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Modeling of helium flux in cosmic rays with Alpha Magnetic Spectrometer measurements

机译:α磁性谱仪测量宇宙射线氦气通量的建模

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摘要

Discrete quantum kinetic model together with the introduction of Pauli-blocking parameter and an orientation parameter are adopted to firstly obtain the dispersion relations of plane waves propagating in dilute Bose gases. With the diffusion mode of the dispersion relations of plane waves propagating in dilute Bose gases as well as the acoustic analog we can study the helium (boson) flux in cosmic rays considering the precision measurement with the Alpha Magnetic Spectrometer (AMS) on the International Space Station (ISS). Our approximately numerical as well as analytic results match qualitatively quite well with those data measured with the AMS on the ISS.
机译:采用离散量子动力学模型以及引入Pauli阻断参数和取向参数,首先获得在稀释瓶气中传播的平面波的分散关系。 利用在稀释的瓶气中传播的平面波的分散方式以及声学类似物,我们可以考虑在国际空间上的α磁光频仪(AMS)的精度测量,研究宇宙射线中的氦气(玻色子)通量 站(ISS)。 我们近似数值以及分析结果与ISS上的AMS测量的数据相比很好地匹配。

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