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Lensing of Fast Radio Bursts as a Probe of Compact Dark Matter

机译:作为紧凑暗物质探测器的快速射电爆发的发射

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摘要

The possibility that part of the dark matter is made of massive compact haloobjects (MACHOs) remains poorly constrained over a wide range of masses, andespecially in the $20-100\, M_\odot$ window. We show that strong gravitationallensing of extragalactic fast radio bursts (FRBs) by MACHOs of masses largerthan $\sim20\,M_\odot$ would result in repeated FRBs with an observable timedelay. Strong lensing of an FRB by a lens of mass $M_L$ induces two images,separated by a typical time delay $\sim$ few $\times(M_L/30\, M_\odot)$milliseconds. Considering the expected FRB detection rate by upcomingexperiments, such as CHIME, of $10^4$ FRBs per year, we should observe fromtens to hundreds of repeated bursts yearly, if MACHOs in this window make upall the dark matter. A null search for echoes with just $10^4$ FRBs, wouldconstrain the fraction $f_{\rm DM}$ of dark matter in MACHOs to $f_{\rmDM}\lesssim 0.08$ for $M_L\gtrsim 20\,M_\odot$.
机译:暗物质的一部分是由大型致密光晕物体(MACHOs)构成的可能性仍然受到很大范围的限制,尤其是在$ 20-100 \,M_ \ odot $窗口中。我们显示,质量大于$ \ sim20 \,M_ \ odot $的MACHO会强烈地引诱银河外快速无线电脉冲串(FRB),这将导致重复的FRB出现可观察到的时延。用质量为$ M_L $的透镜对FRB进行强力成像会产生两个图像,它们之间的间隔为典型的时间延迟$ \ sim $几$ \ times(M_L / 30 \,M_ \ odot)毫秒。考虑到未来的实验(例如CHIME)预期的FRB检出率为每年$ 10 ^ 4 $ FRB,如果该窗口中的MACHO能够掩盖所有暗物质,则我们应该观察每年数十次至数百次重复爆发。如果仅使用$ 10 ^ 4 $ FRB进行回波的空搜索,则会将MACHO中暗物质的分数$ f _ {\ rm DM} $限制为$ f _ {\ rmDM} \ lesssim 0.08 $(对于$ M_L \ gtrsim 20 \,M_ \ odot $。

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