Gostota stanj in stisljivost elektronskega plina

Iz Fizika trdne snovi 2007 - 2008

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Stisljivost

Stisljivost opazovanega sistema je količina, ki pove, za koliko se mu zmanjša prostornina V, če malo povečamo tlak p, v primerjavi z začetno prostornino:

\chi = -\frac{1}{V} \frac{\partial V}{\partial p}.

V tem primeru bo prikladneje izračunati njeno obratno vrednost - modul stisljivosti K

K = \frac{1}{\chi} = -V \frac{\partial p}{\partial V},

saj bomo tlak dobili iz definicije

p = - \frac{\partial E}{\partial V},

torej iz povečanja energije sistema E ob zmanjšaju njegove prostornine. Energijo izračunamo tako, da seštejemo prispevke vseh delcev. Ti pri temperaturi T = 0 zasedajo stanja do Fermijeve energije εF:

E = \int_0^{\varepsilon_F} g(\varepsilon) \varepsilon d\varepsilon = \frac{2}{5} \frac{\sqrt{2m^3}}{\pi^2\hbar^3} V\varepsilon_F^{5/2},

kjer pa je tudi Fermijeva energija odvisna od prostornine. V k prostoru N delcev zaseda stanja do kF, ki ustreza εF:

N = 2 \frac{V_{kF}}{V_{k0}} = 2 \frac{4\pi k_F^3}{3} \Bigl(\frac{L}{2\pi}\Bigr)^3  = \frac{V k_F^3}{3\pi^2},

od koder lahko izrazimo Fermijev valovni vektor in ga nadomestimo s Fermijevo energijo

\varepsilon_F = \frac{\hbar^2 k_F^2}{2m}= \frac{\hbar^2}{2m} \Bigl(3\pi^2 \frac{N}{V}\Bigr)^{2/3}.

Ko dobljeno vstavimo nazaj v izraz za celotno energijo, ostane

E = \frac{3}{5}\varepsilon_F N \propto V^{-2/3}.

Tlak sedaj dobimo z odvajanjem energije

p = + \frac{3}{5}\frac{2}{3}\varepsilon_F\frac{N}{V} = \frac{2}{5} \varepsilon_F n \propto V^{-5/3},

kjer je n številska gostota delcev. Stisljivostni modul sledi s še enim odvodom

K = + V \frac{2}{5}\frac{5}{3}\varepsilon_F\frac{N}{V^2} = \frac{2}{3} \varepsilon_F n = \frac{5}{3}p.


V dveh oz. eni razsežnosti je ob upoštevanju drugačne gostote stanj in smiselno spremenjenih definicijah tlaka in stisljivosti postopek povsem enak. Rezultati so zbrani v spodnji preglednici.


Povzetek

3D 2D 1D
n \ \frac{N}{V} \frac{N}{S} \frac{N}{L}
g(\varepsilon) \frac{V\sqrt{2m^3\varepsilon}}{\pi^2 \hbar^3} \frac{Sm}{\pi\hbar^2} \frac{L}{\pi\hbar} \sqrt{\frac{2m}{\varepsilon}}
\varepsilon_F \frac{\hbar^2}{2m} (3\pi^2 n)^{2/3} \frac{\pi\hbar^2}{m} n \frac{\pi\hbar^2}{8m} n^2
E \ \frac{3}{5} \varepsilon_F N \frac{1}{2} \varepsilon_F N \frac{1}{3} \varepsilon_F N
p \ \frac{2}{5} \varepsilon_F n \frac{1}{2} \varepsilon_F n \frac{2}{3} \varepsilon_F n
K \ \frac{5}{3} p 2p \ 3p \