2020
DOI: 10.1016/j.physletb.2020.135258
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Dark matter, dark photon and superfluid He-4 from effective field theory

Abstract: We consider a model of sub-GeV dark matter whose interaction with the Standard Model is mediated by a new vector boson (the dark photon) which couples kinetically to the photon. We describe the possibility of constraining such a model using a superfluid He-4 detector, by means of an effective theory for the description of the superfluid phonon. We find that such a detector could provide bounds that are competitive with other direct detection experiments only for ultralight vector mediator, in agreement with pr… Show more

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Cited by 28 publications
(14 citation statements)
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“…In this case the dark matter can still deposit energy by producing one or more athermal phonons in the target. Such processes have been studied extensively in both superfluid He [35][36][37][38][39][40] and solid state targets [13,14,[41][42][43][44][45][46][47]. Given the existing constraints on models of sub-MeV dark matter, DM scattering through a dark photon mediator and dark photon DM absorption appear to be the most promising processes [48].…”
mentioning
confidence: 99%
“…In this case the dark matter can still deposit energy by producing one or more athermal phonons in the target. Such processes have been studied extensively in both superfluid He [35][36][37][38][39][40] and solid state targets [13,14,[41][42][43][44][45][46][47]. Given the existing constraints on models of sub-MeV dark matter, DM scattering through a dark photon mediator and dark photon DM absorption appear to be the most promising processes [48].…”
mentioning
confidence: 99%
“…3. Write down an effective field theory (EFT) based on the spontaneous breaking of particle number symmetry, interpreting the acoustic phonon as a Goldstone mode and using measurements to fix the unknown coefficients in the effective action [83,[111][112][113]. This approach can be used for single and multi-excitation rates, but is limited to treating only the acoustic phonons in the excitation spectrum.…”
Section: Superfluid Heliummentioning
confidence: 99%
“…Owing to the continuous developments in detector technologies in recent years, the frontier of the dark matter direct detection has been pushed to the mass range below the GeV scale, where the traditional detection methods based on the nuclear scattering are expected to lose sensitivity. So more and more theorists and experimentalists have begun to shift to other alternative proposals based on new detection channels and materials, such as with semiconductors [1][2][3][4], Dirac materials [5][6][7], superconductors [8,9], superfluid helium [10][11][12], and via phonon excitations [13][14][15] and bremsstrahlung photons [16][17][18], as well as other proposals and analyses .…”
Section: Introductionmentioning
confidence: 99%