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Impact of neutron energy on asteroid deflection performance

机译:中子能量对小行星偏转性能的影响

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摘要

In the future, a hazardous asteroid will find itself on a collision course with Earth. For asteroids of moderate size or larger, a nuclear device is one of humanity's only technologies capable of mitigating this threat via deflection on a timescale of less than a decade. This work examined how the output neutron energy from a nuclear device standoff detonation affects the deflection of a notional asteroid that is 300 meters in diameter and composed of silicon dioxide at a bulk density of 1.855 g/cm(3). 14.1 MeV and 1 MeV neutron energy sources were modeled in MCNP to quantify the energy deposition in the asteroid target. The asteroid's irradiated region was discretized in angle by tracing the rays emanating from the point of detonation and in depth by considering the neutron mean-free-paths. This high-fidelity approach was shown to deviate from previous analytic approximations commonly used for asteroid energy deposition. 50 kt and 1 Mt neutron yields of the energy deposition mappings were imported into a hydrodynamic asteroid model in ALE3D to simulate the deflective response due to blow-off ejecta. Underexplored in literature, changing the neutron energy was found to have up to a 70% impact on deflection performance due to induced differences in the energy deposition profile and in the energy coupling efficiency. The magnitude of energy deposition accounted for most of the observed variation in the asteroid velocity change, making the coupling efficiency more significant than the spatial profile characteristics. These findings are vital for determining the optimal source neutron energy spectrum for asteroid deflection applications.
机译:未来,危险的小行星将在与地球上的碰撞过程中找到自己。对于中等尺寸或更大的小行星,核设备是人类唯一能够通过偏转不到十年的时间偏转来减轻这种威胁的技术之一。这项工作检测了来自核装置脱离爆炸的输出中子能量如何影响直径为300米的偏转,并且由二氧化硅以1.855g / cm(3)的堆积密度组成。 14.1 MEV和1 MEV中子能源在MCNP中进行建模,以量化小行星目标中的能量沉积。通过考虑中子平均路径来追踪从爆炸点发出的光线,通过追踪从爆炸点发出的光线并深入来分离小行星的照射区域。该高保真方法显示出偏离常用于小行星能量沉积的先前分析近似。将50kt和1 mt中子产量的能量沉积映射的产量导入ALE3D中的流体动力小行星模型中,以模拟由于吹除喷射而导致的偏转反应。在文献中,由于能量沉积轮廓曲线和能量耦合效率的诱导差异,发现更换中子能量对偏转性能的影响高达70%的影响。能量沉积的大小占小行星速度变化的大多数观察到的变化,使得耦合效率比空间轮廓特性更大。这些发现对于确定小行星偏转应用的最佳源中子能谱至关重要。

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