The creation of a new state of matter has won two Americans and a German the 2001 Nobel Prize in Physics.
Their feat, producing a Bose-Einstein condensate (BEC), was achieved in 1995 – over 70 years after Albert Einstein had extended calculations by Satyendra Nath Bose to predict its existence.
In explaining BECs, the prize citation draws an analogy with light. Compared to ordinary light, a laser beam is composed of photons that all have the same energy and oscillate together.
“To cause matter also to behave in this controlled way has long been a challenge for researchers,” reads the citation. “This year’s Nobel Laureates have succeeded – they have caused atoms to ‘sing in unison’.”
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The three honoured are Eric Cornell, at JILA and the National Institute of Standards and Technology in Boulder, Colorado, Carl Wieman JILA and University of Colorado in Boulder, and Wolfgang Ketterle, at the Massachusetts Institute of Technology in Cambridge, Massachusetts. They will share the £690,000 prize money.
Cold, very cold
Einstein predicted that if a gas of certain atoms were cooled to very low temperature all the atoms would suddenly gather in the lowest possible energy state. The process is similar to when drops of liquid form from a gas, hence the term condensation.
In 1995, Cornell and Wieman succeeded in achieving this extreme state of matter. They produced a pure condensate of about 2000 rubidium atoms at 20 nanokelvin, i.e. 20 billionths of a degree above absolute zero.
Independently, Ketterle performed corresponding experiments with sodium atoms. The condensates he managed to produce contained more atoms and could therefore be used to investigate the phenomenon further.
Using two separate BECs that were allowed to expand into one another, he obtained very clear interference patterns. This showed that the condensate contained entirely co-ordinated atoms.
The new “control” of matter which BECs involves may bring applications in fields from precision measurement to nanotechnology.
![Astronomers have long known that understanding how star clusters come to be is key to unlocking other secrets of galactic evolution. Stars form in clusters, created when clouds of gas collapse under gravity. As more and more stars are born in a collapsing cloud, strong stellar winds, harsh ultraviolet radiation and the supernova explosions of massive stars eventually disperse the cloud, and their light can bear down on other star-forming regions in the galaxy. This process is called stellar feedback, and it means that most of the gas in a galaxy never gets used for star formation. Researching how star clusters develop can answer questions about star formation at a galactic scale. Now, the state of the art has been further developed with both Hubble and Webb working together to provide a broad-spectrum view of thousands of young star clusters. An international team of astronomers has pored over images of four nearby galaxies from the FEAST observing programme (#1783), trying to solve this mystery. Their results show that it is the most massive star clusters that clear away their gaseous shroud the fastest, and begin lighting their galaxy the earliest. The team identified nearly 9000 star clusters in the four galaxies in different evolutionary stages: young clusters just starting to emerge from their natal clouds of gas, clusters that had partially dispersed the gas (both from Webb images), and fully unobstructed clusters visible in optical light (found in Hubble images). With Webb???s ability to peer inside the gas clouds, they were able to then estimate the mass and age of each cluster from its light spectrum. This image shows a section of one of the spiral arms of Messier 51 (M51), one of the four galaxies studied in this work, as seen by Webb???s Near-Infrared Camera (NIRCam). The thick clumps of star-forming gas are shown here in red and orange, representing infrared light emitted by ionised gas, dust grains, and complex molecules such as polycyclic aromatic hydrocarbons (PAHs). Within these gas complexes, each tens or hundreds of light years across, Webb reveals the dense, extremely bright clusters of massive stars that have just recently formed. The countless stars strewn across the arm of the galaxy, many of which would be invisible to our eyes behind layers of dust, are also laid bare in infrared light. [Image description: A large, long portion of one of the spiral arms in galaxy M51. Red-orange, clumpy filaments of gas and dust that stretch in a chain from left to right comprise the arm. Shining cyan bubbles light up parts of the gas clouds from within, and gaps expose bright star clusters in these bubbles as glowing white dots. The whole image is dotted with small stars. A faint blue glow around the arm colours the otherwise dark background.]](https://images.newscientist.com/wp-content/uploads/2026/05/13114322/SEI_296271016.jpg)


