A new study by scientists from the University of Southampton’s School of Mathematics explains how the spin of a pulsar slows down as the star gets older. This composite image shows the Crab pulsar, a neutron star about 28–30 km across, at the center of the Crab Nebula. The new mathematical model, developed by Southampton scientists, can explain the observed behavior of young pulsars, such as the 958-year-old Crab pulsar (X-ray: NASA / CXC / SAO...
