LHCb finds tetraquark candidates
The LHCb collaboration has reported the observation of three new exotic hadrons and confirmed the existence of a fourth by analysing the full data sample from LHC Run 1. Although the theoretical inte...
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The LHCb collaboration has reported the observation of three new exotic hadrons and confirmed the existence of a fourth by analysing the full data sample from LHC Run 1. Although the theoretical inte...
When heavy nuclei collide at high energies, a novel state of hot and dense matter – the quark–gluon plasma (QGP) – is expected to form. As a region of QGP expands and cools, it disso...
Precise measurements of final states containing multiple electroweak bosons (W, Z or γ) offer a powerful probe of the gauge structure of the Standard Model.
In a collision between two nuclei that exhibits a large impact parameter, the initial spatial anisotropy of the overlap region was conjectured to be smooth and almond shaped. In the past few years, ho...
The European Union project AIDA-2020 (Advanced European Infrastructure for Detectors and Accelerators), in which CERN is a partner, has launched a proof-of-concept fund for breakthrough projects in th...
Physicists in China have passed an important milestone towards an accelerator-driven sub-critical (ADS) system, a novel accelerator design for advanced energy and other technologies. On 2 July, teams...
SESAME, the pioneering synchrotron facility for the Middle East and neighbouring countries, located in Jordan, has announced its first call for proposals for experiments. A third-generation light sour...
The map shows galaxies being pulled towards each other by dark matter, while on much larger scales it reveals the effect of dark energy ripping the universe apart.
The International Union of Pure and Applied Chemistry (IUPAC) has announced the provisional names of four new super-heavy elements that complete the seventh row of the periodic table. The researchers ...
With its very first observation, Japan’s Hitomi X-ray satellite has discovered that the gas in the Perseus cluster of galaxies is much less turbulent than expected.