欧洲脉冲星计时阵列的第二次数据发布:挑战超轻暗物质范式
Clemente Smarra1,2, Boris Goncharov3,4, Enrico Barausse1,2
1SISSA-International School for Advanced Studies, Via Bonomea 265, 34136, Trieste, Italy and INFN, Sezione di Trieste.
Physical review letters
|November 13, 2023
概括
欧洲脉冲星计时阵列数据显示,超轻的暗物质粒子无法完全解释银河系的暗物质. 这些具有特定质量的粒子被迫具有最大的局部密度.
科学领域:
- 天体物理学 天体物理学
- 粒子物理学 粒子物理学
- 宇宙学的宇宙学是什么?
背景情况:
- 脉冲星定时阵列 (PTA) 实验利用毫秒无线电脉冲星来检测微妙的时间变化.
- 超轻尺度或伪尺度粒子是假设的暗物质候选者.
- 引力相互作用是暗物质对重子物质影响的假设机制.
研究的目的:
- 使用脉冲星计时数据限制超轻暗物质粒子的特性.
- 为了测试这些粒子构成局部暗物质全部的假设.
主要方法:
- 分析欧洲脉冲计时阵列 (EPTA) 的第二次数据发布.
- 专注于黑暗物质仅通过重力相互作用的场景.
- 利用来自银河系毫秒脉冲星集团的十年时间数据.
主要成果:
- 质量在10^{-24.0} eV和10^{-23.3} eV之间的超轻粒子不能占当地暗物质密度的100%.
- 这些颗粒的最大允许局部密度被限制为小于或等于0.3 GeV/cm3.
结论:
- 根据EPTA的数据,超轻暗物质模型面临显著的限制.
- 这些发现排除了暗物质的某些质量范围,如果它仅由这些粒子组成.
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