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Dilute Bose gas in 3D

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Title: Dilute Bose gas in 3D


1
Dilute Bose gas in 3D
  • Wei Bobo
  • Jan 8, 2009

2
Outline
  • Dilute Bose gas.
  • Mean field treatment.
  • Beyond mean field.
  • Pair distribution function.
  • Summary and references.

3
Ideal Bose gas
  • There are two characteristic lengths
  • The mean particle distance
  • Thermal de Broglie wavelength

The number of atoms in the lowest quantum state
is proportional to the so called phase-space
density, and has to exceed a critical number of
2.612 to achieve Bose-Einstein condensation.
4
(No Transcript)
5
Dilute Bose gas
  • Accessible in experiments.
  • Weakly interacting Bose gas
  • There are one more characteristic length range
    of interacting potential
  • At very low temperature, the effective
    interaction can be described by the s wave
    scattering length. which can be considered as
    hard-sphere diameter
  • Dilute condition

6
Effective Hamiltonian
The commonly used effective interaction is
Effective Hamiltonian Where
7
Mean field treatment
8
Mean field
It can not describe the correlations between the
N atoms. The best state given by this variational
approach will describe how the state of each atom
is modified by the mean field of the N-1 other
atoms. So we can use Lagrange multiplier to
get the best single particle state.
9
Mean field
10
Mean field treatment
  • By Minimization procedure
  • This equation describes the evolution of each
    atoms in the trapping potential and in the mean
    field created at its position by the remaining
    N-1 atoms.

11
Mean field treatment
For dilute gases, the potential takes the form
Finally, we have the Gross-Pitaevskii equation
which plays a central role in the study of the
properties of Bose-Einstein condensation.
12
Mean field energy
  • The spatial density
  • The Kinetic energy
  • The Kinetic energy comes from the
    confinement.
  • Trapping energy
  • Interaction energy

13
Mean field ground state energy
  • For the homogenous system we are considering,
    there is no trapping potential, then
  • Total energy
  • Finally, we have mean field ground state energy

14
Beyond mean field
15
Beyond mean field
  • How far does the system differ from the product
    of single particle state?
  • T0, all the particles are not stay at one single
    particle state.
  • What is the number of particles occupy the other
    states?
  • Quantum depletion.
  • Thermal depletion.
  • What is the elementary excitations?

16
Second quantized Hamiltonian
Expand the field operators into free particle
fields
17
Bogoliubov approximation
  • 1. In the dilute gases near T0, the population
    of k0 state is macroscopic compared to the total
    population of the other states.
  • Thus the matrix element of are on
    the order of . We will neglect the non
    commutation of them and make a c-number
    substitution

18
Bogliubov approximation
  • 2. In the interaction terms, there are terms
    including 4,2,0 of , and no terms
    with odd number of due to the
    conservation of momentum.
  • For large value of N we are considering, they
    become three categories in magnitude

19
Effective Hamiltonian
  • By considering terms of categories (1) and (2),
    we would obtain the dominant term of the energy
    of the system
  • This is a quadratic expression of creation and
    annihilation operators, which can be diagonalized
    by Bogoliubov transformation.

20
Bogoliubov transformation
  • Introducing
  • Constrain
  • One have
  • New expressions of the Hamiltonian

21
Bogoliubov transformation
  • In order to diagonalize the Hamiltonian, we must
    have

22
Ground state energy
  • When one evaluate E0, it diverges. This is
    because the potential we have used. When one do
    Fourier transform, it is a constant.
  • To solve this problem, LHY proposed
    pseudo-potential

23
Ground state energy
24
Ground state and excited state
The ground state is that all the oscillators
stay in their ground state, which satisfies
The first excited states with momentum K is
So the quasi-particle appears as a linear
superposition of ordinary particles with momentum
K and ordinary hole with momentum K.
25
Low energy excitations
At low energy excitations, K is very small
So we have obtained the phonon dispersion
relations for the excitations of a weakly
interacting Bose gas. The repulsive interactions
change the elementary excitations at long wave
lengths from free particles to Phonons.
26
Quantum depletion
27
Physical picture of ground state
  • The ground state turns to be a collection of n
    pairs of particles, each pair consists of two
    particles with momentum k and k.
  • Average number of pairs
  • The pairs has a correlation length
  • Within one correlation length, the number of
    particles is, on the average

28
Physical picture of ground state
  • Within one correlations, the number of particles
    have k not equal to 0 is
  • In other words, within one correlation length,
    there are many particles, but only few of them
    with k not equal to 0.

29
Pair distribution function
  • Pair distribution function is defined as
  • Physical meaning of pair distribution function
  • Given a particle at a point, the average
    number of particles in dr at a distance r is
    rouD(r)dr.
  • Thus D(r) extends to 1 as r goes to infinity.
  • It is measurable in experiment.
  • We evaluate D(r) based on the wave function of
    the system.

30
Pair distribution function
31
Summary
  • The mean field gives a good description if the
    system are sufficiently dilute.
  • Beyond mean field can be obtained based on
    Bogliubov approximation.
  • We have evaluated the pair distribution function
    of dilute Bose gas based on the ground state wave
    function.

32
References
  • Lecture notes of BEC by Prof.Cohen-Tannoudji at
    CityU.
  • Bose-Einstein condensation in the alkali gases
    Some fundamental concepts, REVIEWS OF MODERN
    PHYSICS, 73,307 (2001).
  • Statistical mechanics, K. Huang,1987.
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