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=== Assistant: Condensed version of your question: === Condensed version of your question: What physically attracts two atoms into forming a bond, why do they not bond at long distance, and what exact event/threshold triggers the reaction? ==== At the most fundamental level, the attraction comes from the Coulomb force within the electron–nucleus system: ==== F=14πϵ0q1q2r2F = \frac{1}{4\pi\epsilon_0}\frac{q_1 q_2}{r^2}F=4πϵ01r2q1q2 Specifically: * The electrons of one atom are attracted to the nucleus of the other. * If the electronic wavefunctions overlap constructively, the system can reorganize into a lower-energy quantum state (a molecular orbital). This attraction competes with: * electron–electron repulsion * nucleus–nucleus repulsion A bond forms only if the net energy decrease (from electron–nucleus attraction + quantum delocalization) outweighs the repulsive terms. ==== Because at long distances: ==== * The electron wavefunctions do not overlap significantly. * The Coulomb attraction between nuclei and the other atom’s electrons falls off as 1/r21/r^21/r2. * The system’s quantum mechanical state remains essentially the direct product of isolated atomic orbitals. Without overlap, there's no possibility of forming a lower-energy molecular eigenstate—so there is no bond, just weak long-range interactions (van der Waals, dispersion). Mathematically: S=⟨ψA∣ψB⟩≈0⇒no bonding orbital availableS = \langle \psi_A | \psi_B \rangle \approx 0 \quad \Rightarrow \quad \text{no bonding orbital available}S=⟨ψA∣ψB⟩≈0⇒no bonding orbital available ==== Bonding becomes energetically favorable when electron wavefunction overlap becomes non-zero. ==== This occurs when interatomic separation approaches approximately one Bohr radius scale (10⁻¹⁰ m)—in practice, when atoms are close enough that the overlap integral SSS is significant. At this distance: * The bonding molecular orbital becomes lower in energy than the separated-atom state. * The system now has a quantum mechanically available state that is lower in total energy. This distance is where the attractive part of the potential energy curve dominates. ==== Two things must happen simultaneously: ==== ===== Atoms must be close enough that: ===== ΔE=Ebonded−Eseparate<0\Delta E = E_{\text{bonded}} - E_{\text{separate}} < 0ΔE=Ebonded−Eseparate<0 That is: a lower-energy quantum state becomes available. ===== To transition into the lower-energy state, the system must shed energy: ===== * via photon emission * via collisions with nearby particles * via redistribution into vibrational/rotational kinetic energy If the excess energy cannot be removed, the atoms approach → accelerate → and then rebound (like charged elastic balls). So the key trigger is: : Without dissipation, bonding cannot complete. This is why: * cold atoms bond more easily than hot ones * chemistry slows at low pressure * catalysts don't force bonding—they provide energy pathways and intermediate states ==== If the atoms get too close, then: ==== * nucleus–nucleus repulsion rises steeply (Coulomb) * Pauli exclusion forces the electron wavefunctions into antibonding configurations So the total energy curve looks like: <syntaxhighlight>Energy │ ↑ Pauli + nuclear repulsion │ / │ / ← too close → repulsive │ / │ / minimum (bond length) │ / │ / ← attractive region where bond forms │ / │ / │/ _______________________________________ distance → far apart (no overlap) </syntaxhighlight> ==== Two atoms form a bond when they come close enough for their electron wavefunctions to overlap, allowing a lower-energy molecular orbital to exist, and when the system can dissipate the excess energy; before that critical distance there is no significant attraction, and past the equilibrium distance repulsive forces dominate. ==== If you'd like, next step could be: * A full Lennard-Jones/Morse potential derivation * A simulation with actual overlap integrals * How chemistry differs for ionic, covalent, and metallic cases when viewed at this fundamental level Which direction do you want to go?
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