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Abstract
Dark Matter can interact with electroweak gauge bosons via higher-dimensional operators, in spite of being neutral under gauge interactions, much like neutral atoms interact with photons through Rayleigh scattering. This study explores effective interactions between a real scalar Dark Matter particle, singlet under the SM gauge group, and electroweak gauge bosons. We present a comprehensive analysis of current constraints and projected sensitivities from both lepton and hadron colliders as well as direct and indirect detection experiments in testing Rayleigh Dark Matter interactions. We find that, thanks to the complementarity between collider experiments and cosmological probes, thermally produced Rayleigh Dark Matter at the hundreds of GeV scale can be thoroughly tested with the next generation of experiments. For lighter candidates, upcoming forecasts will explore uncharted parameter space, significantly surpassing the thermal Dark Matter benchmark.
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1 Università di Pisa, Dipartimento di Fisica “Enrico Fermi”, Pisa, Italy (GRID:grid.5395.a) (ISNI:0000 0004 1757 3729); INFN, Sezione di Pisa, Pisa, Italy (GRID:grid.470216.6)
2 INFN, Sezione di Pisa, Pisa, Italy (GRID:grid.470216.6)
3 Università di Pisa, Dipartimento di Fisica “Enrico Fermi”, Pisa, Italy (GRID:grid.5395.a) (ISNI:0000 0004 1757 3729); INFN, Sezione di Pisa, Pisa, Italy (GRID:grid.470216.6); Galileo Galilei Institute for Theoretical Physics, Firenze, Italy (GRID:grid.470185.f)
4 Università degli Studi Roma Tre and INFN, Rome, Italy (GRID:grid.8509.4) (ISNI:0000000121622106)
5 INFN, Laboratori Nazionali di Frascati, Frascati, Italy (GRID:grid.463190.9) (ISNI:0000 0004 0648 0236)