Abstract. This Brief Communication presents a series of model calculations for the electron pair donor densities required for tresino thermal energy generation in the Earth. The crucial density of electron donors is determined from the ratio of He This Brief Communication describes a new proposal relating to tresino formation-hence to thermal energy generation (Mayer and Reitz, 2014) in the Earth; it represents an extension of our prior work on the thermal energy generation in the Earth. In our NPG paper, we made an assumption regarding the collisions that gave rise to the transfer of a pair of electrons required to form 10 a tresino, hence energy generation. The assumption was that the electron pairs were delivered in a collision between a proton Figure 1) to form either a proton tresino or a deuteron tresino. The ensuing reaction dynamics and energy generation then follows the same reaction chains as those of our earlier paper (Mayer and Reitz, 2014). Unfortunately, the microphysics of the formation of the Cooper pairs is itself complex because of the physical processes, the materials, and the spatial length scales may all be diverse even in laboratory experiments, which by the way, are generally done at low temperatures, as described in the overview paper of (Hirsh, Maple and Marsiglio , 2015).
20Cooper pairs have been recently been proposed in Feigel'man andIoffe (2015) and S. Dolgopolov (2015) in somewhat mixed materials, including at interfaces, see e.g. [Gariglio, et.al. (2015)]. So considering "superfluids" of Cooper pairs created in Earth materials, perhaps under pressure, seems a reasonable assumption in the Earth. Of course, assessing the materials most operative in the Earth will have to be determined. Interestingly, the "superfluid" has only to be a (local) transient process but 1 Nonlin. Processes Geophys. Discuss., https://doi