Jens Dilling, TRIUMF
Jens Dilling, TRIUMF

Thomas Jefferson National Accelerator Facility

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4 min read

Somewhere beneath the suburban lawns and strip malls of Newport News, Virginia, electrons race through a seven-eighths-mile loop at nearly the speed of light, slamming into targets so physicists can study what protons and neutrons are actually made of. The Thomas Jefferson National Accelerator Facility - Jefferson Lab, or just JLab to the people who work there - does not look like much from above. No dramatic cooling towers, no gleaming domes. The accelerator sits 25 feet underground, inside tunnels with walls two feet thick, shaped like a racetrack and cooled by the world's largest liquid helium refrigerator. More than 2,000 scientists from around the globe have conducted research here since it opened in the 1990s. They come to ask one of the oldest questions in physics: what holds matter together?

A Linear Accelerator, Folded Like Origami

CEBAF - the Continuous Electron Beam Accelerator Facility, the name that predates the Jefferson Lab branding - is an engineering marvel disguised as a racetrack. Two superconducting linear accelerators, each 1,400 meters long, sit parallel to each other, connected at both ends by curved arc sections packed with steering magnets. Electrons from a polarized source enter at one end and make up to five laps around this oval, gaining energy with each pass. The result is effectively a linear accelerator - like SLAC at Stanford - folded to a tenth of its normal length. What makes CEBAF distinctive among the world's accelerators is the continuous nature of its electron beam. Where ring-shaped machines like those at CERN or Fermilab produce pulsed beams, CEBAF delivers an almost unbroken stream of electrons, with pulses lasting less than a picosecond. This continuous beam gives physicists unprecedented resolution when they smash electrons into their targets.

Colder Than Outer Space

The accelerator's secret is superconducting radio frequency technology. Niobium cavities are cooled by liquid helium to approximately 4 Kelvin - about minus 452 degrees Fahrenheit, colder than the void between stars. At this temperature, electrical resistance vanishes entirely, allowing the most efficient possible transfer of energy to the electron beam. Jefferson Lab was one of the first large-scale implementations of this SRF technology, and it houses the world's largest liquid helium refrigerator to maintain these extreme conditions. The technology developed here has spread to accelerator facilities worldwide. JLab builds superconducting accelerator components and helium refrigeration systems for Department of Energy accelerators across the national laboratory complex, and contributed to the construction of the Spallation Neutron Source in Oak Ridge, Tennessee.

Four Halls, Four Windows into the Nucleus

The electron beam terminates in four experimental halls, designated A through D, each equipped with specialized spectrometers and particle detectors. When an electron strikes a nucleus in the target, the collision scatters particles into the hall, where detector arrays track their physical properties. The data reveals the behavior of quarks - the fundamental constituents of protons and neutrons. Hall A uses matching high-resolution spectrometers to study deep-inelastic electron scattering. Hall B houses the CLAS12 detector, successor to the original CLAS that operated from 1998 to 2012. Hall C measures parity-violating electron scattering to determine the weak charge of the proton. Hall D, the newest addition completed as part of the 12 GeV upgrade, houses the GlueX experiment, designed to map the light meson spectrum in search of exotic particles held together by the nuclear glue itself - gluons.

The $338 Million Upgrade

The original CEBAF achieved its design energy of 4 GeV in 1995, reached 6 GeV by 2000, and completed 178 experiments before shutting down in May 2012 for a transformative upgrade. The $338 million project doubled the beam energy to 12 GeV, added Hall D on the opposite end of the accelerator from the other three halls, and expanded the Test Lab where SRF cavities are manufactured. By spring 2018, all four halls were receiving beam and performing experiments. The 12 GeV Upgrade Dedication Ceremony took place on May 2, 2018. The higher energy opened new physics frontiers - allowing researchers to probe deeper into the structure of nucleons and search for particles that had been theoretically predicted but never observed. Jefferson Lab also houses a tunable free-electron laser that achieved first light on June 17, 1998, and later reached an output exceeding 14 kilowatts in November 2006, making it one of the world's most powerful free-electron lasers.

Big Science in a Small City

Jefferson Lab was established in 1984 as CEBAF, funded by the Department of Energy and built by the Southeastern Universities Research Association. Construction of the accelerator began on February 13, 1987, and the first beam reached the experimental area on July 1, 1994. The facility was renamed in 1996, and today employs more than 750 people in Newport News - a city better known for its massive shipyard than for particle physics. Yet here, in the Tidewater region of Virginia, more than 2,000 scientists from dozens of countries have gathered to study the deepest structure of the atom. The lab sits in the same stretch of the Virginia Peninsula as NASA Langley, the Yorktown battlefield, and Colonial Williamsburg - a corridor where American history and American science share the same zip code.

From the Air

Located at 37.09°N, 76.48°W in Newport News, Virginia. The accelerator complex is mostly underground, but the racetrack-shaped footprint is discernible from low altitude by the service buildings and access roads that trace the oval. Best viewed at 3,000-5,000 ft AGL. Newport News/Williamsburg International (KPHF) is 5nm north. Langley Air Force Base (KLFI) is 8nm east - active military airspace, check NOTAMs. The facility is near the intersection of I-64 and Jefferson Avenue. Hampton Roads area is prone to marine layer and haze, especially in summer months.