Article ID Journal Published Year Pages File Type
1874897 Physics Procedia 2012 4 Pages PDF
Abstract

The underlying magnetic field distribution in many samples studied by the μSR technique is asymmetric. Despite this, quite often fit functions assuming symmetric (Gaussian) distributions are used. Here, a back-to-back exponential function, which can be made asymmetric with fit parameters, is studied numerically alongside a Gaussian function to see how well each fits symmetric and asymmetric simulated data. Both fit symmetric data well, but the back-to-back exponential is found to be superior for fitting asymmetric data.

Related Topics
Physical Sciences and Engineering Physics and Astronomy Physics and Astronomy (General)