Quark Deconfinement in Neutron Stars
TITLE:
Quark Deconfinement in Neutron Stars
DATE:
Friday, September 2nd, 2016
TIME:
3:30 PM
LOCATION:
GMCS 324
SPEAKER:
Dr. Fridolin Weber. Professor of Physics at San Diego State University
ABSTRACT:
Neutron stars are the remnants of massive stars that blew apart in supernova explosions. Gravity compresses the matter in the cores of such objects
to densities that are several times higher than the densities inside of atomic nuclei. At such enormous densities atoms themselves collapse and
neutrons and protons are squeezed so tightly together that their quark contents may be released. In this talk, I will discuss the astrophysical
implications of this phase transition for neutron stars, based on numerical state-of-the-art investigations.
HOST:
Dr. Jose Castillo
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