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PhD thesis in English

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Summations <strong>in</strong> the last expression can be exactly performed only numerically, so <strong>in</strong>order to proceed further <strong>in</strong> an analytic way, we use a semiclassical approximation [19,5]. Practically, this means that we neglect the discretness of energy levels and replacesummations by the <strong>in</strong>tegrals over now cont<strong>in</strong>uous n x , n y and n z . Mathematicallyspeak<strong>in</strong>g, the approximation is justified if the values of the functions which wesum over do not vary significantly over the summation step. For the Eq. (1.7), thementioned condition translates <strong>in</strong>to the high-temperature limit k B T ≫ (E n+1 −E n ),where the thermal energy is larger than the typical spac<strong>in</strong>g of energy levels. Withthis simplification, we obta<strong>in</strong>:N ≈===∫ ∞ ∫ ∞ ∫ ∞0∞∑0∏m=1 j=x,y,z0∫ ∞0dn x dn y dn ze β0 c (ωxnx+ωyny+ωznz) − 1dn j e −β0 c mω jn j1 ∑ ∞1(βc 0)3 ω x ω y ω z m 3m=11(β 0 c) 3 ω x ω y ω zζ 3 , (1.8)where we <strong>in</strong>troduce the Bose function (the polylogarithm function) ζ α (x) = ∑ ∞ x nn=1 n αand the abbreviation ζ α ≡ ζ α (1) for the Riemann zeta function. From the lastexpression, we f<strong>in</strong>d that the condensation sets <strong>in</strong> for:k B Tc 0 = ¯ω N 1/3 , (1.9)ζ 1/33where ¯ω is a geometric mean ¯ω = (ω x ω y ω z ) 1/3 . Consequently, we dist<strong>in</strong>guish thephase with a macroscopic occupation of the ground state and denote it as the condensatephase, and the phase without a macroscopic value of N 0 that is designatedas the (normal) gas phase. However, the phase transition is well def<strong>in</strong>ed only <strong>in</strong> thethermodynamic limit [5, 20] and hence <strong>in</strong> the case of f<strong>in</strong>ite-size systems we refer toT 0 cas the condensation temperature <strong>in</strong>stead of the critical temperature.The BEC phase transition is usually depicted <strong>in</strong> the phase diagram show<strong>in</strong>g thecondensate fraction N 0 /N versus temperature. From Eq. (1.8), we <strong>in</strong>fer that <strong>in</strong> thecondensate phase, the number of atoms <strong>in</strong> the thermal component is proportional5

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