When a negatively charged electron interacts with a positive proton, they do not annihilate like an electron and positron; instead, they can merge to form a neutron under certain conditions. This process occurs during events such as the collapse of a star into a neutron star. In radioactive nuclei, a proton can absorb an atomic electron, emit a neutrino, and transform into a neutron, a phenomenon known as electron capture or K-capture. This interaction highlights the complex behavior of subatomic particles and their transformations. Understanding these processes is crucial for comprehending stellar evolution and nuclear physics.