technology for detecting higher energy neutrinos is much better established. For example the Super Kamiokande detector is sensitive to neutrinos from the Sun with energies around 5-20 MeV. To boost the cosmic background neutrinos up to these kinds of energies would require Lorentz factors of $\gamma = (1 - v^2/c^2)^{-1/2} \simeq 10^{10}$ and thus velocities of $0.999999999999999999995c$. So that's a bit faster than the figure hypothesised in your question.
• Quite possibly. The specific intensity is increased by $((c+v)/(c-v))^3$, which appears to be a factor $>10^{60}$, and the light is shifted to gamma wavelengths, and would appear as an incredibly intense spot of light covering an angle $\sim 10^{-10}$ radians on the sky. Commented Apr 20, 2015 at 22:43