Abstract
We report a search for exotic spin-spin interactions between neutrons and electrons which could signal new physics beyond the standard model using slow neutron polarimetric imaging through a dense medium of polarized electrons. Our dense polarized electron target is a ferrimagnet held at its magnetic compensation temperature, which realizes a polarized electron ensemble with zero net magnetization. We sought the spin rotation of transversely polarized neutrons from a neutron-spin–electron-spin interaction of the form V2=-gAegAn(ℏc/4π)σ→e·σ→n(e-r/λc/r), where gAe and gAn are the electron and neutron axial couplings, σe→ and σn→ are the electron and neutron spin, and λc is the interaction range for an exotic axial vector interaction from massive spin-1 boson exchange of mass ℏc/λc. The resulting average neutron-spin-rotation angle per unit length, (dϕ¯F5/dz)=[0.41±6.3(stat)±4.4(sys)]×10-3 rad/m, is consistent with zero. Our novel approach improves the previous upper limits on the coupling constant product gAegAn by several orders of magnitude in the poorly explored 10-8≤λc≤10-2 m range.
| Original language | English |
|---|---|
| Article number | 071801 |
| Journal | Physical Review Letters |
| Volume | 136 |
| Issue number | 7 |
| DOIs | |
| State | Published - Feb 20 2026 |
Funding
M. S. and T. M. acknowledge support from U.S. Department of Energy Grant No. DE-SC0010443. This research was supported in part by an appointment to the Oak Ridge National Laboratory GRO Program, sponsored by the U.S. Department of Energy and administered by the Oak Ridge Institute for Science and Education. K. N. L., M. L., M. V. M., and W. M. S. acknowledge support from US National Science Foundation (NSF) Grants No. PHY-1913789 and No. PHY-2209481 and the Indiana University Center for Spacetime Symmetries. K. N. L. also acknowledges the support of the GEM Consortium and Indiana Space Grant Consortium. J. C. L. and B. H. acknowledge support from grant NSF PHY-1707986. The authors acknowledge the use of facilities supported by NSF through the University of Illinois Materials Research Science and Engineering Center DMR-2309037. This research used resources at the High Flux Isotope Reactor, a DOE Office of Science User Facility operated by the Oak Ridge National Laboratory. The beam time was allocated to MARS on proposals No. IPTS-30635 and No. IPTS-32059. This work was supported by the U.S. Department of Energy (DOE), Office of Science, Office of Basic Energy Sciences, Early Career Research Program Award No. KC0402010, under Contract No. DE-AC05-00OR22725. We thank H.-O. Meyer for suggesting measurements on TbIG.
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