Computes anisotropic CMB spectral distortion power spectra from photon-dark photon conversions, finding that mass controls multipole shape and mixing sets amplitude, then places Planck limits on the minimal model.
Masi et al.,The cosmic monopole observer (cosmo),arXiv:2110.12254
3 Pith papers cite this work. Polarity classification is still indexing.
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tSZ cross-correlations with large-scale structure tracers prefer low S8 and strong baryonic feedback, yielding S8 = 0.72 and low group baryon fraction in FLAMINGO simulations.
Joint analysis of neutrino detectors and CMB observables can constrain dark matter annihilation into neutrinos for MeV-GeV masses.
citing papers explorer
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Spectral distortion anisotropies from photon to dark photon conversions
Computes anisotropic CMB spectral distortion power spectra from photon-dark photon conversions, finding that mass controls multipole shape and mixing sets amplitude, then places Planck limits on the minimal model.
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FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics
tSZ cross-correlations with large-scale structure tracers prefer low S8 and strong baryonic feedback, yielding S8 = 0.72 and low group baryon fraction in FLAMINGO simulations.
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Joint probes of dark matter annihilation from neutrino detectors and CMB targets
Joint analysis of neutrino detectors and CMB observables can constrain dark matter annihilation into neutrinos for MeV-GeV masses.