Ordinarily, neutrinos and antineutrinos readily escape from stellar interiors without making collisions . 通常，中微子和反中微子容易无碰撞地从星体内部逃逸出去。
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There is a good chance that this outward diffusion of neutrinos and antineutrinos plays a crucial role in the supernova explosion . 中微子和反中微子的这种向外的散射很可能在超新星爆发中起着关键的作用。
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Now researchers report that antineutrinos , ghostly particles with tiny masses , might generate these rare ingredients 近来有研究人员提出，这些罕见成份的来源，可能是质量微小的幽灵粒子反微中子。
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In the april 14 physical review letters , investigators at the university of basel in switzerland and their colleagues suggest antineutrinos streaming in huge numbers from the neutron star could irradiate the protons and turn some into neutrons , which build stable , heavy isotopes 在4月14日的《物理评论通讯》中，瑞士巴塞尔大学的研究人员与合作伴提出，从中子星大量涌出的反微中子会照射质子，并使部份质子转变为中子，以形成稳定的重同位素。
