Grieb Christian, Raghavan R S
Institute of Particle, Nuclear and Astronomical Sciences and Department of Physics, Virginia Polytechnic Institute and State University, Blacksburg Virginia 24061, USA.
Phys Rev Lett. 2007 Apr 6;98(14):141102. doi: 10.1103/PhysRevLett.98.141102. Epub 2007 Apr 2.
The particle kinetic energies of thermonuclear 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. This effect may be observable via the unique tools of the LENS solar neutrino detector. The temperature profile of energy production in the Sun may thus be directly probed for the first time.
太阳中热核质子-质子聚变的粒子动能（伽莫夫能量）相对于仅由放热能量学产生的情况，会使质子-质子太阳中微子的能量产生微小变化。通过LENS太阳中微子探测器这一独特工具，这种效应可能是可观测的。因此，太阳能量产生的温度剖面可能首次得到直接探测。
