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University of Cambridge > Talks.cam > DAMTP Friday GR Seminar > The electromagnetic weight loss of compact axion stars
The electromagnetic weight loss of compact axion starsAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Xi Tong. If dark matter is composed of axions, then axion stars are expected to be abundant in the Universe. In this talk, I will demonstrate in fully non-linear (3+1) numerical relativity the instability of compact axion stars due to the electromagnetic Chern-Simons term. The coupling of the axion to electromagnetism forms the basis of various axion detection experiments. I will show that above a critical coupling constant, compact axion stars are unstable, decaying into a less massive, less compact, remnant. Finally, I’ll address this instability in the context of axion star mergers. This talk is part of the DAMTP Friday GR Seminar series. This talk is included in these lists:
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