Abstract
Abstract
The physics that determines the line shape of the 1S–2S transition in magnetically trapped
H
¯
is explored. Besides obtaining an understanding of the line shape, one goal is to replace the dependence on large scale simulations of
H
¯
with a simpler integration over well defined functions. For limiting cases, analytic formulas are obtained. Example calculations are performed to illustrate the limits of simplifying assumptions. We also describe a χ
2 method for choosing experimental parameters that can lead to the most accurate determination of the transition frequency.
Subject
Condensed Matter Physics,Atomic and Molecular Physics, and Optics