Difference between revisions of "Search for CP violation in the gamma-ray sky"
From magneticfields
(→Results) |
(→Results) |
||
| Line 30: | Line 30: | ||
[[File: Q_Rad_80_clean_jan.jpg|200px]] | [[File: Q_Rad_80_clean_jan.jpg|200px]] | ||
[[File:Combinedjan14z100bgt80.jpg|600px]] | [[File:Combinedjan14z100bgt80.jpg|600px]] | ||
| − | |||
| − | CP odd statistics, Qx10^-6, versus patch radius R in degrees for the 6 different energy (E1,E2) combinations. E3 is always taken to be 50 GeV. | + | CP odd statistics, Qx10^-6, versus patch radius R in degrees for the 6 different energy (E1,E2) combinations. E3 is always taken to be 50 GeV. On the left are results of Tashiro's routines; on the right are results obtained using Ferrer's routines. |
Revision as of 12:34, 19 May 2014
Contents
Schema
Illustration of the cut-sky with gamma rays distributed on it. Patches of radius R
degrees are centered on the highest energy gamma rays. In those patches we
test if the lower energy photons are distributed along left- or right-handed spirals.
Fermi Data
Galactic Latitude and Source Cuts
Galactic latitude and Source Cuts
Evaluation of Q Statistic
Mathematica notebook: File:Cpgamma-northsouth.nb
Monte Carlo Simulations
Results
CP odd statistics, Qx10^-6, versus patch radius R in degrees for the 6 different energy (E1,E2) combinations. E3 is always taken to be 50 GeV. On the left are results of Tashiro's routines; on the right are results obtained using Ferrer's routines.
