31 August 2026 to 4 September 2026
Jesi
Europe/Rome timezone

Redshift-dependent cosmic birefringence from pseudoscalar fields

Not scheduled
20m
Sala Congressi della Fondazione Cassa di Risparmio di Jesi (Jesi)

Sala Congressi della Fondazione Cassa di Risparmio di Jesi

Jesi

Piazza Angelo Colocci, 4, 60035 Jesi (AN)
Talk

Speaker

Matteo Galaverni (Vatican Observatory - INAF/OAS - INFN Bologna)

Description

Recent analyses of Cosmic Microwave Background (CMB) polarization data from satellite missions (both WMAP and Planck) as well as from the Atacama Cosmology Telescope, suggest a possible hint of cosmic birefringence (rotation of the linear polarization plane). We discuss the imprints of a redshift/time dependent cosmological pseudoscalar field on the CMB polarization power spectra. We consider several theoretically motivated redshift dependencies of the pseudoscalar field and assess their impact on the power spectra.

Author

Matteo Galaverni (Vatican Observatory - INAF/OAS - INFN Bologna)

Presentation materials

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