Quark Matter Under Pressure: Novel Probes of Hot and Cold Quark Soup
- Speaker
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Krishna Rajagopal, Ph.D.William A. M. Burden Professor of Physics, Massachusetts Institute of Technology
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At Long Island and Geneva laboratories, nuclei collide at speeds incredibly close to the speed of light. The collisions create tiny droplets of quark soup with temperatures of around 1 trillion degrees and pressures 10 million trillion trillion times Earth’s atmospheric pressure at sea level. This hot quark soup is the same stuff which filled the universe microseconds after the Big Bang, and these tiny droplets of it promptly explode. Over the last twenty years, data from these “Little Bangs” have shown that this primordial fluid is the most liquid liquid in the universe. In this Presidential Lecture, Krishna Rajagopal will sketch how we have learned this and look ahead to upcoming measurements that will use jets to probe the microstructure of hot quark soup and see how each droplet ripples after being probed.
Cold quark soup, at pressures almost as high, can be found at the centers of the heaviest neutron stars, where the inward pressure of the surrounding star prevents it from exploding. Cold quark soup is expected to be the quark analog of a superconductor, a prediction that may be within reach of coming astrophysical observations of neutron stars and their mergers.