Skip to main content
. Author manuscript; available in PMC: 2017 Nov 22.
Published in final edited form as: Phys Rev C. 2016 Apr 21;93(4):044614. doi: 10.1103/PhysRevC.93.044614

FIG. 11.

FIG. 11

Xe-Q can be modeled as fractionated by 6.5‰ /u solar Xe [48] with ~3% addition of 136Xe, ~1.5% of 134Xe, and <0.5% of 132Xe and 131Xe (top). The isotopic structure of the required for this model addition matches the pattern of Xe found in the gas bubbles released from the Hanford site [35] (bottom). This model does not require any presolar Xe components.