LHC lifetime frontier and visible decay searches in composite asymmetric dark matter models.

J High Energy Phys

Center for High Energy Physics, Peking University, Beijing, 100871 China.

Published: March 2022

AI Article Synopsis

  • - The LHC lifetime frontier aims to explore the dark sector, focusing on composite asymmetric dark matter and its interactions through dark photons, which could help resolve the relationship between dark matter and visible matter.
  • - Dark strong dynamics produces rich structures where the lightest dark nucleon acts as dark matter, and strong interactions can lead to its decay into dark pions, while dark photons help mitigate certain cosmological issues.
  • - Experiments like MATHUSLA, FASER, and SeaQuest are expected to effectively search for signatures of dark hadrons and dark pions, with increased sensitivity depending on the kinetic mixing angle of the dark photons, and their results could align with future dark photon investigations.

Article Abstract

The LHC lifetime frontier will probe dark sector in near future, and the visible decay searches at fixed-target experiments have been exploring dark sector. Composite asymmetric dark matter with dark photon portal is a promising framework explaining the coincidence problem between dark matter and visible matter. Dark strong dynamics provides rich structure in the dark sector: the lightest dark nucleon is the dark matter, while strong annihilation into dark pions depletes the symmetric components of the dark matter. Dark photons alleviate cosmological problems. Meanwhile, dark photons make dark hadrons long-lived in terrestrial experiments. Moreover, the dark hadrons are produced through the very same dark photon. In this study, we discuss the visible decay searches for composite asymmetric dark matter models. For a few GeV dark nucleons, the LHC lifetime frontier, MATHUSLA and FASER, has a potential to discover their decay when kinetic mixing angle of dark photon is ≳ 10 . On the other hand, fixed-target experiments, in particular SeaQuest, will have a great sensitivity to dark pions with a mass below GeV and with kinetic mixing ≳ 10 in addition to the LHC lifetime frontier. These projected sensitivities to dark hadrons in dark photon parameter space are comparable with the future sensitivities of dark photon searches, such as Belle-II and LHCb.

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Source
http://www.ncbi.nlm.nih.gov/pmc/articles/PMC8959273PMC
http://dx.doi.org/10.1007/JHEP03(2022)176DOI Listing

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