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03/01/06

A special introduction

“It’s not often you get introduced by a Nobel Prize winner,” said US Energy Secretary Samuel Bodman, former professor of chemical engineering at MIT and CEO of a Fortune 300 company.

03/01/06

Where do they go?

High-energy physics labs worldwide are neighbors with numerous butterfly species–from the Common Blue (Polyommatus icarus, photo) found near CERN to the Pipevine Swallowtail (Battus philenor) that shares the Bay Area with SLAC. But where do butterflies go in the winter?

02/01/06

Supernova 1987A

Upon arriving for work at the laboratory of Masatoshi Koshiba at the University of Tokyo, Yoji Totsuka handed me a fax telling of a supernova in the Large Magellanic Cloud, picked up by optical telescopes.

02/01/06

Julian Voss-Andreae: In three dimensions

Unveiling the three-dimensional structure of proteins thrills scientists. While the potential for understanding the folding and function of enzymes is truly exciting by itself, exploring macromolecule structures also satisfies a more fundamental urge: to see the invisible.

02/01/06

Hitting the broad side of a (classified) barn

The distinctive and amusing term "barn" originated with two Purdue University physicists working on the Manhattan Project in 1942—and it was classified information by the US government until after World War II.

02/01/06

Luminosity

Luminosity is a measure of how many particles are brought together in a certain space over a certain period of time.

02/01/06

Collimation

In high-energy collisions, luminosity, or beam brightness, isn't the only thing to consider; low background noise at the detectors is also important. When wayward particles bounce around inside detectors, they can mimic real collisions, muddy results, and even damage parts of the collider.