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Abstract

We use MasterCode to perform a frequentist analysis of the constraints on a phenomenological MSSM model with 11 parameters, the pMSSM11, including constraints from 36/fb of LHC data at 13 TeV and PICO, XENON1T and PandaX-II searches for dark matter scattering, as well as previous accelerator and astrophysical measurements, presenting fits both with and without the (g-2)μ constraint. The pMSSM11 is specified by the following parameters: 3 gaugino masses M1,2,3, a common mass for the first-and second-generation squarks mq~ and a distinct third-generation squark mass mq~3, a common mass for the first-and second-generation sleptons m~ and a distinct third-generation slepton mass mτ~, a common trilinear mixing parameter A, the Higgs mixing parameter μ, the pseudoscalar Higgs mass MA and tanβ. In the fit including (g-2)μ, a Bino-like χ~10 is preferred, whereas a Higgsino-like χ~10 is mildly favoured when the (g-2)μ constraint is dropped. We identify the mechanisms that operate in different regions of the pMSSM11 parameter space to bring the relic density of the lightest neutralino, χ~10, into the range indicated by cosmological data. In the fit including (g-2)μ, coannihilations with χ~20 and the Wino-like χ~1± or with nearly-degenerate first- and second-generation sleptons are active, whereas coannihilations with the χ~20 and the Higgsino-like χ~1± or with first- and second-generation squarks may be important when the (g-2)μ constraint is dropped. In the two cases, we present χ2 functions in two-dimensional mass planes as well as their one-dimensional profile projections and best-fit spectra. Prospects remain for discovering strongly-interacting sparticles at the LHC, in both the scenarios with and without the (g-2)μ constraint, as well as for discovering electroweakly-interacting sparticles at a future linear e+e- collider such as the ILC or CLIC.

Details

Title
Likelihood analysis of the pMSSM11 in light of LHC 13-TeV data
Author
Bagnaschi, E 1   VIAFID ORCID Logo  ; Sakurai, K 2 ; Borsato, M 3 ; Buchmueller, O 4 ; Citron, M 4 ; Costa, J C 4 ; De Roeck, A 5 ; Dolan, M J 6 ; Ellis, J R 7 ; Flächer, H 8 ; Heinemeyer, S 9 ; Lucio, M 3 ; D Martínez Santos 3 ; Olive, K A 10 ; Richards, A 4 ; Spanos, V C 11 ; I Suárez Fernández 3 ; Weiglein, G 1 

 DESY, Hamburg, Germany 
 Faculty of Physics, Institute of Theoretical Physics, University of Warsaw, Warsaw, Poland 
 Instituto Galego de Física de Altas Enerxías, Universidade de Santiago de Compostela, Santiago de Compostela, Spain 
 High Energy Physics Group, Blackett Laboratory, Imperial College, London, UK 
 Experimental Physics Department, CERN, Geneva 23, Switzerland; Antwerp University, Wilrijk, Belgium 
 ARC Centre of Excellence for Particle Physics at the Terascale, School of Physics, University of Melbourne, Melbourne, Australia 
 Theoretical Particle Physics and Cosmology Group, Department of Physics, King’s College London, London, UK; National Institute of Chemical Physics and Biophysics, Tallinn, Estonia; Theoretical Physics Department, CERN, Geneva 23, Switzerland 
 H.H. Wills Physics Laboratory, University of Bristol, Bristol, UK 
 Campus of International Excellence UAM+CSIC, Cantoblanco, Madrid, Spain; Instituto de Física Teórica UAM-CSIC, Madrid, Spain; Instituto de Física de Cantabria (CSIC-UC), Santander, Spain 
10  William I. Fine Theoretical Physics Institute, School of Physics and Astronomy, University of Minnesota, Minneapolis, MN, USA 
11  Section of Nuclear and Particle Physics, Department of Physics, National and Kapodistrian University of Athens, Athens, Greece 
Pages
1-38
Publication year
2018
Publication date
Mar 2018
Publisher
Springer Nature B.V.
ISSN
14346044
e-ISSN
14346052
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2017580199
Copyright
The European Physical Journal C is a copyright of Springer, (2018). All Rights Reserved.