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Quark matter may exist in the cores of neutron stars, where gravity compresses matter to the highest densities attained in nature. I will discuss an interesting feature of stars with a quark matter core: heavy damping of density oscillations arising from periodic conversion between nuclear matter and quark matter. I will show that this process can have a dramatic effect on known oscillatory modes, and could therefore provide a signature of the presence of quark matter.
Sponsored By:
The Flint Fund, Yale Physics, and Yale Wright Lab
Host:
Thursday, December 10, 2015 - 3:45pm