Understanding of ultra-dense neutron stars a step closer
Our understanding of the interior of ultra-dense neutron stars is a step closer following a particle accelerator experiment
The Standard Model of particle physics tells us that most particles we observe are made up of combinations of just six types of fundamental entities called quarks. However, there are still many mysteries, one of which is an exotic, but very short-lived, Lambda resonance known as Λ(1405).
For a long time, it was thought to be a particular excited state of three quarks – up, down, and strange – and understanding its internal structure may help us learn more about the extremely dense matter that exists in neutron stars. Now a particle accelerator experiment that creates an exotic, highly unstable particle and measures its mass, may help explain the interior of ultra-dense neutron stars.
Investigators from Osaka University were part of a team that succeeded in synthesising Λ(1405) for the first time by combining a K– meson and a proton and determining its complex mass (mass and width). The K− meson is a negatively charged particle containing a strange quark and an up antiquark. The much more familiar proton that makes up the matter that we are used to has two up quarks and a down quark.
The researchers showed that Λ(1405) is best thought of as a temporary bound state of the K– meson and the proton, as opposed to a three-quark excited state.
The group carried out the experiment at the J-PARC accelerator where K− mesons were shot at a deuterium target, each of which had one proton and one neutron. In a successful reaction, a K− meson kicked out the neutron, and then merged with the proton to produce the desired Λ(1405).
See also: Particles of light may create fluid flow
One of the authors of the study, Kentaro Inoue, said: “The formation of a bound state of a K– meson and a proton was only possible because the neutron carried away some of the energy.”
One of the aspects that had been perplexing scientists about Λ(1405) was its very light overall mass, even though it contains a strange quark, which is nearly 40 times as heavy as an up quark.
During the experiment, the team of researchers was able to successfully measure the complex mass of Λ(1405) by observing the behaviour of the decay products.
Shingo Kawasaki, another study author, said: “We expect that progress in this type of research can lead to a more accurate description of ultra-high-density matter that exists in the core of a neutron star.”
The work implies that Λ(1405) is an unusual state consisting of four quarks and one antiquark, making a total of five quarks, and does not fit the conventional classification in which particles have either three quarks or one quark and one antiquark.
The research may lead to a better understanding of the early formation of the universe, shortly after the Big Bang, as well as what happens when matter is subject to pressures and densities well beyond what we see under normal conditions.
The study is published in Physics Letters B.
Image: Schematic illustration of the reaction used to synthesise Λ(1405) by fusing a K- (green circle) with a proton (dark blue circle), which takes place inside a deuteron nucleus. © Hiroyuki Noumi.