论文标题
来自天体物理黑洞的超轻骨化场质量边界
Ultralight Bosonic Field Mass Bounds from Astrophysical Black Hole Spin
论文作者
论文摘要
在重力波天文学的新时代，黑洞的测量已从二进制黑洞合并的新时代天文学中显着增长。到目前为止，尚未观察到的大型超轻质骨气场代表了标准模型扩展的最令人兴奋的特征之一，能够为粒子物理和宇宙学中众多范式问题提供解决方案。在这项工作中，我们探索了从旋转天体物理黑洞以及它们的角动量能量转移到玻色晶冷凝物中的范围，这些凝管可以通过超级助力不稳定性形成黑洞周围。使用最新的分析结果，我们通过大量的黑洞参数测量集合进行了简化的分析，在其中我们发现超级良好通常排除了质量范围中的玻感场； spin-0：$ {\ scriptsizize \ {3.8 \ times10^{ - 14} \ {\ rm ev} \ leq leq leqμ_0\ leq 3.4 \ leq 3.4 \ times10^{ - 11}} \ rm ev} 1.3 \ times10^{ - 16} \ {\ rm ev}，2.5 \ times10^{ - 21}} \ {\ rm ev} \ leqμ_0\ leq leq 1.2 \ leq times10^{ - 20} { - 20} \ { 6.2\times10^{-15}\ {\rm eV} \leq μ_1 \leq 3.9\times10^{-11}\ {\rm eV}, 2.8\times10^{-22}\ {\rm eV} \leq μ_1 \leq 1.9\times10^{-16}\ {\rm ev} \}} $ and spin-2：$ {\ scriptSize \ {2.2 \ times10^{ - 14} \ {\ rm ev} \ leq leq leqμ_2\ leq 2.8 \ times10^{ - 11}} μ_2\ leq 1.8 \ times10^{ - 16} \ {\ rm ev}，6.4 \ times10^{ - 22} \ {\ rm ev} \ rm ev} \ leqμ_2\ leq 7.7 \ leq 7.7 \ times10^{ - 21}} { - 21}}} \ rm ev} $ gimeritive。我们还在特定现象学模型的背景下探索了这些界限，特别是QCD轴，M理论模型和模糊的暗物质位于当前限制的边缘。特别是，我们包括对事件GW190521和M87*的最新测量结果，用于限制轴线等磁场的质量和衰减常数。最后，我们评论了SPIN-0和SPIN-1病例的一系列字段的简单示例。
Black Hole measurements have grown significantly in the new age of gravitation wave astronomy from LIGO observations of binary black hole mergers. As yet unobserved massive ultralight bosonic fields represent one of the most exciting features of Standard Model extensions, capable of providing solutions to numerous paradigmatic issues in particle physics and cosmology. In this work we explore bounds from spinning astrophysical black holes and their angular momentum energy transfer to bosonic condensates which can form surrounding the black hole via superradiant instabilities. Using recent analytical results we perform a simplified analysis with a generous ensemble of black hole parameter measurements where we find superradiance very generally excludes bosonic fields in the mass ranges; spin-0: ${\scriptsize \{ 3.8\times10^{-14}\ {\rm eV} \leq μ_0 \leq 3.4\times10^{-11}\ {\rm eV}, 5.5\times10^{-20}\ {\rm eV} \leq μ_0 \leq 1.3\times10^{-16}\ {\rm eV}, 2.5\times10^{-21}\ {\rm eV} \leq μ_0 \leq 1.2\times10^{-20}\ {\rm eV}\}}$, spin-1: ${\scriptsize \{ 6.2\times10^{-15}\ {\rm eV} \leq μ_1 \leq 3.9\times10^{-11}\ {\rm eV}, 2.8\times10^{-22}\ {\rm eV} \leq μ_1 \leq 1.9\times10^{-16}\ {\rm eV} \}}$ and spin-2: ${\scriptsize \{ 2.2\times10^{-14}\ {\rm eV} \leq μ_2 \leq 2.8\times10^{-11}\ {\rm eV}, 1.8\times10^{-20}\ {\rm eV} \leq μ_2 \leq 1.8\times10^{-16}\ {\rm eV}, 6.4\times10^{-22}\ {\rm eV} \leq μ_2 \leq 7.7\times10^{-21}\ {\rm eV} \}}$ respectively. We also explore these bounds in the context of specific phenomenological models, specifically the QCD axion, M-theory models and fuzzy dark matter sitting at the edges of current limits. In particular we include recent measurements of event GW190521 and M87* used to constrain both the masses and decay constants of axion like fields. Finally we comment a simple example of a spectrum of fields for the spin-0 and spin-1 cases.
