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arXiv 1011.0629astro-ph.SR
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太阳轴子/WISP的特征

Signatures for Solar Axions/WISPs

Konstantin Zioutas, Theodoros Vafeiadis, Mary Tsagri, Yannis K Semertzidis, Thomas Papaevangelou, Theopisti Dafni, Vassilis Anastassopoulos

摘要:

标准的太阳物理学无法解释X射线发射和其他谜题,最引人注目的例子是日冕之谜。日冕温度上升以上的非耀斑磁化太阳黑子,而光球下变得更冷,使这个谜更耐人寻味。矛盾的太阳暗示着某种奇异的解决方案,轴子是(唯一的?)选择缺失的成分。我们提出了非典型的轴子签名,描绘太阳轴子的静止质量最大~17毫电子伏/c2。几十年来,太阳一直是被忽视的新粒子物理学的先驱。

英文摘要:

Standard solar physics cannot account for the X-ray emission and other puzzles, the most striking example being the solar corona mystery. The corona temperature rise above the non-flaring magnetized sunspots, while the photosphere just underneath becomes cooler, makes this mystery more intriguing. The paradoxical Sun is suggestive of some sort of exotic solution, axions being the (only?) choice for the missing ingredient. We present atypical axion signatures, which depict solar axions with a rest mass max ~17 meV/c2. Then, the Sun has been for decades the overlooked harbinger of new particle physics.

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