Signals of Bursts from the Very Early Universe

Leo Stodolsky and Joseph Silk
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Abstract

We consider possible observable signals from explosive events in the very early Universe, dubbed “bursts.” These could be expected in connection with massive black hole or “baby Universe” formation. We anticipate that such major disruptions of spacetime would be associated with neutrino and perhaps other pulses. While these seem to be not detectable directly, we discuss how they could lead to potentially observable signals. We analyze how the pulses from very early times may “escape,” that is, propagate to the last scattering epoch at the time tcmb and later, or alternatively be absorbed earlier, i.e., “contained.” The possibly detectable signals include effects on small regions of the cosmic microwave background, a soft X-ray resulting from positron production, or a nonthermal addition to the relic neutrino background.
早期宇宙爆发的信号
我们考虑从宇宙早期爆炸事件中可能观察到的信号,被称为“爆发”。这些可能与大质量黑洞或“婴儿宇宙”的形成有关。我们预计,这种对时空的重大破坏可能与中微子或其他脉冲有关。虽然这些似乎无法直接检测到,但我们讨论了它们如何导致潜在的可观察信号。我们分析了来自非常早期的脉冲是如何“逃逸”的,即传播到最后一个散射时期,即在时间mb和之后,或者更早地被吸收,即“包含”。可能探测到的信号包括对宇宙微波背景小区域的影响,由正电子产生的软x射线,或者对遗迹中微子背景的非热附加。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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