The Photino Induced Distortion of the CMBR Blackbody Spectrum
classification
🌌 astro-ph
hep-ph
keywords
distortionphotinoboundcmbrmassspectrumamplitudeblackbody
read the original abstract
It is shown that photon--photino inter-conversions (if exist) may result in a detectable CMBR spectrum distortion which amplitude depends on photino properties, such as its mass. An upper bound on the distortion parameter determined from the recent COBE-FIRAS data, hence, sets a lower bound on the photino mass, $m_{\tilde\gamma} \gtrsim 300 eV$.
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