33,207 research outputs found

    On Structure of cluster algebras of geometric type I: In view of sub-seeds and seed homomorphisms

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    Our motivation is to build a systematic method in order to investigate the structure of cluster algebras of geometric type. The method is given through the notion of mixing-type sub-seeds, the theory of seed homomorphisms and the view-point of gluing of seeds. As an application, for (rooted) cluster algebras, we completely classify rooted cluster subalgebras and characterize rooted cluster quotient algebras in detail. Also, we build the relationship between the categorification of a rooted cluster algebra and that of its rooted cluster subalgebras. Note that cluster algebras of geometric type studied here are of the sign-skew-symmetric case.Comment: 41 page

    Search for a heavy dark photon at future e+ee^+e^- colliders

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    A coupling of a dark photon AA' from a U(1)AU(1)_{A'} with the standard model (SM) particles can be generated through kinetic mixing represented by a parameter ϵ\epsilon. A non-zero ϵ\epsilon also induces a mixing between AA' and ZZ if dark photon mass mAm_{A'} is not zero. This mixing can be large when mAm_{A'} is close to mZm_Z even if the parameter ϵ\epsilon is small. Many efforts have been made to constrain the parameter ϵ\epsilon for a low dark photon mass mAm_{A'} compared with the ZZ boson mass mZm_Z. We study the search for dark photon in e+eγAγμ+μe^+e^- \to \gamma A' \to \gamma \mu^+ \mu^- for a dark photon mass mAm_{A'} as large as kinematically allowed at future e+ee^+e^- colliders. For large mAm_{A'}, care should be taken to properly treat possible large mixing between AA' and ZZ. We obtain sensitivities to the parameter ϵ\epsilon for a wide range of dark photon mass at planed e+  ee^+\;e^- colliders, such as Circular Electron Positron Collider (CEPC), International Linear Collider (ILC) and Future Circular Collider (FCC-ee). For the dark photon mass 20 GeVmA330 GeV20~\text{GeV}\lesssim m_{A^{\prime}}\lesssim 330~\text{GeV}, the 2σ2\sigma exclusion limits on the mixing parameter are ϵ103102\epsilon\lesssim 10^{-3}-10^{-2}. The CEPC with s=240 GeV\sqrt{s}=240~\text{GeV} and FCC-ee with s=160 GeV\sqrt{s}=160~\text{GeV} are more sensitive than the constraint from current LHCb measurement once the dark photon mass mA50 GeVm_{A^{\prime}}\gtrsim 50~\text{GeV}. For mA220 GeVm_{A^{\prime}}\gtrsim 220~\text{GeV}, the sensitivity at the FCC-ee with s=350 GeV\sqrt{s}=350~\text{GeV} and 1.5 ab11.5~\text{ab}^{-1} is better than that at the 13~TeV LHC with 300 fb1300~\text{fb}^{-1}, while the sensitivity at the CEPC with s=240 GeV\sqrt{s}=240~\text{GeV} and 5 ab15~\text{ab}^{-1} can be even better than that at 13~TeV LHC with 3 ab13~\text{ab}^{-1} for mA180 GeVm_{A^{\prime}}\gtrsim 180~\text{GeV}.Comment: 21 pages, 5 figures, 2 table

    Contagion on complex networks with persuasion

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    The threshold model has been widely adopted as a classic model for studying contagion processes on social networks. We consider asymmetric individual interactions in social networks and introduce a persuasion mechanism into the threshold model. Specifically, we study a combination of adoption and persuasion in cascading processes on complex networks. It is found that with the introduction of the persuasion mechanism, the system may become more vulnerable to global cascades, and the effects of persuasion tend to be more significant in heterogeneous networks than those in homogeneous networks: a comparison between heterogeneous and homogeneous networks shows that under weak persuasion, heterogeneous networks tend to be more robust against random shocks than homogeneous networks; whereas under strong persuasion, homogeneous networks are more stable. Finally, we study the effects of adoption and persuasion threshold heterogeneity on systemic stability. Though both heterogeneities give rise to global cascades, the adoption heterogeneity has an overwhelmingly stronger impact than the persuasion heterogeneity when the network connectivity is sufficiently dense.Comment: 12 pages, 7 figure
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