SLAC National Accelerator Laboratory

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SLAC National Accelerator Laboratory The official account of SLAC National Accelerator Laboratory, a U.S. Department of Energy National Lab operated by Stanford University.

SLAC National Accelerator Laboratory is the U.S. Department of Energy's Silicon Valley national lab, operated by Stanford University. Since its opening in 1962, SLAC has been helping create the future. We built the world’s longest particle accelerator, discovered some of the fundamental building blocks of matter and created the first website in North America. Our top-notch research facilities attract thousands of scientists from all over the world each year. Along with our own staff scientists, they’re working to discover new drugs for healing, new materials for electronics and new ways to produce clean energy and clean up the environment. SLAC’s revolutionary X-ray laser is revealing intimate details of atoms and chemical reactions and making stop-motion movies of this tiny realm, with the goal of doing the same for living cells. Our scientists are also exploring the cosmos, from the origin of the universe to the nature of dark energy, and developing the smaller, more efficient particle accelerators of the future. We built the world's largest digital camera which is now installed in the NSF-DOE Vera C. Rubin Observatory and will capture the cosmos like never before. Four scientists have been awarded Nobel prizes for work done at SLAC, and more than 1,000 scientific papers are published each year based on research at the lab. As our second half-century unfolds, we’re just getting started.

I could be brown, I could be blue, I could be violet sky! 🎵 Did you know that every hutch at LCLS has its own color? Are...
10/22/2026

I could be brown, I could be blue, I could be violet sky! 🎵

Did you know that every hutch at LCLS has its own color? Area managers for each hutch try to match their supplies and equipment in the corresponding hutch color, making it easy to identify where they belong, and fun to look at. Which is your favorite?

🟤 qRIXS & chemRIXS - Materials Science Resonant Inelastic X-ray Scattering & Liquid Chemistry Resonant Inelastic X-ray Scattering

The qRIXS and chemRIXS instruments use a technique called resonant inelastic X-ray scattering (RIXS). With this method, researchers bombard a sample with X-ray pulses, exciting the electrons deep within, then releasing that excess energy in the form of light. Researchers use this light to reconstruct the reaction and study a material’s properties in fine detail.

🔵 TMO - Time-resolved AMO

In the Time-resolved Atomic, Molecular and Optical Science (TMO) end station, several new instruments are leveraging the LCLS-II upgrade to study how electrons kickstart processes in biology, chemistry and materials science. It follows in the footsteps of the now-retired AMO instrument, where scientists developed a way to measure ultrashort X-ray pulses that last for just several hundred attoseconds (or billionths of a billionth of a second).

🟣 XCS - X-ray Correlation Spectroscopy

The X-ray Correlation Spectroscopy (XCS) instrument observes dynamical changes of large groups of atoms in condensed matter systems over a wide range of time scales.
Characteristic timescales ranging from 10 milliseconds to thousands of seconds can be explored using a sequential mode of operation. Ultrafast timescales ranging from 100 femtosecond to several nanoseconds can be probed using a novel “Split-and-Delay” mode of operation.

🔴 CXI - Coherent X-ray Imaging

The CXI instrument uses unique hard X-ray pulses in a vacuum sample environment to provide low background suitable for forward scattering experiments and weakly scattering systems.
CXI primarily uses the “diffraction-before-destruction” method, a technique to quickly acquire data with ultrashort pulses during measurement before the sample is destroyed, benefiting systems that suffer from electronic and structural damage during long-term exposures to X-rays.

🟠 MFX - Macromolecular Femtosecond Crystallography

The MFX instrument is the prime endstation at LCLS for multi-modal crystallographic measurements at atmospheric pressure, combining both macromolecular X-ray crystallography and X-ray spectroscopy. The MFX instrument uses short XFEL X-ray pulses to limit observed damage to samples during the exposure of radiation-sensitive samples, primarily biological samples, at room temperature.

🟡 MEC - Matter in Extreme Conditions

With its high peak brightness, short pulse duration, and tunable X-ray photon energy, our X-ray laser provides revolutionary capabilities to study the transient behavior of matter in extreme conditions.
The MEC instrument combines our unique beam with high power optical laser beams, and a suite of dedicated diagnostics tailored for this field of science. Researchers can create incredibly hot and dense matter that mimics the extreme conditions in the hearts of stars and planets.

🟢 XPP - X-ray Pump Probe

The XPP instrument predominantly uses ultrashort optical laser pulses to generate transient states of matter which are subsequently probed by hard X-ray pulses from the LCLS. The X-ray pulses help to reveal structural dynamics initiated by the laser excitation at the timescale of atomic motions in solid, liquid and gaseous specimens. Researchers have leveraged XPP to pioneer X-ray optics technologies, including cavity-based X-ray oscillators that are shaping future X-ray free-electron laser facilities.

🩷 TXI - Tender X-ray Instrument

This instrument is designed to incorporate X-ray Pump and X-ray Probe techniques, and serve as a general purpose coherent scattering/forward diffraction instrument for sub-micron samples covering the “tender” X-ray range (loosely defined to be between the Si K edge of 1.8 keV and the Fe K edge of 7.1 keV).

Mine! Mine! Mine! Mine! 🌊🦅Taken by our 144-megapixel engineering test camera, this image of the Seagull Nebula commemora...
10/22/2026

Mine! Mine! Mine! Mine! 🌊🦅

Taken by our 144-megapixel engineering test camera, this image of the Seagull Nebula commemorates two years since we first began on-sky testing at the NSF-DOE Vera C. Rubin Observatory.

10/21/2026

Setting new records is hard.

But our X-ray laser has done it again – a new record for the shortest high-energy pulses ever generated by an X-ray free electron laser.
The pulses had energies of about 9 kiloelectronvolts (keV) and clocked in at speeds of 100 to 400 attoseconds – mere billionths of a billionth of a second. These high-energy, or “hard” attosecond X-ray pulses are invaluable for researchers studying the universe at its smallest, fastest scales. https://stanford.io/4jyWyvJ

Music: MB01B9KJDSYP5FO
Narrated by Taran Driver. Video by Olivier Bonin/SLAC.

Congratulations to Shaun Burd and Miguel Correia, our 2026 Panofsky Fellows!The Panofsky Fellowship, named after SLAC's ...
10/19/2026

Congratulations to Shaun Burd and Miguel Correia, our 2026 Panofsky Fellows!

The Panofsky Fellowship, named after SLAC's founder and first Director Wolfgang K. H. "Pief" Panofsky, recognizes exceptional early career scientists and provides funding for five years of research. Burd will be investigating proteins sensitive to magnetic fields and their potential applications, while Correia will explore the fundamental interactions that govern the universe.

The team behind the NSF-DOE Vera C. Rubin Observatory’s historic First Look has received a 2025 Secretary’s Honor Award,...
10/18/2026

The team behind the NSF-DOE Vera C. Rubin Observatory’s historic First Look has received a 2025 Secretary’s Honor Award, one of the U.S. Department of Energy’s forms of internal staff recognition, celebrating the many people whose expertise, collaboration and dedication helped bring this milestone to life.

Allison Eckhardt, Shannon Shea, Bryan Field, Glen Crawford, Aaron Roodman, Phil Marshall, Adam Bolton and Manuel Gnida, representing DOE’s Office of Science and SLAC, attended the Sept. 28 ceremony in Washington, D.C., accepting the honor on behalf of a large team supported by both DOE and the U.S. National Science Foundation (NSF), including staff at NOIRLab, SLAC, the Association of Universities for Research in Astronomy (AURA) and at Rubin Observatory at large.

10/16/2026

What will our 3.2 billion-pixel camera help us see?

The NSF–DOE Vera C. Rubin Observatory will catalog billions of objects and events in the night sky, alerting scientists around the world of where to look deeper to unravel the mysteries of our universe.

How do we protect an open cryomodule from dust and dirt?The same way you keep your hair dry in the shower! Just perhaps ...
10/15/2026

How do we protect an open cryomodule from dust and dirt?

The same way you keep your hair dry in the shower! Just perhaps slightly larger. Meet our “shower cap” (yes, we call it that), which keeps out contamination that would otherwise interfere with electrons accelerated within.

10/15/2026

Numerical simulations turned into striking scenes. This sequence follows the formation of the cosmic web in a region about 500 million lightyears across. The black shapes are filaments of dark matter, and their intersections host massive clusters of galaxies, shown in yellow.

Kavli Institute for Particle Astrophysics and Cosmology visualization expert Ralf Kaehler and astrophysicist Tom Abel, teamed up with the American Museum of Natural History’s director of astrovisualization Carter Emmart and museum coordinator and Columbia University professor Mordecai-Mark Mac Low to bring the mysteries of dark matter to the Hayden Planetarium. Music: MB01IIDDAQMNVFS

10/13/2026

Scott Manley came to SLAC last week to get a behind-the-scenes look at the world’s most powerful X-ray laser, now undergoing a high‑energy upgrade. He stopped by our X-ray Pump Probe Experiment hutch, the accelerator control room, the cryoplant, and saw our superconducting accelerator up close!

Music: MB01CDKNTM63XXB

Congratulations! Our own Adam Nielander has won a U.S. Department of Energy Office of Science Early Career Research Prog...
10/13/2026

Congratulations! Our own Adam Nielander has won a U.S. Department of Energy Office of Science Early Career Research Program award!

He will pursue research on light-powered catalysts for next-gen energy technologies using our Stanford Synchrotron Radiation Lightsource and cryoEM facilities, in order to tackle environmental remediation of nitrogen-based contaminants in groundwater and soil. https://stanford.io/4yLBPtb

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2575 Sand Hill Rd
Menlo Park, CA
94025

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