Dr. Ming Xiong Liu, Los Alamos National Laboratory
Nov8

The Asymmetry of Anti-Quarks in the Proton

Dr. Ming Xiong Liu, Los Alamos National Laboratory

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What is really inside a proton? The fundamental building blocks of the proton, quarks and gluons, have been known for decades. However, we still have an incomplete understanding of how these particles and their dynamics give rise to the quantum bound state of the proton and its physical properties, such as for example its spin and mass. The two “up” and one “down” quarks that comprise the proton in the simplest picture account only for a few percent of the proton mass, the bulk of which is in the form of quark and gluon kinetic and potential energy from the strong force. An essential feature of this force, as described by quantum chromodynamics, is its ability to create quark-antiquark pairs through quantum fluctuation inside the proton that exist only for a very short time. In this picture of quark-antiquark creation by the strong force, the probability distributions as a function of momentum for the presence of “up” and “down” antiquarks should be nearly identical, since their masses are quite similar and small compared to the mass of the proton. However, our recent results from the Fermilab E906/SeaQuest experiment at the Main Injector show evidence that they are very different, with more abundant “down” antimatter quarks than “up” antimatter quarks over a wide range of momentum fraction of the parent proton. These results revive interest in several proposed mechanisms as the origin of this antiquark asymmetry in the proton and point to the future measurements at the follow-up E1039/SpinQuest experiment with polarized proton/neutron targets that can distinguish between these mechanisms. Furthermore, the recent new initiative to search for Dark Sector physics with moderate upgrade to the SeaQuest/SpinQuest spectrometer will also be discussed briefly at the end.   

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About Dr. Ming Xiong Liu

Dr. Ming Xiong Liu, Los Alamos National Laboratory

Dr. Ming Xiong Liu received Ph.D from Yale University in 1997, on the experimental investigation of electroweak physics in high energy e+e- collisions by studying B0-B0bar mixing using data from the SLD experiment at SLAC. Afterward, he joined the BNL Omega group to work on the D0 experiment at Tevatron to search for BSM physics. In 1999, he moved to Los Alamos to work on the new PHENIX experiment at the Relativistic Heavy Ion Collider at BNL. Since then, his primary research focus has been on the study of nucleon spin structure and novel QCD dynamics in polarized proton + proton (or ion) collisions, Quark-Gluon-Plasma created in heavy ion collisions at RHIC, as well as the Fermilab experiments to be discussed today. He is currently leading the silicon pixel detector project for the DOE next generation heavy ion experiment, sPHENIX, scheduled to be online in early 2023 at RHIC, to further investigate QGP properties and study nucleon structure and spin physics with heavy quarks.

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