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Title: LHC SUSY and WIMP dark matter searches confront the string theory landscape

Abstract

The string theory landscape of vacua solutions provides physicists with some understanding as to the magnitude of the cosmological constant. Similar reasoning can be applied to the magnitude of the soft SUSY breaking terms in supersymmetric models of particle physics: there appears to be a statistical draw towards large soft terms which is tempered by the anthropic requirement of the weak scale lying not too far from ~100 GeV. For a mild statistical draw of m softn with n = 1 (as expected from SUSY breaking due to a single F term) then the light Higgs mass is preferred at ~125 GeV while sparticles are all pulled beyond LHC bounds. We confront a variety of LHC and WIMP dark matter search limits with the statistical expectations from a fertile patch of string theory landscape. The end result is that LHC and WIMP dark matter detectors see exactly that which is expected from the landscape: a Standard Model-like Higgs boson of mass 125 GeV but as yet no sign of sparticles or WIMP dark matter. SUSY from the n = 1 landscape is most likely to emerge at LHC in the soft opposite-sign dilepton plus jet plus MET channel. Multi-ton noblemore » liquid WIMP detectors should be able to completely explore the n = 1 landscape parameter space.« less

Authors:
ORCiD logo [1]; ; ; ;
  1. University of Oklahoma
Publication Date:
Research Org.:
Univ. of Oklahoma, Norman, OK (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP)
OSTI Identifier:
1600529
Report Number(s):
arXiv:1901.11060
Journal ID: ISSN 1029-8479; arXiv:1901.11060; TRN: US2103559
Grant/Contract Number:  
SC0009956
Resource Type:
Accepted Manuscript
Journal Name:
Journal of High Energy Physics (Online)
Additional Journal Information:
Journal Name: Journal of High Energy Physics (Online); Journal Volume: 2019; Journal Issue: 4; Journal ID: ISSN 1029-8479
Publisher:
Springer Berlin
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; supersymmetry; LHC; dark matter; string theory

Citation Formats

Baer, Howard, Barger, Vernon, Salam, Shadman, Serce, Hasan, and Sinha, Kuver. LHC SUSY and WIMP dark matter searches confront the string theory landscape. United States: N. p., 2019. Web. doi:10.1007/JHEP04(2019)043.
Baer, Howard, Barger, Vernon, Salam, Shadman, Serce, Hasan, & Sinha, Kuver. LHC SUSY and WIMP dark matter searches confront the string theory landscape. United States. https://doi.org/10.1007/JHEP04(2019)043
Baer, Howard, Barger, Vernon, Salam, Shadman, Serce, Hasan, and Sinha, Kuver. Thu . "LHC SUSY and WIMP dark matter searches confront the string theory landscape". United States. https://doi.org/10.1007/JHEP04(2019)043. https://www.osti.gov/servlets/purl/1600529.
@article{osti_1600529,
title = {LHC SUSY and WIMP dark matter searches confront the string theory landscape},
author = {Baer, Howard and Barger, Vernon and Salam, Shadman and Serce, Hasan and Sinha, Kuver},
abstractNote = {The string theory landscape of vacua solutions provides physicists with some understanding as to the magnitude of the cosmological constant. Similar reasoning can be applied to the magnitude of the soft SUSY breaking terms in supersymmetric models of particle physics: there appears to be a statistical draw towards large soft terms which is tempered by the anthropic requirement of the weak scale lying not too far from ~100 GeV. For a mild statistical draw of m softn with n = 1 (as expected from SUSY breaking due to a single F term) then the light Higgs mass is preferred at ~125 GeV while sparticles are all pulled beyond LHC bounds. We confront a variety of LHC and WIMP dark matter search limits with the statistical expectations from a fertile patch of string theory landscape. The end result is that LHC and WIMP dark matter detectors see exactly that which is expected from the landscape: a Standard Model-like Higgs boson of mass 125 GeV but as yet no sign of sparticles or WIMP dark matter. SUSY from the n = 1 landscape is most likely to emerge at LHC in the soft opposite-sign dilepton plus jet plus MET channel. Multi-ton noble liquid WIMP detectors should be able to completely explore the n = 1 landscape parameter space.},
doi = {10.1007/JHEP04(2019)043},
journal = {Journal of High Energy Physics (Online)},
number = 4,
volume = 2019,
place = {United States},
year = {Thu Apr 04 00:00:00 EDT 2019},
month = {Thu Apr 04 00:00:00 EDT 2019}
}

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Works referencing / citing this record:

Is the magnitude of the Peccei–Quinn scale set by the landscape?
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Revisiting the SUSY mu problem and its solutions in the LHC era
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