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大爆炸后的中微子混合的暗辐射核合成
Daniel Aloni1,2, Melissa Joseph1, Martin Schmaltz1,3
1Physics Department, Boston University, Boston, Massachusetts 02215, USA.
Physical review letters
|December 15, 2023
概括
浅暗费米子可以与标准模型中微子相互作用,可能在早期宇宙中平衡. 这一过程发生在黑暗费米子质量附近,影响宇宙进化,并为宇宙学紧张局势提供解决方案.
科学领域:
- 粒子物理学 粒子物理学
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
背景情况:
- 标准模型 (SM) 中微子可以与明暗费米子相互作用.
- 这些相互作用可以通过振荡和散射导致早期宇宙的平衡.
- 暗费米子相互作用在高温下抑制生产,但在晚些时候增强它.
研究的目的:
- 研究光暗费米子与SM中微子平衡的条件和影响.
- 探索黑暗部门动态在宇宙学可观测物上的潜在可观测印记.
- 评估这些暗费米子对当前宇宙学张力 (H0和S8) 的相关性.
主要方法:
- 对黑色费米子质量与SM中微子混合的分析.
- 通过振荡和散射来建模平衡过程.
- 检查温度依赖的相互作用对生产率的影响.
主要成果:
- 在广泛的参数中,平衡发生在黑暗费米子质量附近.
- 对于低于MeV的质量,平衡自然发生在核合成后.
- 这种晚期平衡为宇宙微波背景 (CMB) 和大规模结构上可观测的印记打开了道路.
结论:
- 浅暗费米子提供了一个可行的暗部门,具有可观测的后果.
- 拟议的机制为哈勃 (H0) 和S8张力提供了潜在的分辨率.
- 进一步的研究可以探索CMB和大规模结构调查的详细预测.
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