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34 CHAPTER 3. FROM ATOMS TO SOLIDS<br />

Figure 3.1: Two dipoles represent model atoms that are arranged along a line, with the positive<br />

charges (+e) fixed at the positions 0, R, and the negative charges (-e) at the points x 1 , R + x 2 .<br />

If the atoms move together so that the electron charge distributions begin to overlap, repulsive<br />

forces come into play. While there is <strong>of</strong> course a contribution from the direct electrostatic<br />

repulsion <strong>of</strong> the electrons, more important is the Pauli exclusion principle that prevents two<br />

electrons having their quantum numbers equal. The effect <strong>of</strong> Pauli exclusion can be seen by an<br />

extreme example, <strong>of</strong> overlapping two Hydrogen atoms entirely, with the electrons for simplicity<br />

assumed to be in the same spin state. In this case, while two separated atoms may be both in<br />

the 1S ground state, the combined molecule must have a configuration 1s2s, and thus is higher<br />

by the promotion energy.<br />

Calculations <strong>of</strong> the repulsive interaction are complex but the answer is clearly short-ranged.<br />

They are <strong>of</strong>ten modelled empirically by an exponential form e −R/Ro , or a power law with a<br />

large power. A commonly used empirical form to fit experimental data on inert gases is the<br />

Lennard-Jones potential<br />

with A and B atomic constants obtained from gas-phase data.<br />

U(R) = − A R 6 + B R 12 (3.3)<br />

With the exception <strong>of</strong> He, the rare gases from close-packed (face-centered cubic) solids with<br />

a small cohesive energy, and low melting temperatures. Helium is special because zero-point<br />

motion <strong>of</strong> these light atoms is substantial enough that they do not solidify at zero pressure<br />

down to the absolute zero <strong>of</strong> temperature. The quantum fluids 3 He and 4 He have a number <strong>of</strong><br />

extraordinary properties, including superfluidity.<br />

Ionic Crystals<br />

Given the stability <strong>of</strong> the electronic configurations <strong>of</strong> a rare gas, atoms that are close to a filled<br />

shell will have a tendency to lose or gain electrons to fill the shell.<br />

• The energy for the reaction M− > M + + e − in the gas phase is called the ionization<br />

energy I.<br />

• The energy for the reaction X + e − − > X − in the gas phase is called the electron affinity<br />

A.<br />

• The cohesion <strong>of</strong> an ionic molecule can overcome the energy cost I + A by the electrostatic<br />

attraction, e 2 /R

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