Expert reviewed • 22 November 2024 • 5 minute read
Einstein's discovery that mass and energy are interchangeable forms of the same fundamental quantity revolutionized our understanding of physics. This principle, expressed through the famous equation , explains phenomena ranging from nuclear reactions in stars to particle physics interactions.
In Einstein's special relativity, mass and energy are equivalent and interchangeable. This relationship is expressed by the equation:
Where:
For practical calculations, we often use alternative units:
The Sun generates energy through nuclear fusion, primarily through two processes:
[Insert PP-Chain Diagram]
In this process, four hydrogen nuclei (protons) combine to form one helium nucleus. The mass difference between reactants and products converts to energy:
The nuclear equation for this process is:
\4 ^1H \rightarrow ^4He + 2e^+ + 2\nu_e + 2\gamma$$
This cycle uses carbon, nitrogen, and oxygen as catalysts to facilitate hydrogen fusion. The net result is identical to the proton-proton chain: four hydrogen nuclei combine to form one helium nucleus.
When an electron meets its antiparticle (positron), they annihilate to produce two gamma-ray photons:
Each photon carries energy of 0.511 MeV, for a total energy of:
The annihilation of protons and antiprotons is more complex due to their composite nature. The total energy released is:
In chemical reactions like combustion, the mass difference between reactants and products is much smaller than in nuclear reactions. For example, the combustion of octane:
The mass difference, while present, is typically too small to measure directly with conventional equipment.