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arXiv 1007.4126gr-qcmath-phmath.MP
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介绍第二次大挑战研讨会-宇宙学理解的大挑战:引力,暗物质和暗能量。走向新的场景

Presentation of the Second Big Challenge Symposium - The Big Challenge of Cosmological Understanding: Gravitation, Dark Matter and Dark Energy. Towards New Scenarios

Christian Corda

摘要:

本次研讨会是专门为列夫·考夫曼的记忆,6月17日至1957年11月12日至2009年。宇宙的加速膨胀,这是今天观察到的,表明宇宙动力学是由所谓的暗能量场提供了一个大的负压占主导地位。这是一幅标准图,其中这种新成分被认为是场方程右边的一个源。它应该是某种形式的非聚集的非零真空能量,与聚集的暗物质一起驱动着全球动力学。这就是所谓的“和谐模型”(ACDM),它与宇宙微波背景辐射(CMBR)、昏暗莱曼极限系统(LLS)和Ia型超新星(SNeIa)数据相一致,为理解今天观测到的宇宙提供了一个很好的框架。但是,它也存在一些缺点,如著名的“符合”和“宇宙学常数“问题。另一种方法是更好地理解广义相对论中的能量概念,并改变场方程的左侧,并检查所观察到的宇宙动力学是否可以通过扩展广义相对论来实现。在这种不同的背景下,我们不需要去寻找暗能量和暗物质的候选者,因为到目前为止还没有发现它们,而只需要站在“观测到的”成分上:曲率和重子物质,来解释观测结果。考虑到这个观点,我们可以认为引力不是标度不变的。本次研讨会的目的是获得一个挂毯的理论和观测有关引力和暗宇宙的现状。

英文摘要:

This Symposium is devoted to the Memory of Lev Kofman, June-17-1957-November-12-2009. The accelerated expansion of the Universe, which is today observed, shows that cosmological dynamics is dominated by the so-called Dark Energy field which provides a large negative pressure. This is the standard picture, in which such new ingredient is considered as a source of the right hand side of the field equations. It should be some form of non-clustered non-zero vacuum energy which, together with the clustered Dark Matter, drives the global dynamics. This is the so-called "concordance model" (ACDM) which gives, in agreement with the Cosmic Microwave Background Radiation (CMBR), dim Lyman Limit Systems (LLS) and type la supernovae (SNeIa) data, a good framework to understand the today observed Universe. However, it presents several shortcomings as the well known "coincidence" and "cosmological constant" problems . An alternative approach is to have a better understanding of the energy concept in General Relativity and also to change the left hand side of the field equations, and check if observed cosmic dynamics can be achieved by extending general relativity. In this different context, it is not required to search candidates for Dark Energy and Dark Matter, which till now have not been found. Rather, one can only stand on the "observed" ingredients: curvature and baryon matter, to account for the observations. Considering this point of view, one can think of that gravity is not scale-invariant. The goal of this Symposium is to obtain a tapestry of the present status of theory and observations concerning Gravitation and Dark Universe.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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