5,940 research outputs found

    Magnetic moments of the spin-32{3\over 2} doubly heavy baryons

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    In this work, we investigate the chiral corrections to the magnetic moments of the spin-323\over 2 doubly charmed baryons systematically up to next-to-next-to-leading order with the heavy baryon chiral perturbation theory. The numerical results are given up to next-to-leading order: μΞcc∗++=1.72μN\mu_{\Xi^{*++}_{cc}}=1.72\mu_{N}, μΞcc∗+=−0.09μN\mu_{\Xi^{*+}_{cc}}=-0.09\mu_{N}, μΩcc∗+=0.99μN\mu_{\Omega^{*+}_{cc}}=0.99\mu_{N}. As a by-product, we have also calculated the magnetic moments of the spin-323\over 2 doubly bottom baryons and charmed bottom baryons: μΞbb∗0=0.63μN\mu_{\Xi^{*0}_{bb}}=0.63\mu_{N}, μΞbb∗−=−0.79μN\mu_{\Xi^{*-}_{bb}}=-0.79\mu_{N}, μΩbb∗−=0.12μN\mu_{\Omega^{*-}_{bb}}=0.12\mu_{N}, μΞbc∗+=1.12μN\mu_{\Xi^{*+}_{bc}}=1.12\mu_{N}, μΞbc∗0=−0.40μN\mu_{\Xi^{*0}_{bc}}=-0.40\mu_{N}, μΩbc∗0=0.56μN\mu_{\Omega^{*0}_{bc}}=0.56\mu_{N}.Comment: 10 pages,2 figures. arXiv admin note: text overlap with arXiv:1707.02765. Replace the published versio

    Radiative decays of the doubly charmed baryons in chiral perturbation theory

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    We have systematically investigated the spin-32\frac{3}{2} to spin-12\frac{1}{2} doubly charmed baryon transition magnetic moments to the next-to-next-to-leading order in the heavy baryon chiral perturbation theory (HBChPT). Numerical results of transition magnetic moments and decay widths are presented to the next-to-leading order: μΞcc∗++→Ξcc++=−2.35μN\mu_{\Xi_{cc}^{*++}\rightarrow\Xi_{cc}^{++}}=-2.35\mu_{N}, μΞcc∗+→Ξcc+=1.55μN\mu_{\Xi_{cc}^{*+}\rightarrow\Xi_{cc}^{+}}=1.55\mu_{N}, μΩcc∗+→Ωcc+=1.54μN\mu_{\Omega_{cc}^{*+}\rightarrow\Omega_{cc}^{+}}=1.54\mu_{N}, ΓΞcc∗++→Ξcc++=22.0\Gamma_{\Xi_{cc}^{*++}\rightarrow\Xi_{cc}^{++}}=22.0 keV, ΓΞcc∗+→Ξcc+=9.57\Gamma_{\Xi_{cc}^{*+}\rightarrow\Xi_{cc}^{+}}=9.57 keV, ΓΩcc∗+→Ωcc+=9.45\Gamma_{\Omega_{cc}^{*+}\rightarrow\Omega_{cc}^{+}}=9.45 keV.Comment: arXiv admin note: text overlap with arXiv:1707.02765, arXiv:1706.0645

    Distributed Power-Line Outage Detection Based on Wide Area Measurement System

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    In modern power grids, the fast and reliable detection of power-line outages is an important functionality, which prevents cascading failures and facilitates an accurate state estimation to monitor the real-time conditions of the grids. However, most of the existing approaches for outage detection suffer from two drawbacks, namely: (i) high computational complexity; and (ii) relying on a centralized means of implementation. The high computational complexity limits the practical usage of outage detection only for the case of single-line or double-line outages. Meanwhile, the centralized means of implementation raises security and privacy issues. Considering these drawbacks, the present paper proposes a distributed framework, which carries out in-network information processing and only shares estimates on boundaries with the neighboring control areas. This novel framework relies on a convex-relaxed formulation of the line outage detection problem and leverages the alternating direction method of multipliers (ADMM) for its distributed solution. The proposed framework invokes a low computational complexity, requiring only linear and simple matrix-vector operations. We also extend this framework to incorporate the sparse property of the measurement matrix and employ the LSQRalgorithm to enable a warm start, which further accelerates the algorithm. Analysis and simulation tests validate the correctness and effectiveness of the proposed approaches
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