Content area

Abstract

We perform a likelihood analysis of the minimal anomaly-mediated supersymmetry-breaking (mAMSB) model using constraints from cosmology and accelerator experiments. We find that either a wino-like or a Higgsino-like neutralino LSP, χ~10, may provide the cold dark matter (DM), both with similar likelihoods. The upper limit on the DM density from Planck and other experiments enforces mχ~103TeV after the inclusion of Sommerfeld enhancement in its annihilations. If most of the cold DM density is provided by the χ~10, the measured value of the Higgs mass favours a limited range of tanβ5 (and also for tanβ45 if μ>0) but the scalar mass m0 is poorly constrained. In the wino-LSP case, m3/2 is constrained to about 900TeV and mχ~10 to 2.9±0.1TeV, whereas in the Higgsino-LSP case m3/2 has just a lower limit 650TeV (480TeV) and mχ~10 is constrained to 1.12(1.13)±0.02TeV in the μ>0 (μ<0) scenario. In neither case can the anomalous magnetic moment of the muon, (g-2)μ, be improved significantly relative to its Standard Model (SM) value, nor do flavour measurements constrain the model significantly, and there are poor prospects for discovering supersymmetric particles at the LHC, though there are some prospects for direct DM detection. On the other hand, if the χ~10 contributes only a fraction of the cold DM density, future LHC -based searches for gluinos, squarks and heavier chargino and neutralino states as well as disappearing track searches in the wino-like LSP region will be relevant, and interference effects enable BR(Bs,dμ+μ-) to agree with the data better than in the SM in the case of wino-like DM with μ>0.

Details

Title
Likelihood analysis of the minimal AMSB model
Author
Bagnaschi, E 1 ; Borsato, M 2 ; Sakurai, K 3 ; Buchmueller, O 4 ; Cavanaugh, R 5 ; Chobanova, V 2 ; Citron, M 4 ; Costa, J C 4 ; De Roeck, A 6 ; Dolan, M J 7 ; Ellis, J R 8 ; Flächer, H 9 ; Heinemeyer, S 10 ; Isidori, G 11 ; Lucio, M 2 ; Luo, F 12 ; D Martínez Santos 2 ; Olive, K A 13 ; Richards, A 4 ; Weiglein, G 1 

 DESY, Hamburg, Germany 
 Universidade de Santiago de Compostela, Santiago de Compostela, Spain 
 Science Laboratories, Department of Physics, Institute for Particle Physics Phenomenology, University of Durham, Durham, UK; Faculty of Physics, Institute of Theoretical Physics, University of Warsaw, Warsaw, Poland 
 High Energy Physics Group, Blackett Laboratory, Imperial College, London, UK 
 Fermi National Accelerator Laboratory, Batavia, IL, USA; Physics Department, University of Illinois at Chicago, Chicago, IL, USA 
 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; Theoretical Physics Department, CERN, Geneva 23, Switzerland 
 H.H. Wills Physics Laboratory, University of Bristol, Bristol, UK 
10  Campus of International Excellence UAM+CSIC, Madrid, Spain; Instituto de Física Teórica UAM-CSIC, Madrid, Spain; Instituto de Física de Cantabria (CSIC-UC), Cantabria, Spain 
11  Physik-Institut, Universität Zürich, Zurich, Switzerland 
12  Kavli IPMU (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba, Japan 
13  William I. Fine Theoretical Physics Institute, School of Physics and Astronomy, University of Minnesota, Minneapolis, MN, USA 
Pages
1-28
Publication year
2017
Publication date
Apr 2017
Publisher
Springer Nature B.V.
ISSN
14346044
e-ISSN
14346052
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
1977905451
Copyright
The European Physical Journal C is a copyright of Springer, (2017). All Rights Reserved.