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Three-Body Recombination in Cold Atomic Gases

PhD-defense by

Peder Klokmose Sørensen


Tuesday September 17th, 2013

Supervisors:
Dmitri V. Fedorov
Aksel S. Jensen

Department of Physics
and Astronomy
Aarhus University

Outline

Introduction

The problem:

  • System of cold atoms in a trap
  • Interactions lead to losses

The question:

  • How to describe the interactions?

The fun part:

  • Three-body physics
  • Efimov physics

The guy:

Vitaly Efimov

r12

r23

r13

1

2

3

x1

y1

x2

y2

x3

y3

Jacobi coordinates

Hyper-spherical coordinates


Cartesian coordinates Jacobi coordinates
\[ \rho^2=x_i^2+y_i^2\quad,\quad \rho\sin(\alpha_i)=x_i\quad,\quad \rho\cos(\alpha_i)=y_i \]

Hyper-spherical coordinates II

\(\alpha\qquad\quad\;\pi\)

\(\rho\qquad\; r_0\)

Zero-range models

\(\psi=cx+d\) \(=c\left(x+\dfrac{d}{c}\right)\) \(\propto x-a\)

\(\dfrac{\psi'}{\psi\phantom{'}}\bigg\vert_{x\,=\,0}\) \(=-\dfrac{1}{a}\) \(+\dfrac{1}{2}Rk^2\)

Bound states

\(-\left\vert E_T^{(n)}\dfrac{2ma_0^{2}}{\hbar^2}\right\vert^{1/8}\)

Efimov spectrum

\(\textrm{sign}(a)\times\left\vert\dfrac{a_0^2}{a^2}\right\vert^{1/8}\)
rvdW /a(-)

Three-body parameter

log10(sres)

Three-body recombination

Three particles collide... ... and form a dimer and a free particle
All particles are lost at a rate given by

\(\dot n = -\alpha_\text{rec}n^3\)
αrec [cm6/s]

Three-body recombination rate

a[a0]
[1] Pollack et. al. Science vol. 326 [2009]
\(\dfrac{\nu_1^2-\frac{1}{4}}{2(\rho/a)^2}\)

Optical potential model

ρ /|a|
αrec [cm6/s]

Finite temperature effects

a[a0]
[1] Pollack et. al. arXiv:1302.0281v2

Mass-imbalanced systems


  • For instance the system of   133Cs – 7Li
  • Mass ratio of ~19 fairly large
  • Scaling ratio reduced down to ~4.8
This leads to almost twice as many interference features in any given scattering length range for for the equal mass system
αrec [ cm6/s ]

Mass imbalanced recombination rate

a [ a0 ]

Thank you for your attention