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Talk1 h 14 min

The cosmic optical background excess, line-intensity mapping

Marc Kamionkowski · CERN

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About

Recently, the New Horizons spacecraft was able to detect, for the first time, the cosmic background of optical light. The signal was twice that expected from galaxy number counts. This excess can be explained in terms of two-photon decay of a dark-matter axion, a hypothesis that will be tested with line-intensity mapping very high significance with the impending launch of NASA's SphereX. I will discuss line-intensity mapping and show how it can be used to probe dark matter, neutrino decays, and other exotic physics. .

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The talk

  1. The cosmic optical background excess, line-intensity mapping 2022-12-07 · 1 h 14 min · CERN's player

Credits and licence

Institution
CERN
Department
Theory Colloquia
Speaker
Marc Kamionkowski
Year
2022
Language
English
Source
CERN
Licence
CERN, as CERN states it. CERN's terms
Attribution
© CERN. CERN provides its audiovisual media free of charge for educational and informational use, credited to CERN; this lecture is shown in CERN's own player.
Who can watch
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