Let There Be Neutrons! Hadronic Photoproduction from a Large Flux of High-energy Photons

Matthew R. Mumpower, Tsung-Shung H. Lee, Nicole Lloyd-Ronning, Brandon L. Barker, Axel Gross, Samuel Cupp and Jonah M. Miller
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Abstract

We propose that neutrons may be generated in high-energy, high-flux photon environments via photo-induced reactions on pre-existing baryons. These photohadronic interactions are expected to occur in astrophysical jets and surrounding material. Historically, these reactions have been attributed to the production of high-energy cosmic rays and neutrinos. We estimate the photoproduction off of protons in the context of gamma-ray bursts, where it is expected there will be sufficient baryonic material that may be encompassing or entrained in the jet. We show that typical stellar baryonic material, even material completely devoid of neutrons, can become inundated with neutrons in situ via hadronic photoproduction. Consequently, this mechanism provides a means for collapsars and other astrophysical sites containing substantial flux of high-energy photons to be favorable for neutron-capture nucleosynthesis.
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让中子存在吧!高能光子大通量产生强子光
我们提出中子可能在高能量、高通量的光子环境中通过光诱导反应在已有重子上产生。这些光强子相互作用预计会发生在天体物理喷流和周围物质中。从历史上看,这些反应被归因于高能宇宙射线和中微子的产生。我们估计了在伽马射线爆发的背景下质子的光产生,在那里,预计将有足够的重子物质可能包围或携带在喷流中。我们证明了典型的恒星重子材料,甚至是完全没有中子的材料,可以通过强子光产生在原位被中子淹没。因此,这一机制为坍缩和其他天体物理场所提供了一种方法,这些场所含有大量高能光子,有利于中子捕获核合成。
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