Heavy-ion physics at the LHC

Heavy-ion physics at the LHC

In the LHC heavy-ion programme, beams of heavy nuclei ("ions") collide at energies up to 30 times higher than in previous laboratory experiments. In these heavy-ion collisions, matter is heated to more than 100,000 times the temperature at the centre of the Sun, reaching conditions that existed in the first microseconds after the Big Bang. The aim of the heavy-ion programme at the LHC is to produce this matter at the highest temperatures and densities ever studied in the laboratory, and to investigate its properties in detail. This is expected to lead to basic new insights into the nature of the strong interaction between fundamental particles.
The strong interaction is the fundamental force that binds Nature's elementary particles, called quarks, into bigger objects such as protons and neutrons, which are themselves the building blocks of the atomic elements. Much is known today about the mechanism with which the elementary force-carriers of the strong interaction, the gluons, bind quarks together into protons and neutrons. However, two aspects of the strong interaction remain particularly intriguing.
First, no quark has ever been observed in isolation: quarks and gluons seem to be confined permanently inside composite particles, such as protons and neutrons. Second, protons and neutrons contain three quarks, but the mass of these three quarks accounts for only one percent of the total mass of a proton or neutron. So while the Higgs mechanism could give rise to the masses of the individual quarks, it cannot account for most of the mass of ordinary matter.
The current theory of strong interactions, called quantum chromodynamics, predicts that at very high temperatures, quarks and gluons are deconfined and can exist freely in a new state of matter known as the quark-gluon plasma. Theory also predicts that at the same temperature, the mechanism that is responsible for giving composite particles most of their mass ceases to act.
In the LHC heavy-ion programme, three experiments – ALICE, ATLAS and CMS – aim to produce and study this extreme, high-temperature phase of matter and provide novel access to the question of how most of the mass of visible matter in the Universe was generated in the first microseconds after the Big Bang.