4,280 research outputs found

    Radiative Decays of the Higgs Boson to a Pair of Fermions

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    We revisit the radiative decays of the Higgs boson to a fermion pair h→ffˉγh\rightarrow f\bar{f}\gamma where ff denotes a fermion in the Standard Model (SM). We include the chirality-flipping diagrams via the Yukawa couplings at the order O(yf2α)\mathcal{O}(y_f^2 \alpha), the chirality-conserving contributions via the top-quark loops of the order O(yt2α3)\mathcal{O}(y_t^2 \alpha^3), and the electroweak loops at the order O(α4)\mathcal{O}(\alpha^4). The QED correction is about Qf2×O(1%)Q_f^2\times {\cal O}(1\%) and contributes to the running of fermion masses at a similar level, which should be taken into account for future precision Higgs physics. The chirality-conserving electroweak-loop processes are interesting from the observational point of view. First, the branching fraction of the radiative decay h→μ+μ−γh \to \mu^+\mu^- \gamma is about a half of that of h→μ+μ−h \to \mu^+\mu^-, and that of h→e+e−γh \to e^+ e^- \gamma is more than four orders of magnitude larger than that of h→e+e−h \to e^+ e^-, both of which reach about 10−410^{-4}. The branching fraction of h→τ+τ−γh \to \tau^+\tau^- \gamma is of the order 10−310^{-3}. All the leptonic radiative decays are potentially observable at the LHC Run 2 or the HL-LHC. The kinematic distributions for the photon energy or the fermion pair invariant mass provide non-ambiguous discrimination for the underlying mechanisms of the Higgs radiative decay. We also study the process h→ccˉγh \to c\bar c \gamma and evaluate the observability at the LHC. We find it comparable to the other related studies and better than the h→J/ψ γh \to J/\psi\ \gamma channel in constraining the charm-Yukawa coupling.Comment: 23 pages, 6 figures, 6 tables; Minor corrections, references updated, version published in JHE

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    Dark Matter Blind Spots at One-Loop

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    We evaluate the impact of one-loop electroweak corrections to the spin-independent dark matter (DM) scattering cross-section with nucleons (σSI\sigma_{\rm SI}), in models with a so-called blind spot for direct detection, where the leading-order prediction for the relevant DM coupling to the Higgs boson, and therefore σSI\sigma_{\rm SI}, are vanishingly small. Adopting a simple illustrative scenario in which the DM state results from the mixing of electroweak singlet and doublet fermions, we compute the relevant higher order corrections to the scalar effective operator contributions to σSI\sigma_{\rm SI}, stemming from both triangle and box diagrams involving the SM and dark sector fields. It is observed that in a significant region of the singlet-doublet model-space, the one-loop corrections ``unblind'' the tree-level blind spots and lead to detectable SI scattering rates at future multi-ton scale liquid Xenon experiments, with σSI\sigma_{\rm SI} reaching values up to a few times 10−47 cm210^{-47} {~\rm cm}^2, for a weak scale DM with O(1)\mathcal{O}(1) Yukawa couplings. Furthermore, we find that there always exists a new SI blind spot at the next-to-leading order, which is perturbatively shifted from the leading order one in the singlet-doublet mass parameters. For comparison, we also present the tree-level spin-dependent scattering cross-sections near the SI blind-spot region, that could lead to a larger signal. Our results can be mapped to the blind-spot scenario for bino-Higgsino DM in the MSSM, with other sfermions, the heavier Higgs boson, and the wino decoupled.Comment: 20 pages, 5 figures; Minor corrections, references updated, version published in JHE

    WIMPs at High Energy Muon Colliders

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    The Weakly Interacting Massive Particle (WIMP) paradigm is one of the most compelling scenarios for particle dark matter (DM). We show in this paper that a high energy muon collider can make decisive statements about the WIMP DM, and this should serve as one of its main physics driver cases. We demonstrate this by employing the DM as the lightest member of an electroweak (EW) multiplet, which is a simple, yet one of the most challenging WIMP scenarios given its minimal collider signature and high thermal target mass scale of 1 TeV−-23 TeV. We perform a first study of the reach of high energy muon colliders, focusing on the simple, inclusive and conservative signals with large missing mass, through the mono-photon, VBF di-muon and a novel mono-muon channel. Using these inclusive signals, it is possible to cover the thermal targets of doublet and triplet with a 10 TeV muon collider. Higher energies, 14 TeV−-75 TeV, would ensure a 5σ5 \sigma reach above the thermal targets for the higher EW multiplets. We also estimate the reach of a search for disappearing tracks, demonstrating the potential significant enhancement of the sensitivity.Comment: v1: 33 pages, 16 figures, 3 tables; v2: minor updates, matches PRD published version; v3: doublet disappearing track numerical results corrected, conclusions improves; also matches PRD errat

    Revisiting the Pion Leading-Twist Distribution Amplitude within the QCD Background Field Theory

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    We study the pion leading-twist distribution amplitude (DA) within the framework of SVZ sum rules under the background field theory. To improve the accuracy of the sum rules, we expand both the quark propagator and the vertex (z\cdot \tensor{D})^n of the correlator up to dimension-six operators in the background field theory. The sum rules for the pion DA moments are obtained, in which all condensates up to dimension-six have been taken into consideration. Using the sum rules, we obtain \left|_{\rm 1\;GeV} = 0.338 \pm 0.032, \left|_{\rm 1\;GeV} = 0.211 \pm 0.030 and \left|_{\rm 1\;GeV} = 0.163 \pm 0.030. It is shown that the dimension-six condensates shall provide sizable contributions to the pion DA moments. We show that the first Gegenbauer moment of the pion leading-twist DA is a2π∣1  GeV=0.403±0.093a^\pi_2|_{\rm 1\;GeV} = 0.403 \pm 0.093, which is consistent with those obtained in the literature within errors but prefers a larger central value as indicated by lattice QCD predictions.Comment: 13 pages, 7 figure
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