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• W3100875857 abstract "We present new limits on the amplitude of potential primordial magnetic fields (PMFs) using temperature and polarization measurements of the cosmic microwave background (CMB) from Planck, BICEP2/Keck Array, POLARBEAR, and SPTpol. We reduce twofold the 95% CL upper limit on the CMB anisotropy power due to a nearly-scale-invariant PMF, with an allowed B-mode power at $ell=1500$ of $D_{ell=1500}^{BB} < 0.071 mu K^2$ for Planck versus $D_{ell=1500}^{BB} < 0.034 mu K^2$ for the combined dataset. We also forecast the expected limits from soon-to-deploy CMB experiments (like SPT-3G, Adv. ACTpol, or the Simons Array) and the proposed CMB-S4 experiment. Future CMB experiments should dramatically reduce the current uncertainties, by one order of magnitude for the near-term experiments and two orders of magnitude for the CMB-S4 experiment. The constraints from CMB-S4 have the potential to rule out much of the parameter space for PMFs." @default.
• W3100875857 created "2020-11-23" @default.
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• W3100875857 date "2017-09-13" @default.
• W3100875857 modified "2023-10-12" @default.
• W3100875857 title "Current and Future Constraints on Primordial Magnetic Fields" @default.
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• W3100875857 doi "https://doi.org/10.3847/1538-4357/aa85e2" @default.
• W3100875857 hasPublicationYear "2017" @default.
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