August 14, 2017

Video: Dark Matter Hunt with LUX-ZEPLIN

SLAC scientists are helping to build and test one of the biggest and most sensitive detectors ever designed to catch hypothetical WIMP particles.

Researchers at the Department of Energy’s SLAC National Accelerator Laboratory are on a quest to solve one of physics’ biggest mysteries: What exactly is dark matter – the invisible substance that accounts for 85 percent of all the matter in the universe but can’t be seen even with our most advanced scientific instruments?

Most scientists believe it’s made of ghostly particles that rarely bump into their surroundings; that’s why billions of dark matter particles might zip right through our bodies every second without us even noticing. Leading candidates for dark matter particles are WIMPs, or weakly interacting massive particles.

Now SLAC is helping to build and test one of the biggest and most sensitive detectors ever designed to catch a WIMP – the LUX-ZEPLIN or LZ detector. The following video explains how it works.

Video
(SLAC National Accelerator Laboratory)

Contact

For questions or comments, contact the SLAC Office of Communications at communications@slac.stanford.edu.


SLAC is a multi-program laboratory exploring frontier questions in photon science, astrophysics, particle physics and accelerator research. Located in Menlo Park, Calif., SLAC is operated by Stanford University for the U.S. Department of Energy's Office of Science.

SLAC National Accelerator Laboratory is supported by the Office of Science of the U.S. Department of Energy. The Office of Science is the single largest supporter of basic research in the physical sciences in the United States, and is working to address some of the most pressing challenges of our time. For more information, please visit science.energy.gov.

LZ Dark Matter Detector
SLAC is helping to build and test the LUX-ZEPLIN (LZ) detector, one of the biggest and most sensitive detectors ever designed to catch hypothetical dark matter particles known as weakly interacting massive particles (WIMPs).  (Greg Stewart/SLAC National Accelerator Laboratory)
Dig Deeper

Related stories

Feature

Salleo sees strength in the big picture and minute details of the people, tools and partnerships at SLAC.

Portrait of Alberto Salleo
Feature

Cosmologists Josh Frieman and Risa Wechsler look back on the Dark Energy Survey, sharing how it’s paving the way for Rubin Observatory to dig...

Josh Frieman and Risa Wechsler
News Brief

The latest results combined weak lensing and galaxy clustering and incorporated four dark energy probes from a single experiment for the first time.

Photo of the Cerro Tololo Inter-American Observatory (CTIO) in the Chilean Andes at night.
Feature

Salleo sees strength in the big picture and minute details of the people, tools and partnerships at SLAC.

Portrait of Alberto Salleo
Feature

Cosmologists Josh Frieman and Risa Wechsler look back on the Dark Energy Survey, sharing how it’s paving the way for Rubin Observatory to dig...

Josh Frieman and Risa Wechsler
News Brief

The latest results combined weak lensing and galaxy clustering and incorporated four dark energy probes from a single experiment for the first time.

Photo of the Cerro Tololo Inter-American Observatory (CTIO) in the Chilean Andes at night.
Feature

Researchers find evidence of coexisting atomic stacking patterns in superionic water. 

Dark background with three connected elements: a blue and purple sphere on left, blue molecular spheres in center circle, and green prism on right.
News Release

First peer-reviewed paper using data from SLAC-built LSST Camera identifies an asteroid, nearly the size of eight football fields, rotating every two minutes.

Illustration showing asteroids
News Release

In the largest dataset ever collected by a dark matter detector, LUX-ZEPLIN's latest results provide the strongest constraints on low-mass WIMPs and detect boron-8...

Overhead view looking down into a white structure with dozens of orange circular components arranged radially.