Probing the Temperature Profile of Energy Production in the Sun

Details Probing the Temperature Profile of Energy Production in the Sun Probing the Temperature Profile of Energy Production in the Sun

2006-09-04

arxiv.org/abs/hep-ph/0609030v1

Phys.Rev.Lett.98:141102,2007

Physics

High Energy Physics

High Energy Physics - Phenomenology

Scientific paper

10.1103/PhysRevLett.98.141102

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.

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