孤子-反孤子双夸克对薄壁的变化如何表明爱因斯坦常数主导宇宙学和额外维在新宇宙初始成核中的作用
How the alteration of a thin wall for soliton-anti soliton di quark pairs signifies an Einstein constant dominated cosmology and a role for Extra dimensions in initial nucleation of a new universe
摘要：
我们使用作为一个新的宇宙的成核如何发生的模型，假设一个标量场的孤子反孤子组成部分的双夸克标识。我们构建了一个模型，显示从暗物质暗能量混合到纯宇宙学常数宇宙学的演化，由于所产生的标量场的图的斜率的变化。初始势系统是半经典的，在混沌暴胀结束时成为非经典的，同时宇宙膨胀由爱因斯坦宇宙学常数控制。我们使用谢勒推导的声速为零，在初始暴胀宇宙学和改变它之后的标量场的斜率远离薄壁近似。此外，秦波关于暗物质的额外维度的文章中的结果允许我们显示维度对暴胀模型的半经典近似规则的影响。我们的结论是，新的力定律指定的薄秦和额外的维度将在早期宇宙中发挥作用，是非常重要的暴胀膨胀由于双夸克对成核的孤子反孤子配置的开始。
英文摘要：
We use as a model of how nucleation of a new universe occurs, assuming a di quark identification for soliton-anti soliton constituent parts of a scalar field. We construct a model showing evolutin from a dark matter dark energy mix to a pure cosmological constant cosmology due to changes in the slope of a graph of the resulting scalar field. The initial potential system employed is semi classical in nature, becoming non classical at the end of chaotic inflation at the same time cosmological expansion is dominated by the Einstein cosmological constant. We use Scherrer's derivation of a sound speed being zero during initial inflationary cosmology and change it afterwards as the slope of the scalar field moves away from a thin wall approximation. Furthermore, the results in Bo Qin's article about extra dimensions from dark matter, permit us to show the impact of dimensionality upon the rule of semi classical approximations to inflation models. We conclude that the new force law specified by Bo Qin and additional dimensions would play a role in the early universe and be extremely important to the onset of inflationary expansion due to nucleation of di quark pairs in a soliton-anti soliton configuration.
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