Difference between revisions of "Search for CP violation in the gamma-ray sky"
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[[File:Combinedjan14z100bgt80.jpg|600px]] | [[File:Combinedjan14z100bgt80.jpg|600px]] | ||
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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. | ||
Revision as of 12:32, 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
(Ferrer's routines)
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.
