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arXiv 1706.03393astro-ph.HEhep-phhep-th
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超新星Ia中激进新物理学的六个迹象

Six indications of radical new physics in supernovae Ia

L. Clavelli

摘要:

在超新星Ia的基本标准模型提出40多年后,许多天文学家仍然希望这种现象最终能被牛顿引力加上核物理和粒子物理所理解,就像它们在20世纪30年代存在一样。尽管如此,超新星物理学中至少有六个令人困扰的难题表明,一些激进的新物理学输入可能是必要的。在这里,“激进”是指一个在20世纪30年代不存在的物理学想法,并且在2017年仍然没有得到实验证实。

英文摘要:

After more than forty years since the basic standard model for supernovae Ia was proposed many astronomers are still hopeful that this phenomenon will ultimately be understood in terms of Newtonian gravity plus nuclear and particle physics as they existed in the 1930's. In spite of this fact there are at least six nagging puzzles in supernova physics that suggest some radical new physics input may be necessary. "Radical" in this context means a physics idea that did not exist in the 1930's and that is still not experimentally confirmed in 2017.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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