Dark Matter, Baryon Asymmetry, and Spontaneous B and L Breaking
Timothy R. Dulaney (1), Pavel Fileviez Perez (2), Mark B. Wise (1), ((1) Caltech, (2) Wisconsin U., Madison)

TL;DR
This paper explores a model where baryon and lepton numbers are local gauge symmetries that are spontaneously broken, addressing dark matter stability and baryon asymmetry with specific predictions for dark matter interactions.
Contribution
It introduces a simple gauge theory model with spontaneously broken baryon and lepton numbers that explains dark matter stability and baryon asymmetry, with testable predictions.
Findings
Dark matter candidate is the lightest baryon-number-carrying field.
Dark matter annihilation can occur via a leptophobic gauge boson or the Higgs.
Predicted lower bound on dark matter-nucleon elastic cross section is about 5x10^{-46} cm^2.
Abstract
We investigate the dark matter and the cosmological baryon asymmetry in a simple theory where baryon (B) and lepton (L) number are local gauge symmetries that are spontaneously broken. In this model, the cold dark matter candidate is the lightest new field with baryon number and its stability is an automatic consequence of the gauge symmetry. Dark matter annihilation is either through a leptophobic gauge boson whose mass must be below a TeV or through the Higgs boson. Since the mass of the leptophobic gauge boson has to be below the TeV scale one finds that in the first scenario there is a lower bound on the elastic cross section of about 5x10^{-46} cm^2. Even though baryon number is gauged and not spontaneously broken until the weak scale, a cosmologically acceptable baryon excess is possible. There is tension between achieving both the measured baryon excess and the dark matter…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
