• Open Access

LHC luminosity and energy upgrades confront natural supersymmetry models

Howard Baer, Vernon Barger, James S. Gainer, Dibyashree Sengupta, Hasan Serce, and Xerxes Tata
Phys. Rev. D 98, 075010 – Published 12 October 2018

Abstract

The electroweak fine-tuning measure ΔEW allows for correlated supersymmetry (SUSY) soft terms as are expected in any ultraviolet complete theory. Requiring no less than 3% electroweak fine-tuning implies upper bounds of about 360 GeV on all Higgsinos, while top squarks are lighter than 3TeV and gluinos are bounded by 69TeV. We examine the reach for SUSY of the planned high luminosity (HL: 3ab1 at 14 TeV) and the proposed high energy (HE: 15ab1 at 27 TeV) upgrades of the LHC via four LHC collider search channels relevant for natural SUSY: 1. gluino pair production followed by gluino decay to third generation (s)quarks, 2. top squark pair production followed by decay to third generation quarks and light Higgsinos, 3. neutral Higgsino pair production with QCD jet radiation (resulting in monojet events with soft dileptons), and 4. wino pair production followed by decay to light Higgsinos leading to same-sign diboson production. We confront our reach results with upper limits on superpartner masses in four natural SUSY models: natural gravity mediation via the 1. two- and 2. three-extra-parameter nonuniversal Higgs models, 3. natural minilandscape models with generalized mirage mediation and 4. natural anomaly mediation We find that while the HL-LHC can probe considerable portions of natural SUSY parameter space in all these models, the HE-LHC will decisively cover the entire natural SUSY parameter space with better than 3% fine-tuning.

  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
1 More
  • Received 21 August 2018

DOI:https://doi.org/10.1103/PhysRevD.98.075010

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)

  1. Research Areas
Particles & Fields

Authors & Affiliations

Howard Baer1,*, Vernon Barger2,†, James S. Gainer3,‡, Dibyashree Sengupta1,§, Hasan Serce1,∥, and Xerxes Tata3,4,¶

  • 1Department of Physics and Astronomy, University of Oklahoma, Norman, Oklahoma 73019, USA
  • 2Department of Physics, University of Wisconsin, Madison, Wisconsin 53706, USA
  • 3Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA
  • 4Centre for High Energy Physics, Indian Institute of Science, Bangalore 560012, India

  • *baer@nhn.ou.edu
  • barger@pheno.wisc.edu
  • jgainer@hawaii.edu
  • §Dibyashree.Sengupta-1@ou.edu
  • serce@ou.edu
  • tata@phys.hawaii.edu

Article Text

Click to Expand

References

Click to Expand
Issue

Vol. 98, Iss. 7 — 1 October 2018

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
×