2–3 Nov 2024
University of Kansas
US/Central timezone

Navigating the flood of electromagnetic secondary production at SHiP

3 Nov 2024, 10:12
18m
2049 Malott Hall (University of Kansas)

2049 Malott Hall

University of Kansas

Speaker

Tao Zhou (Texas A&M University)

Description

We perform a simulation of dark-vector production from electromagnetic cascades at SHiP. The cascades are initiated by photons from $\pi^0\rightarrow \gamma \gamma$, and lead to substantial increases in sensitivity for long-lived dark vectors with masses below $\sim 50-300~{\rm MeV}$. The dominant production mode in the regions of new sensitivity is $e^+ e^- \rightarrow V(\gamma)$. New sensitivity projections for dark photons and gauged $L_i-L_j$ models are provided for SHiP and compared to previous literature.

Authors

Kevin Kelly (Texas A&M University) Nikita Blinov (Fermi National Accelerator Laboratory) Patrick Fox Pedro Machado (Fermilab) Ryan Plestid Tao Zhou (Texas A&M University)

Presentation materials