扩张的介质中的相位过渡:热残留物
Romuald A Janik1, Matti Järvinen2,3, Jacob Sonnenschein4
1Jagiellonian University, Institute of Theoretical Physics and Mark Kac Center for Complex Systems Research, Łojasiewicza 11, 30-348 Kraków, Poland.
Physical review letters
|August 12, 2025
概括
我们研究了膨胀宇宙中的相位过渡. 热等离子体残留物持续存在,抵御冷却和泡核形成,即使在宇宙膨胀下.
科学领域:
- 高能物理 高能物理
- 宇宙学的宇宙学是什么?
- 量子场理论 量子场理论
背景情况:
- 了解早期宇宙需要研究不断膨胀的介质中的相位过渡.
- 全息模型为强合的量子场理论提供了洞察力.
研究的目的:
- 分析扩张系统中封闭-解封阶段过渡的动态.
- 为了研究在膨胀过程中热等离子体残余的行为.
主要方法:
- 使用有效的边界描述.
- 将描述与全息Witten模型相匹配.
- 在提升不变和宇宙膨胀场景中模拟动态.
主要成果:
- 观察到持久的热血残留物没有降温.
- 尽管系统扩张,这些残留物抵御了泡核形成.
- 在不同的膨胀模型中,残留物收缩,溶解和重新加热的动力学是强大的.
结论:
- 热等离子体残留物在膨胀过程中表现出稳定的行为,挑战了典型的相位过渡期望.
- 这些发现在Minkowski和Friedmann-Robertson-Walker时空中都是一致的.
- 这种强度表明,在不断膨胀的宇宙中,这些残留物具有基本的特性.
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