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
The 2025 lecture series in physics is “Matter Under Pressure.” This series will investigate the fascinating behaviors of matter when subjected to extreme conditions. From the intense forces found in planetary cores to the violent dynamics of cosmic events, speakers will discuss how pressure can alter the physical and chemical properties of materials. The lectures will cover a range of topics, including the creation of new materials, the study of exotic states of matter in stars and the implications for understanding both Earth and exoplanetary environments.
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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 mimics what the universe was like mere microseconds after the Big Bang, and the tiny droplets 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 go over this extreme area of research and look ahead to upcoming measurements that will use jets to probe the microstructure of the quark soup to 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