有限泡统计 约束 后期宇宙学阶段过渡
Gilly Elor1, Ryusuke Jinno2,3, Soubhik Kumar4,5,6
1Weinberg Institute, Department of Physics, <a href="https://ror.org/00hj54h04">University of Texas at Austin</a>, Austin, Texas 78712, USA.
Physical review letters
|December 6, 2024
概括
这项研究探讨了宇宙相位过渡,揭示了泡核的波动如何产生普遍曲率波动. 这些发现限制了暗部门相位过渡,比目前的中微子测量提供了更强大的极限.
科学领域:
- 宇宙学的宇宙学是什么?
- 粒子物理学 粒子物理学
- 天体物理学 天体物理学
背景情况:
- 晚期的第一阶层宇宙阶段转换 (PTs) 在标准模型温度以下发生.
- 在这些PT中,随机气泡核化会在完成时间中产生超视界波动.
研究的目的:
- 计算这些波动是如何产生普遍曲率波动的.
- 通过使用观测数据,限制黑暗部门PT中释放的能量.
主要方法:
- 分析随机泡核形成的超视界波动.
- 利用宇宙微波背景 (CMB) 和大规模结构测量限制.
- 与现有边界 (例如,ΔNeff) 和未来预测 (例如,CMB-S4) 进行比较.
主要成果:
- 在PT完成时间的波动是普遍源曲率波动.
- 对于0.1 eVT_{PT}keV的温度来说,暗板PT能量释放的限制得到了推导.
- 这些约束比当前的 ΔNeff 极限和一些 CMB-S4 预测更为严格.
结论:
- 这项研究提供了一种通过引力效应探测早期宇宙物理学的新方法.
- 未来的CMB光谱扭曲和脉冲星计时阵列将为更高的PT温度 (keVT_{PT}GeV) 提供竞争性的灵敏度.
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