微米到比科米的领先边界是来自中子星冷却的第五种力
Damiano F G Fiorillo1, Alessandro Lella2,3, Ciaran A J O'Hare4
1Deutsches Elektronen-Synchrotron DESY, Platanenallee 6, 15738 Zeuthen, Germany.
Physical review letters
|December 5, 2025
概括
新的研究使用中子星冷却来限制假设的标量粒子. 这些发现排除了以前未经验证的合,大大推进了超越标准模型的新物理学的搜索.
科学领域:
- 粒子物理学 粒子物理学
- 天体物理学 天体物理学
- 引力物理 引力物理
背景情况:
- 同等性原理和反正方体引力定律可能会被短距离的标量粒子违反.
- 这些假设的标量体与核子配对,其质量在EV到MeV范围内.
研究的目的:
- 为了在这些标量粒子的存在上建立严格的界限.
- 研究中子星 (NS) 冷却的潜力,作为一种限制这些粒子的方法.
主要方法:
- 分析了附近孤立中子星的冷却数据.
- 将导出的极限与现有的极限进行比较,例如超新星 (SN) 1987A.的极限.
主要成果:
- 中子星的冷却提供了最严格的限制在尺度合 (gN 5×10^{-14}) 跨越6个数量级的质量 (mφ).
- 尺度发射率显著增强了冷中子星的冷却.
- 这些结果也限制了希格斯门户模型,限制了标量-希格斯混合角度 (sinθ 6×10^{-11}).
结论:
- 观察到的中子星冷却数据排除了这些奇特的标量粒子的存在.
- 这项研究为标量粒子和希格斯门户模型建立了新的,更高的极限,超越了以前的约束.
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