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首页> 外文期刊>International journal of modern physics, D. Gravitation, astrophysics, cosmology >WMAPing the Universe: Supersymmetry, dark matter, dark energy, proton decay and collider physics [Review]
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WMAPing the Universe: Supersymmetry, dark matter, dark energy, proton decay and collider physics [Review]

机译:WMAP宇宙:超对称,暗物质,暗能量,质子衰减和对撞机物理学[评论]

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摘要

In this review we critically discuss constraints on minimal supersymmetric models of particle physics as implied by the recent astrophysical observations of WMAP satellite experiment. Although the prospects of detecting supersymmetry increase dramatically, at least within the context of the minimal models, and 90% of the available parameter space can safely be reached by the sensitivity of future colliders, such as Tevatron, LHC and linear colliders, nevertheless we pay particular emphasis on discussing regions of the appropriate phase diagrams, which - if realized in nature - would imply that detection of supersymmetry, at least in the context of minimal models, could be out of colliders reach. We also discuss the importance of a precise determination of the radiative corrections to the muon anomalous magnetic moment, gmu - 2, both theoretically and experimentally, which could lead to elimination of such "out of reach" regions in case of a confirmed discrepancy of gmu - 2 from the standard model value. Finally, we briefly commend upon recent evidence, supported by observations, on a dark energy component of the Universe, of as yet unknown origin, covering 73% of its energy content. To be specific, we discuss how supergravity quintessence (relaxation) models can be made consistent with recent observations, which may lead to phenomenologically correct constrained supersymmetric models, accounting properly for this dark energy component. We also outline their unresolved problems. [References: 311]
机译:在这篇综述中,我们严格地讨论了WMAP卫星实验的最新天体观测所隐含的对粒子物理学的最小超对称模型的约束。尽管检测超对称性的前景急剧增加,但至少在最小模型的背景下,未来的对撞机(如Tevatron,LHC和线性对撞机)的灵敏度可以安全地达到90%的可用参数空间,但是我们还是要付出代价特别强调要讨论适当相图的区域,如果本质上实现,则意味着至少在最小模型的情况下,超对称性的检测可能超出对撞机的范围。我们还将讨论从理论上和实验上精确确定辐射校正对μ子异常磁矩gmu-2的重要性,这在确定gmu差异的情况下可以消除此类“无法到达”的区域-标准模型值中的2。最后,我们简短地赞扬来自宇宙的暗能量成分的最新证据,这些证据得到了观测的支持,该成分至今尚不为人所知,覆盖了其能量含量的73%。具体来说,我们讨论了如何使超重力典型(松弛)模型与最近的观测结果相一致,这可能导致从现象学上正确的约束超对称模型,并适当地考虑了这种暗能量成分。我们还概述了他们尚未解决的问题。 [参考:311]

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