Welcome to the new version of CaltechAUTHORS. Login is currently restricted to library staff. If you notice any issues, please email coda@library.caltech.edu
Published April 15, 2016 | Submitted + Published
Journal Article Open

Probing the Dark Sector with Dark Matter Bound States

Abstract

A model of dark sector where O(few GeV) mass dark matter particles χ are supplied by a lighter dark force mediator V, m_V ≪ m_χ, is motivated by the recently discovered mismatch between simulated and observed shapes of galactic haloes. Such models, in general, provide a challenge for direct detection efforts and collider searches. We show that for a large range of coupling constants and masses, the production and decay of the bound states of χ, such as 0^(−+) and 1^(−−) states, η_D and Υ_D, is an important search channel. We show that e+e− → η_D + V or Υ_D + γ production at B-factories for α_D > 0.1 is sufficiently strong to result in multiple pairs of charged leptons and pions via η_D → 2V → 2(l^+l^−) and Υ_D → 3V → 3(l+l−) (l = e, µ, π). The absence of such final states in the existing searches performed at BABAR and Belle sets new constraints on the parameter space of the model. We also show that a search for multiple bremsstrahlung of dark force mediators, e^+e^− → χχ¯ + nV , resulting in missing energy and multiple leptons, will further improve the sensitivity to self-interacting dark matter.

Additional Information

© 2016 American Physical Society. Received 29 October 2015; revised manuscript received 9 February 2016; published 11 April 2016. We would like to thank Clifford Cheung, Ying Fan, Ming Liu, Mark Wise, and Hai-bo Yu for useful discussions. H. A. is supported by the Walter Burke Institute at Caltech and by DOE Grant No. de-sc0011632. B. E. is supported by the U.S. Department of Energy (DOE) under Grants No. DE-FG02-92ER40701 and No. DE-SC0011925. The work of M. P. is supported in part by NSERC, Canada, and research at the Perimeter Institute is supported in part by the Government of Canada through NSERC and by the Province of Ontario through MEDT. Y. Z. is supported by the Gordon and Betty Moore Foundation through Grant No. 776 to the Caltech Moore Center for Theoretical Cosmology and Physics, and by the DOE Grant No. DE-FG02-92ER40701, and also by a DOE Early Career Award under Grant No. DE-SC0010255. H. A., M. P., and Y. Z. acknowledge the hospitality from the Aspen Center for Physics and the support from NSF Grant No. PHY-1066293.

Attached Files

Published - PhysRevLett.116.151801.pdf

Submitted - 1510.05020v1.pdf

Files

PhysRevLett.116.151801.pdf
Files (1.2 MB)
Name Size Download all
md5:15676d615cc8ae803b2b656d536a701c
439.4 kB Preview Download
md5:a7a5f491a9c2c7b38d1382f3dbee11dd
746.6 kB Preview Download

Additional details

Created:
August 20, 2023
Modified:
October 25, 2023