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Exotic spin-dependent interactions mediated by new light particles led tosolutions to several important questions in modern physics. Such interactionsinvolving a scalar coupling $g_S^N$ at one vertex and a pseudo-scalar coupling$g_P^n$ at the polarized neutron vertex can be induced by the exchange ofspin-0 bosons, or a vector/axial-vector coupling $g_V^N$/$g_A^N$ at one vertexand an axial-vector coupling $g_A^n$ at the polarized neutron vertex can beinduced by the exchange of spin-1 bosons. If such new interactions exist, theSun and the Moon can induce sidereal variations of effective fields along thedirection perpendicular to the Earth's rotation axis. We derived newexperimental upper limits on such exotic spin-dependent interactions atastronomical interaction ranges by analyzing existing data from laboratorymeasurements on the Lorentz and CPT violation. We set the most stringentexperimental limits on $g_S^Ng_P^n$ ranging from $\sim 2\times 10^{10}$m to$\sim 10^{14}$m. Previously, the best limit on $g_S^Ng_P^n$ at this range isfrom astrophysics. The result is the first time laboratory limits surpass theastrophysical ones on the scalar-pseudoscalar type interaction, to our bestknowledge. We report new constraints on vector-axial-vector andaxial-axial-vector type interaction at the range of astronomical scales. Thenew limits on vector-axial-vector are improved by as much as $\sim$12 orders ofmagnitude. We also apply the analysis to the Hari-Dass interactions and obtaincorresponding new constraints on the interactions. We discuss the possibilitiesof using the beam method to further search the interaction involving otherparticles, such as electrons, muons, etc., based on the same idea.

Using the Sun and the Moon as Source masses and the Earth's Rotation as  a Modulation to Search for Exotic Spin-Dependent Interactions at Astronomical  Distances