Dark Matter after LHC Run I: Clues to Unification

Keith A. Olive

doi:10.1051/epjconf/201713601001

Dark Matter after LHC Run I: Clues to Unification

Keith A. Olive

Physics and Astronomy (Twin Cities)

Research output: Contribution to journal › Conference article › peer-review

Abstract

After the results of Run I, can we still 'guarantee' the discovery of supersymmetry at the LHC? It is shown that viable dark matter models in CMSSM-like models tend to lie in strips (co-annihilation, funnel, focus point). The role of grand unification in constructing supersymmetric models is discussed and it is argued that non-supersymmetric GUTs such as SO(10) may provide solutions to many of the standard problems addressed by supersymmetry.

Original language	English (US)
Article number	01001
Journal	EPJ Web of Conferences
Volume	136
DOIs	https://doi.org/10.1051/epjconf/201713601001
State	Published - Mar 23 2017
Event	6th Roma International Conference on Astroparticle Physics, RICAP 2016 - Frascati, Roma, Italy Duration: Jun 21 2016 → Jun 24 2016

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© The Authors, published by EDP Sciences, 2017.

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title = "Dark Matter after LHC Run I: Clues to Unification",

abstract = "After the results of Run I, can we still 'guarantee' the discovery of supersymmetry at the LHC? It is shown that viable dark matter models in CMSSM-like models tend to lie in strips (co-annihilation, funnel, focus point). The role of grand unification in constructing supersymmetric models is discussed and it is argued that non-supersymmetric GUTs such as SO(10) may provide solutions to many of the standard problems addressed by supersymmetry.",

author = "Olive, \{Keith A.\}",

note = "Publisher Copyright: {\textcopyright} The Authors, published by EDP Sciences, 2017.; 6th Roma International Conference on Astroparticle Physics, RICAP 2016 ; Conference date: 21-06-2016 Through 24-06-2016",

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N1 - Publisher Copyright: © The Authors, published by EDP Sciences, 2017.

PY - 2017/3/23

Y1 - 2017/3/23

N2 - After the results of Run I, can we still 'guarantee' the discovery of supersymmetry at the LHC? It is shown that viable dark matter models in CMSSM-like models tend to lie in strips (co-annihilation, funnel, focus point). The role of grand unification in constructing supersymmetric models is discussed and it is argued that non-supersymmetric GUTs such as SO(10) may provide solutions to many of the standard problems addressed by supersymmetry.

AB - After the results of Run I, can we still 'guarantee' the discovery of supersymmetry at the LHC? It is shown that viable dark matter models in CMSSM-like models tend to lie in strips (co-annihilation, funnel, focus point). The role of grand unification in constructing supersymmetric models is discussed and it is argued that non-supersymmetric GUTs such as SO(10) may provide solutions to many of the standard problems addressed by supersymmetry.

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DO - 10.1051/epjconf/201713601001

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AN - SCOPUS:85017097627

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JO - EPJ Web of Conferences

JF - EPJ Web of Conferences

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Y2 - 21 June 2016 through 24 June 2016

ER -

Dark Matter after LHC Run I: Clues to Unification

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