Probing the Temperature Profile of Energy Production in the Sun
classification
✦ hep-ph
astro-ph
keywords
energyenergiesproductionprofilesolartemperaturechangesdetector
read the original abstract
The particle kinetic energies of pp fusion in the sun (Gamow Energy) produce small changes in the energies of pp solar neutrinos relative to those due only to exothermal energetics. Observation of this effect may be possible via the unique tools of the upcoming LENS solar neutrino detector. The temperature profile of energy production in the sun may thus be directly probed for the first time.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.