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Supersymmetric large extra dimensions and the cosmological constant: an update

机译:超对称超大尺寸和宇宙常数:更新

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This article critically reviews the proposal for addressing the cosmological constant problem within the framework of supersymmetric large extra dimensions (SLED), as recently proposed in hep-th/0304256. After a brief restatement of the cosmological constant problem, a short summary of the proposed mechanism is given. The emphasis is on the perspective of the low-energy effective theory in order to see how it addresses the problem of why low-energy particles like the electron do not contribute too large a vacuum energy. This is followed by a discussion of the main objections, which are grouped into the following five topics: (1) Weinberg's No-Go Theorem. (2) Are hidden Innings of the theory required, and are these stable under renormalization? (3) Why should the mechanism apply only now and not rule out possible earlier epochs of inflationary dynamics? (4) How big are quantum effects, and which are the most dangerous? and (5) Even if successful, can the mechanism be consistent with cosmological or current observational constraints? It is argued that there are plausible reasons why the mechanism can thread the potential objections, but that a definitive proof that it does depends on addressing well-defined technical points. These points include identifying what fixes the size of the extra dimensions, checking how topological obstructions renormalize and performing specific calculations of quantum corrections. More detailed studies of these issues, which are well within reach of our present understanding of extra-dimensional theories, are currently underway. As such, the jury remains out concerning the proposal, although the prospects for acquittal still seem good. (An abridged version of this article appears in the proceedings of SUSY 2003.) (C) 2004 Elsevier Inc. All rights reserved.
机译:本文严格审查了在hepth / 0304256中提出的在超对称大尺寸(SLED)框架内解决宇宙常数问题的建议。在简短地重述了宇宙常数问题之后,对所提出的机制作了简短的总结。重点是从低能效理论的角度出发,以了解它如何解决为什么像电子这样的低能粒子不会贡献太大的真空能的问题。接下来是对主要反对意见的讨论,这些反对意见分为以下五个主题:(1)温伯格的“不行定理”。 (2)是否需要理论的隐藏因果,并且在重新归一化后这些因果是否稳定? (3)为什么该机制应仅在现在应用,而不排除通货膨胀动态的更早时期? (4)量子效应有多大,哪个最危险? (5)即使成功,该机制是否也符合宇宙学或当前的观测限制?有人认为,该机制可以提出潜在反对意见的理由很合理,但它确实有确凿的证据取决于解决明确定义的技术要点。这些要点包括确定什么可以固定额外尺寸的大小,检查拓扑障碍物如何重新规范化以及执行量子校正的特定计算。目前正在对这些问题进行更详细的研究,而这正是我们目前对超维理论的理解。因此,尽管有无罪开释的前景似乎仍然不错,但陪审团仍未就该提案作出决定。 (本文的节略版本出现在SUSY 2003的会议记录中。)(C)2004 Elsevier Inc.保留所有权利。

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