然而，通过光谱学测量，宇宙中氦的数量表明，宇宙中重子的数量要比基于星系光度所估计的要多得多。
However, the amount of helium in the universe, as measured by spectroscopy, suggests that there are far more baryons in the universe than estimates based on galactic luminosity indicate.
对我们而言，重子的CP镜像对称需要被打破。“Buckley解释说。”
"For us, made of baryons, to exist, the mirror of charge-parity symmetry needs to be broken," Buckley explains.
本文的主要目的和任务是求解基态八重态重子的光锥分布振幅，以及研究其在光锥求和规则中的应用。
The main aims of this thesis are to examine the distribution amplitudes of the octet baryons, and to investigate their applications.
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