When two nuclei (protons) move closer than atomic size, the strong nuclear force manifests.
The potential energy of the system decreases as the protons approach each other, due to attractive forces.
Start with protons at a significant distance apart (high potential energy).
Initially, protons experience repulsion due to electrostatic forces (Coulombic barrier), causing an increase in potential energy.
As protons get closer, potential energy decreases drastically when strong nuclear force overwhelms electrostatic repulsion.
Correct diagram representation is option C.
Electrostatic forces initially repel protons, making fusion unlikely under normal conditions.
This barrier requires significant energy input to overcome.
After surpassing the Coulombic barrier, the strong nuclear force draws nuclei together, causing potential energy to drop significantly.
Similar to bond formation, energy is released during fusion, termed binding energy.
Nuclear reactions release more energy than chemical reactions, quantified using Einstein's equation E=mc².
Example: Fusing deuterium and tritium produces helium and neutron, with a decrease in total mass, indicating energy release.
Mass defect (difference between calculated and actual mass) results in binding energy, emphasized in E=mc².
For deuterium formation, mass defect = 0.002388 amu.
Energy released by a single deuterium atom calculated as 3.56 x 10⁻¹³ joules.
For one mole of deuterium, energy released = 2.14 x 10¹¹ joules.
This energy is significantly higher than combustion reactions (e.g., methane).
Despite high energy output, fusion needs extreme conditions (temperature and pressure) similar to the sun.
Overcoming the Coulombic barrier in a controlled environment remains a challenge.
Hydrogen burning: Four protons fuse to make helium, releasing energy.
Helium burning: Forms carbon from three helium nuclei.
Hydrogen burning entails a decrease in atom number leading to heavier elements.
Fission: Splitting of heavy atomic nuclei into lighter, more stable ones, releasing energy.
Example: Neutron bombardment on U-235 causes fragmentation into smaller nuclei and more neutrons.
Uncontrolled fission can lead to chain reactions.
Enrichment required for effective nuclear reactions due to low natural U-235 abundance.
Iron has the most stable nucleus structure.
Energy dynamics in nuclei (fusion/fission) depend on the ratio of neutrons to protons.
Occurs spontaneously, involving alpha, beta, and gamma emissions.
Stability band indicates that heavier nuclei require higher neutron ratios; decay aims to reach stability.
Interactions and external conditions dictate how atoms behave (solid, liquid, gas).
Emergent properties arise from collective atomic interactions, not single isolated atoms.
Electrons in molecules dictate properties; changes in phase indicate energy absorption or release.
Energy required to break bonds during phase transitions reflects individual atomic interactions.
Covalent bonds (strong) vs. metallic bonds (which allow for conductivity and malleability).
Molecular orbital theory helps explain material behavior at atomic levels, including electrical conductivity in metals.
Metals shine due to their continuous metallic bond and electron mobility.
Diamond (hard, non-conductive, forms strong covalent bonds) vs. graphite (soft, conducts electricity, contains layers held by London dispersion forces).
Bonding in diamond involves hybridization (sp3) forming tetrahedrally arranged bonds, while graphite has sp2 hybridized carbon with delocalized electrons.