We have measured the ratio of nuclear spin-precession frequencies of ¹⁹⁹Hg and ²⁰¹Hg atoms for two orientations of magnetic field relative to the Earth's gravitational field. We find that the spin-dependent component of gravitational energy is less than 2.2×{}10^-21 eV, a substantial improvement over previous limits. Our result provides a test of the equivalence principle for nuclear spins, and sets limits on the magnitude of possible scalar-pseudoscalar interactions which would couple to the spins.
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Venema et al. (1992) studied this question.
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