Abstract
We present a search for anisotropic cosmic birefringence in of southern sky observed at 150 GHz with the SPTpol camera on the South Pole Telescope. We reconstruct a map of cosmic polarization rotation anisotropies using higher-order correlations between the observed cosmic microwave background (CMB) and fields. We then measure the angular power spectrum of this map, which is found to be consistent with zero. The nondetection is translated into an upper limit on the amplitude of the scale-invariant cosmic rotation power spectrum, (, 95% C.L.). This upper limit can be used to place constraints on the strength of primordial magnetic fields, (95% C.L.), and on the coupling constant of the Chern-Simons electromagnetic term (95% C.L.), where is the inflationary Hubble scale. For the first time, we also cross-correlate the CMB temperature fluctuations with the reconstructed rotation angle map, a signal expected to be nonvanishing in certain theoretical scenarios, and find no detectable signal. We perform a suite of systematics and consistency checks and find no evidence for contamination.
- Received 16 June 2020
- Accepted 17 August 2020
DOI:https://doi.org/10.1103/PhysRevD.102.083504
© 2020 American Physical Society