In beta-minus (\( \beta^- \)) decay, a neutron in the nucleus transforms into a proton, emitting an electron and an antineutrino (\(\bar{\nu}\)).
The reaction follows: \[ n \rightarrow p + e^{-} + \bar{\nu} \] The antineutrino is emitted to ensure the conservation of energy, angular momentum, and lepton number.
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of