Optical Trapping of Atoms: Characterization and Optimization Charlie Fieseler University of Kentucky UW REU 2011 Subhadeep Gupta.

Slides:



Advertisements
Similar presentations
Outline Index of Refraction Introduction Classical Model
Advertisements

18th International IUPAP Conference on Few-Body Problems in Physics Santos – SP – Brasil - Agosto Global variables to describe the thermodynamics.
Light Waves and Polarization Xavier Fernando Ryerson Communications Lab
Adnan Doyuran a, Joel England a, Chan Joshi b, Pietro Musumeci a, James Rosenzweig a, Sergei Tochitsky b, Gil Travish a, Oliver Williams a a UCLA/Particle.
Ultracold Quantum Gases: An Experimental Review Herwig Ott University of Kaiserslautern OPTIMAS Research Center.
Natural Broadening From Heisenberg's uncertainty principle: The electron in an excited state is only there for a short time, so its energy cannot have.
Geonium A Fake but Useful Atom BoBo. Overview What is Geonium and why is it useful? A little bit of history What is a Penning trap? Penning trap components.
The Sum Over States model, although exact, requires a detailed knowledge of many parameters which are not generally available. Experience has shown that.
Light and Matter Tim Freegarde School of Physics & Astronomy University of Southampton The tensor nature of susceptibility.
The Bose-Einstein Condensate Jim Fung Phys 4D Jim Fung Phys 4D.
Non-Equilibrium Dynamics in Ultracold Interacting Atoms Sergio Smith (Howard University) Simulations of Ultracold Atoms in Optical Lattices.
Ultracold Atoms, Mixtures, and Molecules
Lecture 8: Measurement of Nanoscale forces II. What did we cover in the last lecture? The spring constant of an AFM cantilever is determined by its material.
World of ultracold atoms with strong interaction National Tsing-Hua University Daw-Wei Wang.
c = km/sec I F = I 0 x (cosθ) 2.
Danielle Boddy Durham University – Atomic & Molecular Physics group Red MOT is on its way to save the day!
Observation of universality in 7 Li three-body recombination across a Feshbach resonance Lev Khaykovich Physics Department, Bar Ilan University,
Hyperfine Studies of Lithium using Saturated Absorption Spectroscopy Tory Carr Advisor: Dr. Alex Cronin.
Shock Waves & Potentials
Guillermina Ramirez San Juan
Quantum Computation Using Optical Lattices Ben Zaks Victor Acosta Physics 191 Prof. Whaley UC-Berkeley.
LESSON 4 METO 621. The extinction law Consider a small element of an absorbing medium, ds, within the total medium s.
Ultracold Plasmas ( Zafar Yasin). Outline - Creation and why considered important? - Characterization. - Modeling. -My Past Research. - Current Research.
Lecture II Non dissipative traps Evaporative cooling Bose-Einstein condensation.
On the path to Bose-Einstein condensate (BEC) Basic concepts for achieving temperatures below 1 μK Author: Peter Ferjančič Mentors: Denis Arčon and Peter.
1 Bose-Einstein Condensation PHYS 4315 R. S. Rubins, Fall 2009.
1 射电天文基础 姜碧沩北京师范大学天文系 2009/08/24-28 日,贵州大学. 2009/08/24-28 日射电天文暑期学校 2 Spectral Line Fundamentals The Einstein Coefficients Radiative Transfer with Einstein.
Bose-Einstein Condensate Fundaments, Excitation and Turbulence Vanderlei Salvador Bagnato Instituto de Física de São Carlos – Universidade de São Paulo.
Anharmonic Oscillator Derivation of Second Order Susceptibilities
Colleen Downs Stephanie Pietromonaco Sanjay Talluri
Building a Photodetector to Observe the Polarization of Light Kevin J. McElwee Bridgewater State University, Bridgewater MA Mentor: Edward F. Deveney.
Studying dipolar effects in degenerate quantum gases of chromium atoms G. Bismut 1, B. Pasquiou 1, Q. Beaufils 1, R. Chicireanu 2, T. Zanon 3, B. Laburthe-Tolra.
Vibrational and Rotational Spectroscopy
Optical Lattices 1 Greiner Lab Winter School 2010 Florian Huber 02/01/2010.
Determination of fundamental constants using laser cooled molecular ions.
Spectroscopy of a forbidden transition in a 4 He BEC and a 3 He degenerate Fermi gas Rob van Rooij, Juliette Simonet*, Maarten Hoogerland**, Roel Rozendaal,
High-performance Apparatus for Bose-Einstein Condensation of Rubidium Yoshio Torii Erik Streed Micah Boyd Gretchen Campbell Pavel Gorelik Dominik Schneble.
Buffer Gas Cooling of atomic and molecular beams Wenhan Zhu Princeton University 11/06/2007.
Photoassociation Spectroscopy of Ytterbium Atoms with Dipole-allowed and Intercombination Transitions K. Enomoto, M. Kitagawa, K. Kasa, S. Tojo, T. Fukuhara,
Laser Cooling/Trapping of atoms We will discuss this in more detail toward the end of the semester, but it is possible to slow-down (cool) atoms by passing.
Collective excitations in a dipolar Bose-Einstein Condensate Laboratoire de Physique des Lasers Université Paris Nord Villetaneuse - France Former PhD.
Critical stability of a dipolar Bose-Einstein condensate: Bright and vortex solitons Sadhan K. Adhikari IFT - Instituto de Física Teórica UNESP - Universidade.
Spin-statistics theorem As we discussed in P301, all sub-atomic particles with which we have experience have an internal degree of freedom known as intrinsic.
Obtaining Ion and Electron Beams From a source of Laser-Cooled Atoms Alexa Parker, Gosforth Academy  Project Supervisor: Dr Kevin Weatherill Department.
Effect of Temperature on Magnetic Field Measurements Doug Hockey 1, Brendan Van Hook 1, Ryan Price 2 Sponsored by the Department of Physics, University.
Experimental study of Efimov scenario in ultracold bosonic lithium
Stefan Truppe MM-Wave Spectroscopy and Determination of the Radiative branching ratios of 11 BH for Laser Cooling Experiments.
Prospects for ultracold metastable helium research: phase separation and BEC of fermionic molecules R. van Rooij, R.A. Rozendaal, I. Barmes & W. Vassen.
Toward a Stark Decelerator for atoms and molecules exited into a Rydberg state Anne Cournol, Nicolas Saquet, Jérôme Beugnon, Nicolas Vanhaecke, Pierre.
-Plasma can be produced when a laser ionizes gas molecules in a medium -Normally, ordinary gases are transparent to electromagnetic radiation. Why then.
Bose-Einstein Condensation (a tutorial) Melinda Kellogg Wyatt Technology Corporation Santa Barbara, CA June 8, 2010.
Laser Cooling and Trapping Magneto-Optical Traps (MOTs) Far Off Resonant Traps (FORTs) Nicholas Proite.
Duke University, Physics Department and the Fitzpatrick Institute for Photonics · Durham, NC Collective Nonlinear Optical Effects in an Ultracold Thermal.
Laser Cooling/Trapping of atoms We will discuss this in more detail toward the end of the semester, but it is possible to slow-down (cool) atoms by passing.
Condensed matter physics in dilute atomic gases S. K. Yip Academia Sinica.
State Scientific Center of the Russian Federation National Research Institute for Physical-Technical and Radio Engineering Measurements Progress in deep.
Bose-Einstein Condensates The Coldest Stuff in the Universe Hiro Miyake Splash! November 17, 2012.
Waves We talked about the motion of bodies, such as planets and baseballs. At the most fundamental level, one has elementary particles (electrons, quarks).
Jerzy Zachorowski M. Smoluchowski Institute of Physics, Jagiellonian University Nonlinear Spectroscopy of Cold Atoms, Preparations for the BEC Experiments.
Dipolar relaxation in a Chromium Bose Einstein Condensate Benjamin Pasquiou Laboratoire de Physique des Lasers Université Paris Nord Villetaneuse - France.
Functional Integration in many-body systems: application to ultracold gases Klaus Ziegler, Institut für Physik, Universität Augsburg in collaboration with.
Ultracold gases Jami Kinnunen & Jani-Petri Martikainen Masterclass 2016.
Laser Cooling and Trapping
Raman Effect The Scattering of electromagnetic radiation by matter with a change of frequency.
Laser Cooling and Trapping
Chapter 1 Electromagnetic Fields
B. Liu, J. Goree, V. Nosenko, K. Avinash
Dan Mickelson Supervisor: Brett D. DePaola
Bose-Einstein Condensation Ultracold Quantum Coherent Gases
Cold Atom project 12/02/2019.
Presentation transcript:

Optical Trapping of Atoms: Characterization and Optimization Charlie Fieseler University of Kentucky UW REU 2011 Subhadeep Gupta

So… why? Studying superfluid/degenerate gas properties –Two species, Lithium and Ytterbium, can use one as a probe –Condensed matter simulations Molecule formation, specifically polar –Quantum computing in a lattice Fundamental physics, of course –Fine structure constant measurement through Yb BEC atom interferometry –Electric dipole moment of electron

Getting Cool Atoms: Laser cooling Zeeman Slower –absorbs on-resonance light in the atom’s frame of reference, with a magnetic field to counteract Doppler MOT (also using Zeeman effect) –A 3D trap that catches the cooler atoms –Oppositely polarized light is preferentially absorbed After compression, ends up: –>10^6 atoms at ~20 μK

Getting Cold Atoms Using an optical dipole trap (ODT), cool evaporatively (two step) >2*10^4 Yb atoms below ~170nK (critical temperature), and can go below 30nK >10^4 Li atoms below ~300nK, and can go below 100nK With both species, can cool sympathetically (different trap depths)

Optical Dipole Trap

ODT (cont.) The atoms are high-field seeking, i.e. optical tweezers None of the other measurements make any sense unless you know the waist and position of the focus Cameras are usually used, but they can be quite expensive and (firsthand) very unreliable Do something simple: razorblade

A different method of beam profiling A more conventional method scans perpendicular to the beam –This is not very sensitive to small waists –Hard to know where the minimum is For the proof of concept, the beam is single-mode with a Gaussian shape –A scan along the axis of propagation can measure small waists with <5% error

The shape of the beam This method can also measure deviations from a Gaussian shape A Gaussian intensity function gives the power by integrating:

Setup: single-mode fiber

Setup: “razor” blade

3D Power as a function of razor position zx P

It really does fit well!

Progression of plots

Modeling the trap geometry What do you want the waists to be? In reaching degeneracy, trapping frequencies (i.e. of an harmonic oscillator) are key:

Optimizing (or at least a first guess) Symmetrical makes the most sense: same power, circular, same size But then gravity… poof, nonlinear Harder to model, but there are some theoretical benefits –Weaken dependence of frequency on trap depth: if gravity were tunable, could get down to.075 from.5

Effects of Gravity To the right: Trap at 10W and.25W The trap becomes dominated by gravity at low power: two effects –Lower exponent –Smaller curvature and therefore coefficients

Trap depth vs. frequency

The aforementioned first guess The trap disappears in one dimension before the others The power in that beam should be held at a minimum, while the other beam continues the evaporation Gravity is not a large enough effect to break the symmetry earlier

Next steps Actually build this setup! –Will be used for a Ytterbium BEC interferometry experiment The curves shown do not really show a benefit, but other tweaks need to be tested.

References 05/ v1.pdfhttp://lanl.arxiv.org/PS_cache/arxiv/pdf/11 05/ v1.pdf NWAPS 2010 (Walla Walla, WA) Invited Talk by Deep GuptaNWAPS 2010 (Walla Walla, WA) Invited Talk by Deep Gupta ex1.html