# Dark Matter and Exotic Neutrino Interactions in Direct Detection   Searches

**Authors:** Enrico Bertuzzo, Frank F. Deppisch, Suchita Kulkarni, Yuber F. Perez, Gonzalez, Renata Zukanovich Funchal

arXiv: 1701.07443 · 2024-02-06

## TL;DR

This paper explores how new physics involving dark matter and neutrinos could influence direct detection experiments, setting limits on mediator couplings and assessing the impact on dark matter discovery potential.

## Contribution

It introduces a simplified model framework with vector and scalar mediators to analyze their effects on dark matter and neutrino scattering in direct detection experiments.

## Key findings

- Vector mediators can reduce the discovery potential for low-mass dark matter.
- Scalar mediators have negligible impact on detection sensitivity.
- Current data constrains mediator couplings to quarks, neutrinos, and dark matter.

## Abstract

We investigate the effect of new physics interacting with both Dark Matter (DM) and neutrinos at DM direct detection experiments. Working within a simplified model formalism, we consider vector and scalar mediators to determine the scattering of DM as well as the modified scattering of solar neutrinos off nuclei. Using existing data from LUX as well as the expected sensitivity of LUX-ZEPLIN and DARWIN, we set limits on the couplings of the mediators to quarks, neutrinos and DM. Given the current limits, we also assess the true DM discovery potential of direct detection experiments under the presence of exotic neutrino interactions. In the case of a vector mediator, we show that the DM discovery reach of future experiments is affected for DM masses $m_\chi \lesssim 10$ GeV or DM scattering cross sections $\sigma_\chi \lesssim 10^{-47}$ cm$^2$. On the other hand, a scalar mediator will not affect the discovery reach appreciably.

## Full text

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## Figures

7 figures with captions in the complete paper: https://tomesphere.com/paper/1701.07443/full.md

## References

47 references — full list in the complete paper: https://tomesphere.com/paper/1701.07443/full.md

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Source: https://tomesphere.com/paper/1701.07443