# Mass dimension one fermions and their gravitational interaction

**Authors:** R. J. Bueno Rogerio, R. de C. Lima, L. Duarte, J. M. Hoff da Silva, M., Dias, C. R. Senise Jr

arXiv: 1902.01379 · 2019-12-17

## TL;DR

This paper explores the gravitational interactions of mass dimension one fermions, deriving their vertex, ensuring gauge invariance, and showing they produce an attractive Newtonian potential suitable for dark matter.

## Contribution

It provides a detailed derivation of the fermion-graviton vertex, analyzes one-loop corrections, and demonstrates the potential of these fermions as dark matter candidates.

## Key findings

- Vertex obeys Ward-Takahashi identity, ensuring gauge invariance.
- One-loop corrections can cancel tadpole terms with a cosmological counter-term.
- Non-relativistic limit yields an attractive Newtonian potential.

## Abstract

We investigate in detail the interaction between the spin-${1/2}$ fields endowed with mass dimension one and the graviton. We obtain an interaction vertex that combines the characteristics of scalar-graviton and Dirac's fermion-graviton vertices, due to the scalar-dynamic attribute and the fermionic structure of this field. It is shown that the vertex obtained obeys the Ward-Takahashi identity, ensuring the gauge invariance for this interaction. In the contribution of the mass dimension one fermion to the graviton propagator at one-loop, we found the conditions for the cancellation of the tadpole term by a cosmological counter-term. We calculate the scattering process for arbitrary momentum. For low energies, the result reveals that only the scalar sector present in the vertex contributes to the gravitational potential. Finally, we evaluate the non relativistic limit of the gravitational interaction and obtain an attractive Newtonian potential, as required for a dark matter candidate.

## Full text

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## Figures

5 figures with captions in the complete paper: https://tomesphere.com/paper/1902.01379/full.md

## References

45 references — full list in the complete paper: https://tomesphere.com/paper/1902.01379/full.md

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Source: https://tomesphere.com/paper/1902.01379