"The Fate of Axion Stars"

Speaker: 
Hong Zhang
Institution: 
Ohio State Univ.
Date: 
Wednesday, October 19, 2016
Time: 
3:00 pm
Location: 
FRH 4135
 
 

 
ABSTRACT:
 
If the dark matter consists of axions, some of it will condense into axion stars, which are gravitationally bound Bose-Einstein condensates of axions. If an axion star accretes enough axions to exceed a critical mass, it will collapse. The fate of a collapsing axion star has not been established. One possibility for the remnant is a much denser axion star in which the attractive forces of gravity and axion pair interactions are balanced by the mean-field pressure of the axion Bose-Einstein condensate. A nonrelativistic effective field theory for axions can provide insights into the fate of axion stars. The collapsing process of axion stars and the possible denser remnant produce unique monochromatic radio-frequency signals at odd-integer harmonics of the fundamental frequency set by the axion mass.
 

 
Host: 
Iftah Galon