This research, published in 2017, aimed to solve the solar neutrino and antineutrino flux for extremely low energies (keV range). Processes at these low energies consisted vital information that told researchers about the solar metallicity. Solar metallicity is the measure of elements present in the particle that are heavier than hydrogen and helium, typically in this field this element is usually iron. The results from this research yielded significantly different findings compared to past research in terms of the overall flux spectrum. Currently technology does not yet exist to put these findings to the test.