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PhD thesis in English

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Chapter 1Introduction1.1 ForewordThe essential <strong>in</strong>gredients of the quantum mechanical theory are dual particle-wavenature of the matter, and the notion of identical particles. The quantum <strong>in</strong>dist<strong>in</strong>guishabilityof particles has a profound impact on the statistical properties. Whileparticles with a half-<strong>in</strong>teger sp<strong>in</strong> (fermions) try to avoid each other due to the Pauliexclusionpr<strong>in</strong>ciple, particles with an <strong>in</strong>teger sp<strong>in</strong> (bosons) do not exhibit such restrictionsand are actually, as a consequence of the m<strong>in</strong>imal energy pr<strong>in</strong>ciple, try<strong>in</strong>gto occupy the same s<strong>in</strong>gle-particle ground state. These effects are captured by twodifferent probability distributions that describe the thermal equilibrium <strong>in</strong> the twotypes of physical systems. The Fermi-Dirac distribution for fermions was orig<strong>in</strong>allyderived <strong>in</strong> 1926 by its two authors <strong>in</strong>dependently, while try<strong>in</strong>g to <strong>in</strong>troduce quantizationconcepts <strong>in</strong>to an ideal gas of particles obey<strong>in</strong>g the Pauli exclusion pr<strong>in</strong>ciple.The Bose-E<strong>in</strong>ste<strong>in</strong> distribution for bosons was <strong>in</strong>troduced <strong>in</strong> 1924 by the jo<strong>in</strong>t effortof Bose and E<strong>in</strong>ste<strong>in</strong> [1, 2]. At the time, it was a miss<strong>in</strong>g piece of knowledge for thecomplete explanation of the Planck’s law of black body radiation.In the high-temperature limit, both distributions are well approximated by acommon Maxwell-Boltzmann distribution. The condition necessary for the effectsof the quantum statistics to become observable can be roughly estimated as follows.The non<strong>in</strong>teract<strong>in</strong>g particles of the mass M affect each other if their thermal deBroglie wavelength λ T at temperature T,√2πλ T =2k B TM , (1.1)is comparable to the <strong>in</strong>ter-particle distance given by n −1/3 , where n is a typical particledensity. Naturally, the notion of the “high temperature” and “low temperature”depends on the features of the considered system. For example, electrons <strong>in</strong> a typical1

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