Town Hall on QCD: why we should accelerate positrons

This past weekend in Cambridge, MA, was one of several town hall meetings being held around the country to get input from the community as NSAC (Nuclear Science Advisory Committee) undertakes the next “Long-Range Plan.” These plans are developed every seven years or so and set the priorities for nuclear physics research funding by government agencies such as the U.S. Department of Energy and the National Science Foundation. This weekend’s town hall was on Quantum Chromodynamics (QCD), and I had the privilege to be invited to talk about physics that would be made possible with an accelerator that could accelerate positrons.

Accelerating positrons isn’t hard. An existing electron accelerator, such as Jefferson Lab’s CEBAF, can do the job, provided the polarities of all the steering magnets are reversed. But it’s making the positrons in the first place that requires some investment. It’s not cheap (in the ball park of tens of millions of dollars), but it’s not nearly as expensive as, say, upgrading CEBAF’s terminal energy from 12 GeV to 24 GeV. And it’s no where near as expensive as building a new accelerator, such as the upcoming electron ion collider. As part of the Jefferson Lab Positron Working Group, I am advocating that a positron source be built at Jefferson Lab, so that positrons could be accelerated using th CEBAF accelerator, and experiments could be conducted with all of the amazing detectors and equipment that are already part of the laboratory’s infrastructure.

There are many great experiments one can do with a positron beam, and among them, the application I find to be most critical is determining how much two-photon exchange occurs in electron scattering. Electron scattering is a great probe for learning about how quarks are distributed within protons, but in analyzing such measurements, we assume that the electron exchanges one and only one virtual photon with the quark that it collides with. It can exchange more than one photon (with each additional photon being significantly less likely), but calculating the probability of a second exchanged photon is not straightforward, and we typically assume that it has a negligible impact on the results. This may not have gotten us into trouble everywhere, but it likely has gotten us into trouble in our efforts to measure the proton’s charge distribution (its so-called “electromagnetic form factors.”)

Positrons can help clear up this mess because two-photon exchange has the opposite effect on positron scattering as it does on electron scattering. If we can measure a difference between, say, a positron-proton scattering reaction, and an electron-proton scattering reaction, then it tells us exactly what the effects of two-photon exchange are. This could help clear up the proton’s form factors, and tell us what to watch out for as we embark on measuring challenging new reactions like deeply virtual compton scattering or deeply virtual meson production.

Positrons are great for answering lots of other questions too, such as helping to map out the protons 3D structure (via its Generalized Parton Distributions), probing for “strange quarks” in the proton, or even searching for light dark matter. I think the benefits are really clear, and cost is not exorbitant, and I hope that a positron source at Jefferson Lab is endorsed in the Long-Range Plan.

If you’d like to learn more, I highly recommend checking out the JLab Positron Working Group’s White Paper, published as a special topical issue of the European Physical Journal A.

Electromagnetic Interactions of Nucleons and Nuclei Conference

I just returned from the 13th European Research Conference on Electromagnetic Interactions of Nucleons and Nuclei, a biannual conference held in Cyprus. There were some fascinating results presented, including a new determination of the proton’s charge radius by the PRad Experiment (it’s small!), a calculation of the “gluon EMC Effect” using Lattice QCD by MIT’s Phiala Shanahan, and lots of discussion about Large Momentum Effective Theory (LaMET), a new technique which may finally allow calculations of parton distribution functions on the Lattice.

The 2019 Frontiers and Careers Workshop participants

One of the best things about this conference is that it is preceded by a two-day workshop called “Frontiers and Careers in Photonuclear Physics,” which is specifically geared for students and early-career physicists. I feel honored that I was invited to give a pedagogical lecture about the EMC Effect at this year’s Frontiers, and I was so impressed by the job the organizers, Lena Heikenskjöld (Mainz) and Afroditi Papadopoulou (MIT), to put a wonderful workshop together. I highly encourage students to attend the 2020 edition of Frontiers, which will be held in August in New England in advance of the Gordon Research Conference on Photonuclear Reactions. You will learn a ton and meet a bunch of very interesting young physicists.

Afro Papadopoulou and I overlooking St. George’s Beach, near Chloraka, Cyprus.

Not only did Afroditi co-organize a fantastic Frontiers workshop, she also gave an outstanding talk on one of her research projects, “Electrons for Neutrinos,” in which analysis techniques from neutrino-nucleus scattering are benchmarked on electron-scattering data. Neutrino scattering experiments face the challenge of reconstructing the incoming neutrino energy event-by-event while simultaneously having to model the wide range of nuclear effects that can lead to the event’s measured final state. It’s a tough game, but Afroditi and others are showing how electron data can help.

From Afro’s talk: trying to reconstruct the beam energy from just one out-going electron, as is done in Cherenkov-based neutrino experiments is really hard, as shown by electron scattering data in which the beam energy is known precisely. Using a coincident proton can help, but it’s still far from perfect.

“Quasi-Free Scattering with Radioactive Beams” Workshop

It was a pleasure to be invited to Maresias, Brazil, for the 4th International Workshop on “Quasi-Free Scattering with Radioactive Beams” to talk about some on-going work on short-range nuclear correlations. I primarily use electron-scattering as my experimental technique of choice, and to hear about all of the incredible work being done using nuclear reactions, especially with unstable nuclei in inverse kinematics was fascinating. I will be thinking about ways to incorporate these methods into my own research.

Nothing like a tropical location to catalyze productive discussions. I’m here with my collaborator, Ronen Weiss, from Hebrew University.

My collaborator, MIT graduate student Efrain Segarra gave an outstanding talk about the hypothesis that the EMC Effect may stem from the modification of nucleons in short-range correlated pairs. Specifically, he presented results on how we can use measurements of the EMC Effect in heavy nuclei to constrain what we might expect when looking at light nuclei (specifically helium-3 and tritium!) and infer some information about free neutron structure. You can read our paper on the arXiv.

If short-range correlations are responsible for the EMC Effect, then heavy nuclei would indicate a larger F2n/F2p ratio at large x.