• Open Access

Closing in on the chargino contribution to the muon g2 in the MSSM: Current LHC constraints

Kaoru Hagiwara, Kai Ma, and Satyanarayan Mukhopadhyay
Phys. Rev. D 97, 055035 – Published 26 March 2018

Abstract

We revisit the current LHC constraints on the electroweak-ino sector parameters in the minimal supersymmetric standard model (MSSM) that are relevant to explaining the (g2)μ anomaly via the dominant chargino and muon sneutrino loop. Since the LHC bounds on electroweak-inos become weaker if they decay via an intermediate stau or a tau sneutrino instead of the first two generation sleptons, we perform a detailed analysis of the scenario with a bino as the lightest supersymmetric particle (LSP) and a light stau as the next-to-lightest one (NLSP). Even in this scenario, the chargino sector parameters in the MSSM that can account for the (g2)μ anomaly within 1σ are already found to be significantly constrained by the 8 TeV LHC and the available subset of the 13 TeV LHC limits. We also estimate the current LHC exclusions in the left-smuon (and/or left-selectron) NLSP scenario from multilepton searches, and further combine the constraints from the multitau and multilepton channels for a mass spectrum in which all three generations of sleptons are lighter than the chargino. In the latter two cases, small corners of the 1σ favored region for (g2)μ are still allowed at present.

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  • Received 18 July 2017

DOI:https://doi.org/10.1103/PhysRevD.97.055035

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
Particles & Fields

Authors & Affiliations

Kaoru Hagiwara1,2,*, Kai Ma1,3,†, and Satyanarayan Mukhopadhyay2,‡

  • 1KEK Theory Center, Tsukuba 305-0801, Japan
  • 2PITT-PACC, Department of Physics and Astronomy, University of Pittsburgh, Pennsylvania 15260, USA
  • 3Department of Physics, Shaanxi Sci-Tech University, Hanzhong 723000, Shaanxi, China

  • *kaoru.hagiwara@kek.jp
  • makainca@yeah.net
  • satya@pitt.edu

Article Text

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Issue

Vol. 97, Iss. 5 — 1 March 2018

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