Spherically symmetric Earth models yield no net electron spin
Nathan B. Clayburn, Andrew Glassford, Andrew Leiker, Thomas Uelmen,, Jung-Fu Lin, and Larry R. Hunter

TL;DR
This paper demonstrates that Earth's spherically symmetric models lead to a net zero electron spin, impacting constraints on exotic spin-dependent interactions and dark matter coupling bounds.
Contribution
It shows that Earth's overall electron spin cancels out in spherical models, revising previous bounds on monopole-dipole couplings derived from perihelion precession data.
Findings
Net electron spin in Earth is effectively zero in spherical models.
At least 5 x 10^38 spin-polarized electrons are aligned anti-parallel to Earth's rotation axis.
Constraints on exotic couplings need to be relaxed by a factor of about 2000.
Abstract
Terrestrial experiments that use electrons in Earth as a spin-polarized source have been demonstrated to provide strong bounds on exotic long-range spin-spin and spin-velocity interactions. These bounds constrain the coupling strength of many proposed ultralight bosonic dark-matter candidates. Recently, it was pointed out that a monopole-dipole coupling between the Sun and the spin-polarized electrons of Earth would result in a modification of the precession of the perihelion of Earth. Using an estimate for the net spin-polarization of Earth and experimental bounds on Earth's perihelion precession, interesting constraints were placed on the magnitude of this monopole-dipole coupling. Here we investigate the spin associated with Earth's electrons. We find that there are about spin-polarized electrons in the mantle and crust of Earth oriented anti-parallel to their…
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Taxonomy
TopicsGeophysics and Gravity Measurements · Geomagnetism and Paleomagnetism Studies · Geophysical and Geoelectrical Methods
