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Indirect detection of low-mass dark matter through the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mi>π</mml:mi><mml:mn>0</mml:mn></mml:msup></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>η</mml:mi></mml:math> windows
We consider the search for gamma rays produced by the annihilation or decay of low-mass dark matter which couples to quarks. In this scenario, most of the photons are produced from the decays of ${\ensuremath{\pi}}^{0}$ or $\ensuremath{\eta}$ mesons. These decays produce distinctly different photon signatures due to the difference in …