Brief communication: Electron pair donors and Earth's energy generation

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 He³ and He⁴ after many years starting from initial densities of the donor pairs. In addition, a new proposal is introduced that connects Cooper pair formations to the deuteron tresino nuclear reaction chain (the chain that determines the He³ / He⁴ ratio). Furthermore, it is proposed that magnetotelluric (MT) observations may be connected to Cooper pair formation either with or without substantial heating.