Ang Li

The atomic nucleus is not a solid ball but a drop of liquid that can be squeezed. To understand how elastic it is, physicists accelerate gold nuclei and smash them into each other. On impact, the matter compresses to densities like those in a neutron star, then flies apart. The shape of this debris tells us about the properties of the matter inside.

The brain of a person with Parkinson's disease works like an orchestra where the conductor either freezes or waves the baton off-beat. Medications don't help everyone, so doctors turn to stimulation — weak electrical pulses that restore the rhythm.

The proton looks like a solid ball, but inside it's a hive of activity: quarks exchange gluons — the particles that bind them together. Gluons pop in and out of existence, and their distribution within the proton is not just a curious detail but a key to predictions at the Large Hadron Collider.

A neutron star is the core left behind after a massive star explodes. Its matter is so compressed that a teaspoonful would weigh billions of tons. But the exact size and mass of such objects remain debated. A team of astronomers studied the system EXO 0748-676, where a neutron star pulls matter from a normal companion star. It occasionally flares up and then quiets down.

Pulsar PSR J1637−4642 is like a drum with a ratchet: it spins at enormous speed, and each radio flash is a click marking time. For nine and a half years, astronomers listened to this rhythm on the 64-meter Murriyang telescope in Australia, and heard not a single skip. The mechanism seemed to work flawlessly.