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Published on: November 15, 2013
Pair creation constrains superluminal neutrino propagation
Andrew G Cohen1, Sheldon L Glashow
1Physics Department, Boston University, Boston, Massachusetts 02215, USA. cohen@bu.edu
Physical Review Letters
|November 24, 2011
Summary
Superluminal neutrinos may rapidly lose energy through pair production, challenging OPERA
Area of Science:
- Particle Physics
- Neutrino Physics
- Astroparticle Physics
Background:
- The OPERA collaboration reported evidence of muon neutrinos traveling faster than light.
- This finding, if true, would challenge fundamental principles of physics.
Purpose of the Study:
- To investigate the physical consequences of superluminal neutrino propagation.
- To assess the viability of the OPERA collaboration's claim.
Main Methods:
- Theoretical analysis of energy loss mechanisms for superluminal neutrinos.
- Calculation of neutrino energy spectrum depletion due to pair production.
- Re-analysis of existing experimental data from Super-Kamiokande and IceCube.
Main Results:
- Superluminal neutrinos at the claimed energy and velocity would rapidly lose energy via electron-positron pair bremsstrahlung.
- This energy loss mechanism would significantly deplete the neutrino beam of higher-energy particles.
- Existing data from Super-Kamiokande and IceCube place stringent limits on superluminal neutrino propagation.
Conclusions:
- The OPERA collaboration's claim of superluminal neutrinos faces significant theoretical challenges.
- The proposed energy loss mechanism provides a plausible explanation for potential discrepancies.
- New experimental constraints strongly disfavor superluminal neutrino propagation.
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