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Search for cosmic ultra-high energy neutrinos with ANITA-IV
Completed
Description
The ANITA long-duration balloon payload is designed to search for radio pulses associated with interactions of cosmic ultra-high energy neutrinos in the Antarctic ice sheets. Neutrinos are the only other stable fundamental particles, along with photons, whose directions be traced directly back to their sources without significant deflection or energy loss. By successfully determining the trajectories of observed impulsive radio signals from the ice, ANITA offers the possibility of neutrino astronomy at the highest possible energies. This includes sources such as ultra-high energy cosmic rays which outside the 50-100 MPc range of the local epoch are otherwise expected to be opaque to conventional photometric methods. Detecting at an energy regime not probed by other similar projects, each iteration of the ANITA project provides insights and improved understanding of limitations on the observability of the universe.
Details
| Technology area | Propulsion Systems > Chemical Space Propulsion > Warm Gas |
| Program | Astrophysics (APD) |
| Start date | 2016-09-01 |
| End date | 2017-08-31 |
Project contacts
Listed on TechPort itself — the most direct way to ask about this specific project.
- Peter W Gorham
- Georgette S Sakumoto
- John W Russell
How to get involved
This is a mature technology (TRL 7+) — the realistic path in is usually NASA's Technology Transfer Program: licensing an existing NASA patent, or a Space Act Agreement to use NASA facilities/expertise directly. NASA also runs a startup licensing program with no upfront fee for companies formed to commercialize a specific NASA technology.
None of these are guaranteed paths for this specific project — TechPort itself doesn't have an "apply" button. Reaching out to the contact(s) above with a specific question is usually the fastest way to find out what's actually open.