Axion Star and NS: Difference between revisions

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|GWCounterpart          = --
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|NeutrinoCounterpart    = --
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|References            = https://arxiv.org/pdf/1410.4323.pdf, https://arxiv.org/pdf/1412.7825.pdf, http://adsabs.harvard.edu/abs/2015PhRvD..91b3008I, http://adsabs.harvard.edu/abs/2016PhRvD..94j3004R
|References            = http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1412.7825, http://adsabs.harvard.edu/abs/2015PhRvD..91b3008I, http://adsabs.harvard.edu/abs/2016PhRvD..94j3004R
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Revision as of 05:32, 11 October 2018





Summary Table
Category Progenitor Type Energy Mechanism Emission Mechanism Counterparts References Brief Comments
LF Radio HF Radio Microwave Terahertz Optical/IR X-rays Gamma-rays Gravitational Waves Neutrinos
Collision / Interaction Axion Star and NS Single Electron oscillation -- Yes -- -- -- -- -- -- -- -- http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1412.7825, http://adsabs.harvard.edu/abs/2015PhRvD..91b3008I, http://adsabs.harvard.edu/abs/2016PhRvD..94j3004R None

Definitions: LF Radio (3 MHz to 3 GHz); HF Radio (3 GHz to 30 GHz); Microwave (30 to 300 GHz)


Model Description

To be filled in with updated draft

Observational Constraints

To be filled in with updated draft