The weak force is responsible for the decay of matter: unstable particles made of heavy quarks and antiquarks decay into particles made of their lighter cousins. The rates of these decay processes are related to a set of numbers called the Cabibbo-Kobayashi-Maskawa (CKM) matrix, named for the three physicists who introduced it. The numbers are often shown in a graphical form called the unitarity triangle.
Deconstruction: Unitarity triangle
The weak force is responsible for the decay of matter: unstable particles made of heavy quarks and antiquarks decay into particles made of their lighter cousins. The rates of these decay processes are related to a set of numbers called the Cabibbo-Kobayashi-Maskawa (CKM) matrix, named for the three physicists who introduced it. The numbers are often shown in a graphical form called the unitarity triangle.
The CKM matrix gives rise to CP violation, the subtle difference between matter and antimatter. The area of the triangle is a measure of the amount of CP violation caused by the weak force. This CP violation partly explains why we live in a matter-dominated universe rather than one full of antimatter or radiation.
Experiments at many different laboratories are examining weak decay processes to determine the angles and the lengths of the sides of the triangle. The red blob surrounding the peak of the triangle represents the constraint obtained by combining all measurements: the smaller the blob, the better the physicists’ understanding of the location of the peak, the shape and area of the triangle, and hence the weak force.
|
Looking for new physics
Currently, all measurements of the unitarity triangle are consistent with the peak lying somewhere within the red-outlined region. By improving the current measurements and performing new ones, scientists will reduce the size of this allowed region, measuring the position of the vertex ever more precisely. If any experimental result is inconsistent with this vertex, scientists have evidence that the CKM picture of the weak force is incomplete. Such a discovery would overhaul our current understanding of the weak force, and provide us with a glimpse of new physics that may have played a role in the evolution of the early universe.
Michael Mazur, Istituto Nazionale di Fisica Nucleare (INFN), Pisa
Click here to download the pdf version of this article.


