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arXiv 2602.04285astro-ph.COgr-qchep-phhep-th
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参数共振与反作用效应在超轻暗物质磁生成中的作用

Parametric Resonance and Backreaction Effects in Magnetogenesis from Ultralight Dark Matter

McGill University(麦吉尔大学)

Nirmalya Brahma, Robert Brandenberger

AI总结:

超轻暗物质通过窄带参数共振生成磁场,克服反作用效应影响,产生宇宙学尺度磁场。

摘要:

我们对最近提出的一种由超轻暗物质与电磁学耦合触发的磁生成机制进行了更深入的探讨。该机制利用了趋近于光速的共振通道,导致红外模式的指数放大。在此,我们首先研究了一种可能的窄带参数共振通道,该通道可以产生更高频率的光子。其次,我们估计了反作用效应在终止共振中的影响。我们发现确实存在一个窄共振通道。其特征是Floquet指数略小于对应于趋近于光速共振的指数。然而,在参数空间中存在一个区域(对应于非常小的耦合常数),使得趋近于光速共振无效。在这种情况下,窄共振将占主导地位,并且它仍然足以在宇宙学尺度上生成观测到的磁场。我们在这里对反作用效应的分析表明,初始暗物质密度的一小部分会流入规范场中。因此,我们的磁生成情景似乎对反作用效应具有鲁棒性。

英文摘要:

We take a more detailed look at the recently proposed magnetogenesis mechanism triggered by ultralight dark matter coupled to electromagnetism. The proposed mechanism made use of a tachyonic resonance channel which leads to the exponential amplification of infrared modes. Here, we first investigate a possible narrow band parametric resonance channel which can produce photons at higher frequencies. Secondly, we estimate the effects of back-reaction on terminating the resonance. We find that there is indeed a narrow resonance channel. It is characterized by a Floquet exponent which is slightly smaller than the corresponding exponent for the tachyonic resonance. However, there is a region of parameter space (corresponding to a very small coupling constant) for which the tachyonic resonance is ineffective. In this case, the narrow resonance will dominate, and it will still be sufficiently strong to generate the observed magnetic fields on cosmological scales. Our analytical treatment of the back-reaction effects considered here indicates that a fraction of order one of the initial dark matter density can flow into the gauge fields. Hence, our magnetogenesis scenario appears to be robust to back-reaction effects.

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