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Physical Review A

Evaporative cooling of magnetically trapped atomic molybdenum

Cindy Hancox, Matthew T. Hummon, Scott V. Nguyen, John M. Doyle

Published Mar 11, 2005• 14 citations
Publisher

Abstract

We have magnetically trapped and evaporatively cooled atomic molybdenum. Using a cryogenic helium buffer gas, $2\ifmmode\times\else\texttimes\fi{}{10}^{10}$ molybdenum atoms are loaded into a magnetic trap at an initial temperature of 500 mK. The molybdenum atoms undergo two-body decay with a measured inelastic rate constant of ${g}_{\mathrm{in}}=(1.2\ifmmode\pm\else\textpm\fi{}0.6)\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}12}\phantom{\rule{0.3em}{0ex}}{\mathrm{cm}}^{3}\phantom{\rule{0.2em}{0ex}}{\mathrm{s}}^{\ensuremath{-}1}$ for the initial conditions after loading. The molybdenum atoms are cooled by adiabatic expansion and forced evaporation to 200 mK.

DOI
10.1103/physreva.71.031402

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We report the magnetic trapping and evaporative cooling of bosonic and fermionic isotopes of atomic chromium. Using a cryogenic helium buffer gas, 1012{10}^{12}1012 chromium atoms are trapped at an initial temperature of \ensuremath{\sim}1 K. The chromium atoms are then cooled adiabatically and evaporatively to temperatures as low as \ensuremath{\sim}10 mK. Elastic and inelastic 52Cr{}^{52}\mathrm{Cr}52Cr collisional cross sections are measured over this temperature range. Prospects for simultaneously creating a 52Cr{}^{52}\mathrm{Cr}52Cr Bose-Einstein condensate and 53Cr{}^{53}\mathrm{Cr}53Cr Fermi degenerate gas will be discussed.
We report the magnetic trapping and evaporative cooling of bosonic and fermionic isotopes of atomic chromium. Using a cryogenic helium buffer gas, 10 1 2 chromium atoms are trapped at an initial temperature of ∼ 1 K. The chromium atoms are then cooled adiabatically and evaporatively to temperatures as low as ∼10 mK. Elastic and inelastic 5 2 Cr collisional cross sections are measured over this temperature range. Prospects for simultaneously creating a 5 2 Cr Bose-Einstein condensate and 5 3 Cr Fermi degenerate gas will he discussed.
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Metastable helium is buffer gas cooled, magnetically trapped, and evaporatively cooled in large numbers. 1011{10}^{11}1011 4He∗^{4}\mathrm{He}^{*}4He∗ atoms are trapped at an initial temperature of 400mK400\phantom{\rule{0.3em}{0ex}}\mathrm{mK}400mK and evaporatively cooled into the ultracold regime, resulting in a cloud of $2\ifmmode\pm\else\textpm\fi{}0.5\ifmmode\times\else\texttimes\fi{}{10}^{9}$ atoms at $1.4\ifmmode\pm\else\textpm\fi{}0.2\phantom{\rule{0.3em}{0ex}}\mathrm{mK}$. Efficient evaporation indicates low collisional loss for 4He∗^{4}\mathrm{He}^{*}4He∗ in both the ultracold and multi-partial-wave regime, in agreement with theory.
Atomic manganese 55Mn^{55}\mathrm{Mn}55Mn and chromium 52Cr^{52}\mathrm{Cr}52Cr are simultaneously loaded and confined in a magnetic trap. Using a cryogenic 3He^{3}\mathrm{He}3He buffer gas, 1011{10}^{11}1011 manganese and 1012{10}^{12}1012 chromium atoms are trapped at an initial temperature of 600 mK. The buffer gas is then pumped away, thermally isolating the sample. The Mn-Cr interspecies inelastic rate constant is measured to be ${\ensuremath{\Gamma}}_{\mathrm{Mn},\mathrm{Cr}}=1.5(\ifmmode\pm\else\textpm\fi{}0.2)\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}13}\phantom{\rule{0.2em}{0ex}}{\mathrm{cm}}^{3}∕\mathrm{s}$.
We describe a method for loading paramagnetic atoms or molecules into a magnetic trap. A 3He^{3}\mathrm{He}3He buffer gas is employed to thermalize atoms or molecules to a temperature of approximately 240 mK, lower than the depth of the trap. A model is described that indicates an initial loading density of approximately 1013{10}^{13}1013 ${\mathrm{cm}}^{\ensuremath{-}3}$. Once loading has taken place the buffer gas is removed by cryopumping. Evaporative cooling can then be applied to further lower the temperature and increase the density of the trapped sample.