Using Neutrino Oscillations to Measure ?
arXiv:2206.06115 · doi:10.3390/universe8070377
Abstract
Recently, the idea of using neutrino oscillations to measure the Hubble constant was introduced. We show that such a task is unfeasible because for typical energies of cosmic neutrinos, oscillations average out over cosmological distances and so the oscillation probability depends only on the mixing angles.
arXiv comment4 pages revtex
References in corpus (11)
- A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
- In the Realm of the Hubble tension a Review of Solutions
- Calibration of the Tip of the Red Giant Branch (TRGB)
- The IceCube high-energy starting event sample: Description and flux characterization with 7.5 years of data
- Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Re-determination of the Hubble Constant
- Cosmic Neutrino Pevatrons: A Brand New Pathway to Astronomy, Astrophysics, and Particle Physics
- Coherence Effects in Neutrino Oscillations
- When the Wavepacket is Unnecessary
- Coherence and oscillations of cosmic neutrinos
- Equivalence between Gaussian averaged neutrino oscillations and neutrino decoherence
- Using Neutrino Oscillations to Measure