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Lowest Order Mass of KK Graviton Revisited and How It May Affect the Blue Spectrum for Gravitons

机译:重新讨论了最低订单大量KK格雷顿,以及如何影响着名格琴的蓝色光谱

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The lowest order mass for a KK graviton, as a non-zero product of two branes interacting via a situation similar to Steinhardt’s ekpyrotic universe is obtained, as to an alternative to the present dogma specifying that gravitons must be massless. The relative positions as to the branes give a dynamical picture as to how lowest order KK gravitons could be affected by contraction and then subsequent expansion. Initially we have bulk gravitons as a vacuum state. The massless condition is just one solution to a Stern Liuouville operator equation we discuss, which with a non-zero lowest order mass for a KK graviton permits modeling of gravitons via a dynamical Casmir effect which we generalize using Ruser and Duerrer’s 2007 work. In particular the blue spectrum for (massless gravitons), is revisited, with consequences for observational astrophysics.
机译:KK Graviton的最低订单质量,作为通过类似于Steinhardt的Ekpyric Unkers的情况交互的两个布兰斯的非零产物,对于目前的教条来说,指定的替代品必须是无麻环的。关于布兰斯的相对位置给出了动态图片,至于最低的阶KK引人注目的影响,然后随后的扩展。最初,我们将散装格子作为真空状态。无阻塞的条件只是我们讨论的斯特恩·普鲁维尔操作员方程的一种解决方案,我们讨论的是KK Graviton的非零阶质量允许通过使用Ruser和Duerrer 2007的工作概括的动态Casmir效果建模引人注目。特别是对(无阻比者)的蓝色光谱被重新审视,并且对观察天体物理学产生后果。

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