• Open Access

WIMPs at high energy muon colliders

Tao Han, Zhen Liu, Lian-Tao Wang, and Xing Wang
Phys. Rev. D 103, 075004 – Published 6 April 2021

Abstract

The weakly interacting massive particle (WIMP) paradigm is one of the most compelling scenarios for particle dark matter (DM). We show in this paper that a high energy muon collider can make decisive statements about the WIMP DM, and this should serve as one of its main physics driver cases. We demonstrate this by employing the DM as the lightest member of an electroweak (EW) multiplet, which is a simple, yet one of the most challenging WIMP scenarios given its minimal collider signature and high thermal target mass scale of 1–23 TeV. We perform a first study of the reach of high energy muon colliders, focusing on the simple, inclusive, and conservative signals with large missing mass, through the mono-photon, vector boson fusion di-muon and a novel mono-muon channel. Using these inclusive signals, it is possible to cover the thermal targets of doublet and triplet with a 10 TeV muon collider. Higher energies, 14 TeV–75 TeV, would ensure a 5σ reach above the thermal targets for the higher EW multiplets. We also estimate the reach of a search for disappearing tracks, demonstrating the potential significant enhancement of the sensitivity.

  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
11 More
  • Received 20 November 2020
  • Accepted 24 February 2021
  • Corrected 3 September 2021

DOI:https://doi.org/10.1103/PhysRevD.103.075004

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Corrections

3 September 2021

Correction: The entry in Table I, second row, last column, contained an error and has been fixed. The previously published Figs. 13, 14, 15, and 16 contained errors (cyan curve, dashed curve, bottom two thin bars, and bottom thin bar, respectively) and have been replaced. Equations (3.21) and (3.22) contained errors and have been fixed. The last sentence of the second-to-last paragraph of text contained errors and has been remedied. The last four entries for doublets for each energy in the Appendix table were erroneous and have been fixed.

Authors & Affiliations

Tao Han1, Zhen Liu2, Lian-Tao Wang3, and Xing Wang4

  • 1PITT PACC, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania 15217, USA
  • 2Maryland Center for Fundamental Physics, Department of Physics, University of Maryland, College Park, Maryland 20742, USA
  • 3Department of Physics, Enrico Fermi Institute, and Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
  • 4Department of Physics, University of California at San Diego, La Jolla, California 92093, USA

Article Text

Click to Expand

References

Click to Expand
Issue

Vol. 103, Iss. 7 — 1 April 2021

Reuse & Permissions
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Reuse & Permissions

It is not necessary to obtain permission to reuse this article or its components as it is available under the terms of the Creative Commons Attribution 4.0 International license. This license permits unrestricted use, distribution, and reproduction in any medium, provided attribution to the author(s) and the published article's title, journal citation, and DOI are maintained. Please note that some figures may have been included with permission from other third parties. It is your responsibility to obtain the proper permission from the rights holder directly for these figures.

×

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×