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 »
- Authors:
-
- 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}
}
Web of Science
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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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