arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 2007.03222astro-ph.HEhep-ph
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具有超大质量黑洞自旋测量的轻玻色子模型的严格约束

Stringent constraints on the light boson model with supermassive black hole spin measurements

Lei Zu, Lei Feng, Qiang Yuan, Yi-Zhong Fan

摘要:

大质量玻色子,如光标量和矢量玻色子,可以通过超辐射效应从快速旋转的黑洞中有效地提取能量和角动量,从而导致旋转黑洞的不稳定性。这个过程导致黑洞的自旋下降,并在它们周围形成玻色子云。在这项工作中,我们使用的质量和自旋的超大质量黑洞测量的紫外/光学或X射线观测来约束模型参数的轻玻色子。我们发现从$10^{-22}$ eV到$10^{-17}$ eV的轻玻色子的质量范围在很大程度上可以被一组超大质量黑洞(也包括质量极大的OJ 287、Ton 618和SDSS J140821.67+025733.2)排除,特别是对于矢量玻色子方案,它消除了一大部分所谓的模糊暗物质参数区域。对于具有自相互作用的标量玻色子,从$\sim 3 \times 10^{-19}$ eV到$10^{-17}$ eV的大部分质量范围以及衰减常数为$f_a > 10^{15}$ GeV的部分可以被排除,这令人信服地消除了这些质量的QCD轴子。

英文摘要:

Massive bosons, such as light scalars and vector bosons, can lead to instabilities of rotating black holes by the superradiance effect, which extracts energy and angular momentum from rapidly-rotating black holes effectively. This process results in spinning-down of black holes and the formation of boson clouds around them. In this work, we used the masses and spins of supermassive black holes measured from the ultraviolet/optical or X-ray observations to constrain the model parameters of the light bosons. We find that the mass range of light bosons from $10^{-22}$ eV to $10^{-17}$ eV can be largely excluded by a set of supermassive black holes (including also the extremely massive ones OJ 287, Ton 618 and SDSS J140821.67+025733.2), particularly for the vector boson scenario, which eliminates a good fraction of the so-called fuzzy dark matter parameter regions. For the scalar bosons with self-interaction, most part of the mass range from $\sim 3 \times 10^{-19}$ eV to $10^{-17}$ eV with a decay constant $f_a > 10^{15}$ GeV can be excluded, which convincingly eliminate the QCD axions at these masses.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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