News Center

Confirmed: Stellar Behemoth Self-Destructs in a Type IIb Supernova

The Palomar 48 inch telescope. (Photo by: Iair Arcavi, Weizmann Instiute of Science)

Wolf-Rayet stars, more than 20 times as massive as the Sun and at least five times as hot, are relatively rare and often obscured. Scientists don’t know much about how they form, live and die.

An Inside Look at a MOF in Action

A unique inside look at the electronic structure of a highly touted metal-organic framework (MOF) as it is adsorbing carbon dioxide gas should help in the design of new and improved MOFs for carbon capture and storage.

Nobel Laureate Karplus is Longtime NERSC User

On Wednesday, Oct. 9, the Nobel Prize in Chemistry was awarded to three scientists for pioneering methods in computational chemistry that have brought a deeper understanding of complex chemical structure and reactions in biochemical systems. These methods can precisely calculate how very complex molecules work and even predict the outcomes of very complex chemical reactions. One of the laureates — Martin Karplus of Harvard University — has been using supercomputers at the National Energy Research Scientific Computing Center (NERSC) at Berkeley Lab since 1998.

In Water as In Love, Likes Can Attract

Berkeley Lab researchers have shown that, contrary to the scientific axiom that only opposite charges attract, when hydrated in water, positively charged ions can pair up with one another.

Planck Mission Updates the Age of the Universe and What it Contains

At a March 21 NASA telephone news conference, scientists from the U.S. team participating in the European Space Agency’s Planck mission to map the cosmic microwave background (CMB) discussed Planck’s first cosmological results, including some surprising news. For one thing, the universe is 13.82 billion years old, a hundred million years older than previously thought,

Building the Massive Simulation Sets Essential to Planck Results

The Planck collaboration has released its first cosmological results, based on trillions of measurements of the cosmic microwave background. The results owe much to Berkeley Lab’s National Energy Research Scientific Computing Center (NERSC), including tens of millions of hours of massively parallel processing, plus the expertise of physicists and computational scientists in the Computational Cosmology Center (C3) who generated a quarter of a million simulated maps of the Planck sky, essential to the analysis.

Phase 1 of New Edison Supercomputer Arrives at NERSC

Edison Installation Begins (Photo: Roy Kaltschmidt)

Phase 1 of the National Energy Research Scientific Computing Center (NERSC)’s newest supercomputer, named Edison, has made its way to Berkeley Lab. The architecture is a Cray XC30 (“Cascade”) and will be installed in two phases. When it’s fully installed in 2013, Edison will have a peak performance of more than 2 petaflops (a petaflop

Berkeley Lab Scientists Help Define the Healthy Human Microbiome

The bacterium, Enterococcus faecalis, which lives in the human gut, is just one type of microbe that will be studied as part of NIH's Human Microbiome Project. (Courtesy: United States Department of Agriculture)

A National Institutes of Health (NIH)-organized consortium that includes Berkeley Lab scientists has for the first time mapped the normal microbial make-up of humans. Berkeley Lab’s role in mapping the human microbiome revolves around big data, both analyzing it and making it available for scientists to use worldwide. The research will help scientists understand how our microbiome keeps us healthy. It’ll also shed light on our microbiome’s role in many diseases.

Closest Type Ia Supernova in Decades Solves a Cosmic Mystery

The Palomar Transient Factory caught SN 2011fe in the Pinwheel Galaxy in the vicinity of the Big Dipper on 24 August, 2011. Found just hours after it exploded and only 21 million light years away, the discovery triggered the closest-ever look at a young Type Ia supernova. (Image by B. J. Fulton, Las Cumbres Observatory Global Telescope Network)

Even as the “supernova of a generation” came into view in backyards across the northern hemisphere last August, physicists and astronomers who had caught its earliest moments were developing a surprising and much clearer picture of what happens during a titanic Type Ia explosion. Now they have announced the closest, most detailed look ever at one of the universe’s brightest “standard candles,” the celestial mileposts that led to the discovery of dark energy.

Better Lithium-Ion Batteries Are On The Way From Berkeley Lab

Transmission electron microscopy reveals the new conducting polymer’s improved binding properties. At left, silicon particles embedded in the binder are shown before cycling through charges and discharges (closer view at bottom). At right, after 32 charge-discharge cycles, the polymer is still tightly bound to the silicon particles, showing why the energy capacity of the new anodes remains much higher than graphite anodes after more than 650 charge-discharge cycles during testing.

Lithium-ion batteries power everything from smart phones to electric cars, but especially when it comes to lowering the cost and extending the range of all-electric vehicles, they need to store a lot more energy. The critical component for energy storage is the anode, and Berkeley Lab scientists have developed a new anode material that can absorb eight times the lithium and has far greater energy capacity than today’s designs.