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MSSM: Cornered and Correlated
High Energy Physics - Phenomenology · Submitted 29 Oct 2012
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim In contrast, the Higgs-boson couplings show good overall agreement with the preliminary experimental determinations, the DM abundance is consistent with observation, and the discrepancy in (g-2)_mu is reduced.
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Inspired by the latest results of ATLAS and CMS on the search for the standard model (SM) Higgs scalar, we discuss in this article the correlations between Higgs-boson properties, low-energy observables, such as B -> X_sgamma, B_s -> mu^+mu^-, and (g-2)_mu, and the dark matter (DM) relic density. We focus on the corners of the MSSM parameter space where the pp -> h -> gammagamma signal is enhanced due to the presence of a light stau state. In this region tan(beta), M_A, A_t, and mu take large values, and we find striking correlations between many of the considered observables. In particular, the B -> X_sgamma branching fraction is enhanced, while the B_s -> mu^+mu^- rate tends to be below the SM expectation. In contrast, the Higgs-boson couplings show good overall agreement with the preliminary experimental determinations, the DM abundance is consistent with observation, and the discrepancy in (g-2)_mu is reduced. The predicted deviations and found correlations could be tested in the near future and hence may become very valuable as guidelines and consistency checks.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | Inspired by the latest results of ATLAS and CMS on the search for the standard model (SM) Higgs scalar, we discuss in this article the correlations between Higgs-boson properties, low-energy observables, such as B -> X_sgamma, B_s -> mu^+mu^-, and (g-2)_mu, and the dark matter (DM) relic density. | contribution 0.76 | 0.43 | 0.07 | asserted 0.65 |
| s1 | We focus on the corners of the MSSM parameter space where the pp -> h -> gammagamma signal is enhanced due to the presence of a light stau state. | contribution 0.92 | 0.37 | 0.07 | asserted 0.97 |
| s2 | In this region tan(beta), M_A, A_t, and mu take large values, and we find striking correlations between many of the considered observables. | result 0.75 | 0.94 | 0.17 | asserted 1.00 |
| s3 | In particular, the B -> X_sgamma branching fraction is enhanced, while the B_s -> mu^+mu^- rate tends to be below the SM expectation. | result 1.00 | 0.86 | 0.18 | asserted 0.95 |
| s4 | In contrast, the Higgs-boson couplings show good overall agreement with the preliminary experimental determinations, the DM abundance is consistent with observation, and the discrepancy in (g-2)_mu is reduced. | result 0.99 | 0.84 | 0.33 | asserted 0.77 |
| s5 | The predicted deviations and found correlations could be tested in the near future and hence may become very valuable as guidelines and consistency checks. | interpretation 0.65 | 0.37 | 0.32 | hedged possibility 1.00 |
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The paper
Original abstract
Inspired by the latest results of ATLAS and CMS on the search for the standard model (SM) Higgs scalar, we discuss in this article the correlations between Higgs-boson properties, low-energy observables, such as B -> X_sgamma, B_s -> mu^+mu^-, and (g-2)_mu, and the dark matter (DM) relic density. We focus on the corners of the MSSM parameter space where the pp -> h -> gammagamma signal is enhanced due to the presence of a light stau state. In this region tan(beta), M_A, A_t, and mu take large values, and we find striking correlations between many of the considered observables. In particular, the B -> X_sgamma branching fraction is enhanced, while the B_s -> mu^+mu^- rate tends to be below the SM expectation. In contrast, the Higgs-boson couplings show good overall agreement with the preliminary experimental determinations, the DM abundance is consistent with observation, and the discrepancy in (g-2)_mu is reduced. The predicted deviations and found correlations could be tested in the near future and hence may become very valuable as guidelines and consistency checks.
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References
How the literature uses it
24 arXiv papers cite this in 41 sentences
Papers citing it · 32 sentences without a confident label
Uses its data or values 1 paper
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If we assume a 10% uncertainty in the SUSY calculation and combining the experimental limits together with the corresponding SM predictions, we get the following constraints at 95% C.L. on the $R(X)$: * $B →X_s γ$ [ref] [equation] * $B_q →l^+ l^-$ [ref] [equation] * $ΔM_B_q$ [ref] [equation]
Resurrecting light stops after the 125 GeV Higgs in the baryon number violating CMSSM · Numerical setup · 0.96
Compares with it 1 paper
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We note that the above agrees with the analysis of Ref. [ref] where $Br(B_s →μ^+ μ^-)$ for a large $tanβ$ is seen to be enhanced for $μA_t<0$.
Exploring MSSM for Charge and Color Breaking and Other Constraints in the Context of Higgs@125 GeV · Scan over wide range of $μ$ and $A_t$ for $tanβ=40$ · 0.82
Cites it as background 6 papers
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We consider now the contributions of SUSY particles to the $γγ$ branching fraction and, eventually, to the $gg→h$ amplitude [ref] .
An update of the constraints on the phenomenological MSSM from the new LHC Higgs results · SUSY corrections to the Higgs rates · 0.90
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Most of the papers on these “p$n$MSSM” models analyzed the impact of constraints from direct LHC SUSY searches [ref] , from the Higgs discovery [ref] , from $b$-physics [ref] , and from direct and indirect detection of DM [ref] .
Dark matter and collider signatures of the MSSM · Introduction · 0.95
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In general, many models involving new particles have been introduced to account for the enhancement in the photon channel, some without embedding the new physics into a motivated UV completion, others studying $h→γγ$ in (more) complete models, addressing the hierarchy problem of particle physics [ref] .
Custodial Leptons and Higgs Decays · Introduction · 0.99
What it cites · 65 sentences without a confident label
Builds on 6 papers
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In this article we dissect the “light stau scenario” extending previous analyses [ref] that are similar in spirit.
A 125 GeV SM-like Higgs in the MSSM and the $\gamma \gamma$ rate · Introduction · 0.96
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In this article we dissect the “light stau scenario” extending previous analyses [ref] that are similar in spirit.
Light Stau Phenomenology and the Higgs \gamma\gamma Rate · Introduction · 0.96
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In this article we dissect the “light stau scenario” extending previous analyses [ref] that are similar in spirit.
Searching SUSY Leptonic Partner at the CERN LHC · Introduction · 0.96
Uses the method or tool of 5 papers
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All results presented below have been obtained using SoftSusy 3.3.3 [ref] for the spectrum calculation, Higlu 3.11 [ref] and Hdecay 4.45 [ref] for the computation of Higgs-boson production and decay, and SuperIso Relic 3.3 [ref] for the calculation of the relevant low-energy observables and the DM abundance.
SuperIso: A program for calculating the isospin asymmetry of B -> K* gamma in the MSSM · Numerical Analysis · 1.00
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All results presented below have been obtained using SoftSusy 3.3.3 [ref] for the spectrum calculation, Higlu 3.11 [ref] and Hdecay 4.45 [ref] for the computation of Higgs-boson production and decay, and SuperIso Relic 3.3 [ref] for the calculation of the relevant low-energy observables and the DM abundance.
SuperIso Relic: A program for calculating relic density and flavor physics observables in Supersymmetry · Numerical Analysis · 1.00
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All results presented below have been obtained using SoftSusy 3.3.3 [ref] for the spectrum calculation, Higlu 3.11 [ref] and Hdecay 4.45 [ref] for the computation of Higgs-boson production and decay, and SuperIso Relic 3.3 [ref] for the calculation of the relevant low-energy observables and the DM abundance.
SOFTSUSY: a program for calculating supersymmetric spectra · Numerical Analysis · 1.00
Uses data or values from 11 papers
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Combining the experimental result [ref] with the SM calculation, based on an update of the hadronic vacuum polarisation contributions [ref] and the complete tenth-order QED corrections [ref] , results in Δa_μ= a_μ^exp - a_μ^SM = (2.5 ±0.9) ·10^-9 .
(g-2)_mu and alpha(M_Z^2) re-evaluated using new precise data · Numerical Analysis · 0.97
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Combining the experimental result [ref] with the SM calculation, based on an update of the hadronic vacuum polarisation contributions [ref] and the complete tenth-order QED corrections [ref] , results in Δa_μ= a_μ^exp - a_μ^SM = (2.5 ±0.9) ·10^-9 .
Complete Tenth-Order QED Contribution to the Muon g-2 · Numerical Analysis · 0.97
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While the achieved precision is so far insufficient to draw any final conclusion, one cannot help but noticing that the LHC data match well the SM prediction with one possible exception: the central value of the measured relative strength of the diphoton signal is too large by about $70%$ [ref] .
Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC · Introduction · 0.88
Compares with 1 paper
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The result ([ref]) agrees with the expression given in [ref] .
Viability of MSSM scenarios at very large tan(beta) · Anatomy of Low-Energy Observables · 0.96
Cites as support 1 paper
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In the context of the minimal supersymmetric SM (MSSM) a light, maximally mixed stau can be shown to increase the loop-induced $hγγ$ coupling [ref] , hence leading to the desired effect.
A 125 GeV SM-like Higgs in the MSSM and the $\gamma \gamma$ rate · Introduction · 0.96
Cites as background 2 papers
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In the decoupling limit of the MSSM, , $M_A^2 ≫M_Z^2$, the lightest CP-even Higgs boson (for a review including original references, see [ref] ) acquires the squared tree-level mass M_h^2 ≈M_Z^2 c^2_2β ( 1 - M_Z^2/M_A^2 s_2 β^2 ) .
The Anatomy of Electro-Weak Symmetry Breaking. II: The Higgs bosons in the Minimal Supersymmetric Model · Anatomy of Higgs-Boson Mass · 0.99
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In the MSSM, this observable receives one-loop contributions from Feynman diagrams with neutralino and smuon as well as chargino and sneutrino exchange (see [ref] for topical reviews).
The Muon Magnetic Moment and Supersymmetry · Anatomy of Low-Energy Observables · 0.99
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