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arXiv 1012.2954hep-phgr-qc
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在TeV-scale重力下等离子体引力子的产生

Plasma graviton production in TeV-scale gravity

E. Yu. Melkumova

摘要:

在TeV尺度引力的ADD模型中,发展了经典等离子体与Kaluza-Klein(KK)引力子相互作用的理论。在动力学方法中,等离子体被描述为带电粒子和麦克斯韦场都被限制在膜上的系统。在线性化理论中引入了与生活在大体积中的多维引力和$n$紧致额外维的相互作用。考虑等离子体集体效应,通过等离子体能量动量张量涨落的两点关联函数计算了KK引力子发射率。除了已知的机制(如韧致辐射和重力-普里马科夫效应),我们发现基本上集体渠道,如凝聚的等离子体波引力子可能会表现在湍流等离子体。我们的结果表明,通常使用的速率的KK引力子生产的恒星和超新星可能被低估。

英文摘要:

We develop the theory of interaction of classical plasma with Kaluza-Klein (KK) gravitons in the ADD model of TeV-scale gravity. Plasma is described within the kinetic approach as the system of charged particles and Maxwell field both confined on the brane. Interaction with multidimensional gravity living in the bulk with $n$ compact extra dimensions is introduced within the linearized theory. The KK gravitons emission rates are computed taking into account plasma collective effects through the two-point correlation functions of the fluctuations of the plasma energy-momentum tensor. Apart from known mechanisms (such as bremsstrahlung and gravi-Primakoff effect) we find essentially collective channels such as the coalescence of plasma waves into gravitons which may be manifest in turbulent plasmas. Our results indicate that commonly used rates of the KK gravitons production in stars and supernovae may be underestimated.

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