Randall-Sundrum膜世界有效势如何影响暴胀物理
How a Randall-Sundrum Brane-World Effective Potential Influences Inflation Physics
摘要：
在弦论中，即使存在10的1000次方的真空态，暴胀是否会产生压倒性的一种首选真空态？我们肯定地回答的问题，是否存在的引力子生产是确认使用目前的检测方法。我们使用一个扩展的Randall-Sundrum膜世界有效势作为与暴胀二次势一致的起始势。这发生在Bogomolnyi不等式消除了对轴子壁质量高温相关消失的特设假设的需要之后。引力子的产生与一个五维膜世界负宇宙学常数和一个四维正值宇宙学常数有着明确的联系，它们的温度依赖性允许早期宇宙引力子产生活动的爆发。我们展示了双夸克，波函数，和各种几何形式tien到惠勒-德威特方程。这允许调查一个离散的量子反弹和一个可能的链接到当前宇宙的演化的初始阶段，作为一个逆之前宇宙的坍缩反弹点的初始起点暴胀膨胀。这为实际研究引力子作为空间推进系统的一部分提供了可能性，并解决了由一束重力波引起的问题，这将产生一个g力，因为大地结构是近场的。它可以应用于现有的和新的空间推进概念。
英文摘要：
In string theory, even when there are ten to the thousand power vacuum states, does inflation produce overwhelmingly one preferred type of vacuum state? We respond affirmatively to questions whether existence of graviton production is confirmable using present detector methodology. We use an explcity Randall-Sundrum brane world effective potential as congruent with an inflationary quadratic potential start. This occurs after the Bogomolnyi inequality eliminates the need for the ad hoc assumption of axion wall mass high temperature related dissapearance. Graviton production has explicit links with a five-dimensional brane-world negavit cosmological constant and a four dimensional positive valued cosmological constant, whose temperature dependence permits an early universe graviton production activyt burst. We show how di quarks, wave functions, and various geometrical forms tien into the WHeeler-De Witt equation. This permits investigating a discrete quantum bounce and a possible link to the initial phase of the present universe's evolution as a converse to a prior universe's collapse to the bounce point-the initial starting point to inflationary expansion. This opens a possibility of realstically investigating gravitons as part of a space propusion systme and deal iwth problems resulting from a beam of gravity waves, which would create a g-force because the geodestic structure is near field. It can be applied to existing and to new space propulsion concepts.
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