Limits on Source Distances for the Most Energetic Cosmic Rays

R. Lampard

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Limits on Source Distances for the Most Energetic Cosmic Rays

机译：最高能宇宙射线的源距离限制

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The propagation of the highest energy cosmic rays through the 2?·7 K microwave background is considered. Photo-pion production interactions cause energy losses for primary cosmic ray protons which result in significant energy degradation over intergalactic distances. The process of energy loss is discussed and an estimate is made of the average distances travelled for observed cosmic rays with a range of energies, assuming a power law source spectrum. At energies over 1020 eV, the average distances travelled are a few tens of megaparsecs, limiting possible sources to the volume dominated by the supergalactic plane.

机译：考虑了最高能量的宇宙射线通过2？·7 K微波背景的传播。光电子产生的相互作用会导致主要宇宙射线质子的能量损失，从而导致整个星系间距离的能量明显下降。讨论了能量损失的过程，并假设了幂律源光谱，对观察到的宇宙射线在一定能量范围内的平均行进距离进行了估算。在能量超过1020 eV时，平均行进距离为几十兆帕，将可能的源限制在由超银河系飞机控制的体积内。

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《Publications of the Astronomical Society of Australia》 |2013年第3期|共页
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R. Lampard;
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1. A gamma-ray signature of energetic sources of cosmic-ray nuclei [J] . Kusenko A., Voloshin M.B. Physics Letters, B. Nuclear Physics and High Energy Physics . 2012,第2期

机译：宇宙射线核能量源的伽马射线特征
2. This work extends our previous two-dimensional self-consistent model of the cosmic rays interacting with the solar wind to include anomalous cosmic rays. As before, energetic particles are described kinetically using a Parker equation. The model includes [J] . S. L. SNOWDEN, M. R. COLLIER, K. D. KUNTZ The Astrophysical journal . 2004,第2Pt1期

机译：这项工作扩展了我们先前的与太阳风相互作用的宇宙射线的二维自洽模型，以包含异常的宇宙射线。如前所述，使用Parker方程在动力学上描述了高能粒子。该模型包括
3. This work extends our previous two-dimensional self-consistent model of the cosmic rays interacting with the solar wind to include anomalous cosmic rays. As before, energetic particles are described kinetically using a Parker equation. The model includes [J] . S. L. SNOWDEN, M. R. COLLIER, K. D. KUNTZ The Astrophysical journal . 2004,第2Pt1期

机译：这项工作扩展了我们先前的与太阳风相互作用的宇宙射线的二维自洽模型，以包含异常宇宙射线。如前所述，使用Parker方程动力学地描述了高能粒子。该模型包括
4. Validation of Cosmic Ray Ionization Model CORIMIA Applied for Solar Energetic Particles and Anomalous Cosmic Rays [C] . S. Asenovski, P. Velinov, L. Mateev School and Workshop on Space Plasma Physics . 2016

机译：太阳能粒子和异常宇宙射线施用宇宙射线电离模具科素的验证
5. Upper limits on the ultra-high energy cosmic ray flux from unresolved sources. [D] . Burton, Ross E. 2012

机译：来自未解析源的超高能宇宙射线通量的上限。
6. Energetic Radiation From Galactic Cosmic Ray Interactions With Saturn’s Main Rings [O] . John F. Cooper, Steven J. Sturner -1

机译：银河系与土星主环相互作用的高能辐射
7. Limits on source distances for the most energetic cosmic rays [O] . Lampard, R., Clay, R., Dawson, B. 1997

机译：限制最有活力的宇宙射线的源距离

Limits on Source Distances for the Most Energetic Cosmic Rays

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