233 research outputs found

    Leptophilic dark matter in gauged U(1)Le−LμU(1)_{L_e-L_\mu} model in light of DAMPE cosmic ray e++e−e^+ + e^- excess

    Full text link
    Motivated by the very recent cosmic-ray electron+positron excess observed by DAMPE collaboration, we investigate a Dirac fermion dark matter (DM) in the gauged Le−LμL_e - L_\mu model. DM interacts with the electron and muon via the U(1)e−μU(1)_{e-\mu} gauge boson Z′Z^{'}. The model can explain the DAMPE data well. Although a non-zero DM-nucleon cross section is only generated at one loop level and there is a partial cancellation between Z′eeZ^{'}ee and Z′μμZ^{'}\mu\mu couplings, we find that a large portion of Z′Z^{'} mass is ruled out from direct DM detection limit leaving the allowed Z′Z^{'} mass to be close to two times of the DM mass. Implications for pp→Z′→2ℓpp \to Z^{'} \to 2\ell and pp→2ℓ+Z′pp \to 2\ell + Z^{'} , and muon g−2g-2 anomaly are also studied.Comment: Discussions added, version accepted by EPJ

    Vacuum stability in stau-neutralino coannihilation in MSSM

    Full text link
    The stau-neutralino coannihilation provides a feasible way to accommodate the observed cosmological dark matter (DM) relic density in the minimal supersymmetric standard model (MSSM). In such a coannihilation mechanism the stau mass usually has an upper bound since its annihilation rate becomes small with the increase of DM mass. Inspired by this observation, we examine the upper limit of stau mass in the parameter space with a large mixing of staus. We find that the stau pair may dominantly annihilate into dibosons and hence the upper bound on the stau mass (∼400\sim400 GeV) obtained from the ffˉf\bar{f} final states can be relaxed. Imposing the DM relic density constraint and requiring a long lifetime of the present vacuum, we find that the lighter stau mass can be as heavy as about 1.4 TeV for the stau maximum mixing. However, if requiring the present vacuum to survive during the thermal history of the universe, this mass limit will reduce to about 0.9 TeV. We also discuss the complementarity of vacuum stability and direct detections in probing this stau coannihilation scenario.Comment: 12 pages, 6 figure

    A minimal U(1)′U(1)^\prime extension of MSSM in light of the B decay anomaly

    Full text link
    Motivated by the RKR_K and RK∗R_{K^*} anomalies from B decays, we extend the minimal supersymmetric model with a non-universal anomaly-free U(1)′U(1)^\prime gauge symmetry, coupling non-universally to the lepton sector as well as the quark sector. In particular, only the third generation quarks are charged under this U(1)′U(1)^\prime, which can easily evade the dilepton bound from the LHC searches. An extra singlet is introduced to break this U(1)′U(1)^\prime symmetry allowing for the μ\mu-term to be generated dynamically. The relevant constraints of Bs−BˉsB_s-\bar{B}_s mixing, D0−Dˉ0D^0-\bar{D}^0 mixing and the LHC dilepton searches are considered. We find that in the allowed parameter space this U(1)′U(1)^\prime gauge interaction can accommodate the RKR_K and RK∗R_{K^*} anomalies and weaken considerably the Z′Z^\prime mass limits while remaining perturbative up to the Planck scale.Comment: 12 pages,2 figure

    Probing GeV-scale MSSM neutralino dark matter in collider and direct detection experiments

    Full text link
    Given the recent constraints from the dark matter (DM) direct detections, we examine a light GeV-scale (2-30 GeV) neutralino DM in the alignment limit of the Minimal Supersymmetric Standard Model (MSSM). In this limit without decoupling, the heavy CP-even scalar HH plays the role of the Standard Model (SM) Higgs boson while the other scalar hh can be rather light so that the DM can annihilate through the hh resonance or into a pair of hh to achieve the observed relic density. With the current collider and cosmological constraints, we find that such a light neutralino DM above 6 GeV can be excluded by the XENON-1T (2017) limits while the survivied parameter space below 6 GeV can be fully covered by the future germanium-based light dark matter detections (such as CDEX), by the Higgs coupling precison measurements or by the production process e+e−→hAe^+e^- \to hA at an electron-positron collider (Higgs factory).Comment: 15 pages, 5 figures. Discussions and references added, version accepted by PL

    Narrow line width frequency comb source based on an injection-locked III–V-on-silicon mode-locked laser

    Get PDF
    In this paper, we report the optical injection locking of an L-band (similar to 1580 nm) 4.7 GHz III-V-on-silicon mode-locked laser with a narrow line width continuous wave (CW) source. This technique allows us to reduce the MHz optical line width of the mode-locked laser longitudinal modes down to the line width of the source used for injection locking, 50 kHz. We show that more than 50 laser lines generated by the mode-locked laser are coherent with the narrow line width CW source. Two locking techniques are explored. In a first approach a hybrid mode-locked laser is injection-locked with a CW source. In a second approach, light from a modulated CW source is injected in a passively mode-locked laser cavity. The realization of such a frequency comb on a chip enables transceivers for high spectral efficiency optical communication. (C) 2016 Optical Society of Americ

    Simplified TeV leptophilic dark matter in light of DAMPE data

    Full text link
    Using a simplified framework, we attempt to explain the recent DAMPE cosmic e++e−e^+ + e^- flux excess by leptophilic Dirac fermion dark matter (LDM). The scalar (Φ0\Phi_0) and vector (Φ1\Phi_1) mediator fields connecting LDM and Standard Model particles are discussed. Under constraints of DM relic density, gamma-rays, cosmic-rays and Cosmic Microwave Background (CMB), we find that the couplings P⊗SP \otimes S, P⊗PP \otimes P, V⊗AV \otimes A and V⊗VV \otimes V can produce the right bump in e++e−e^+ + e^- flux for a DM mass around 1.5 TeV with a natural thermal annihilation cross-section ∼3×10−26cm3/s \sim 3 \times 10^{-26} cm^3/s today. Among them, V⊗VV \otimes V coupling is tightly constrained by PandaX-II data (although LDM-nucleus scattering appears at one-loop level) and the surviving samples appear in the resonant region, mΦ1≃2mχm_{\Phi_1} \simeq 2m_{\chi}. We also study the related collider signatures, such as dilepton production pp→Φ1→ℓ+ℓ−pp \to \Phi_1 \to \ell^+\ell^-, and muon g−2g-2 anomaly. Finally, we present a possible U(1)XU(1)_X realization for such leptophilic dark matter.Comment: discussions added, version accepted by JHE

    Propriété en modulation de laser Fabry-Perot verrouillé en longueur d'onde par injection optique

    No full text
    Session affiches 11 « Amplificateurs et Lasers à semi-conducteurs » [A2.1]National audienceUn laser Fabry-Perot fonctionnant en régime monomode grâce au verrouillage en longueur d'onde par injection optique est caractérisé sous modulation directe. Nous démontrons expérimentalement la dépendance de la réponse en régime petit signal et du facteur de couplage phase-amplitude en fonction de la puissance optique injectée

    28 Gb/s direct modulation heterogeneously integrated C-band InP/SOI DFB laser

    Get PDF
    We demonstrate direct modulation of a heterogeneously integrated C-band DFB laser on SOI at 28 Gb/s with a 2 dB extinction ratio. This is the highest direct modulation bitrate so far reported for a membrane laser coupled to an SOI waveguide. The laser operates single mode with 6 mW output power at 100 mA bias current. The 3 dB modulation bandwidth is 15 GHz. Transmission experiments using a 2 km non zero dispersion shifted single mode fiber were performed at 28 Gb/s bitrate using a 2(7)-1 NRZ-PRBS pattern resulting in a 1 dB power penalty. (C) 2015 Optical Society of Americ
    • …
    corecore