nukleoszintézisek
Nukleoszintézis refers to the process by which atomic nuclei are created within stars and other cosmic environments. It is a fundamental concept in astrophysics that explains the origin of all the chemical elements heavier than hydrogen and helium, which were formed during the Big Bang. The primary mechanism for nucleosynthesis is nuclear fusion, where lighter atomic nuclei combine to form heavier ones, releasing vast amounts of energy.
In stars, nucleosynthesis begins with the fusion of hydrogen nuclei into helium. This process, known as stellar
When massive stars reach the end of their lives, they undergo supernova explosions. These cataclysmic events
The study of nucleosynthesis is crucial for understanding the composition of the universe, the evolution of