T3.2 Primordial magnetic field and the CMB
T3.2.1 CMB constraints on inflationary magnetic fields (PD-B1):
what are the constraints on magnetic fields generated during inflation based on CMB data?
T3.2.2 Magnetic field effect on recombination and Hubble tension (w/ PhD-B2 and PD-B4):
how much is the evolution of the Universe during Dark Ages affected by primordial magnetic fields?
Papers acknowledging COSMOMAG
5.
Iarygina, O., & Brandenburg, A.: 2026, “Primordial turbulence from inflation: a new inflaton-driven turbulent regime,” Phys. Rev. Lett., to be submitted
(arXiv:2609.10326, ADS, HTML)
| 4.
Brandenburg, A., Ntormousi, E., & Schober, J.: 2026, “No evidence of vorticity production from irrotational turbulent gravitational collapse yet,” Astrophys. J., in press
(arXiv:2607.01207, ADS, HTML)
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| 3.
Brandenburg, A., Cielo, M., Iarygina, O., Vazza, F.: 2026, “Isochrones in primordial magnetic field evolution,” Astron. Astrophys., submitted
(arXiv:2606.10863, ADS)
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| 2. | Kumar, V., & Brandenburg, A.: 2026, “Magnetic Prandtl number dependence of plasmoid-mediated reconnection,” J. Plasma Phys., submitted
(arXiv:2605.18946, ADS)
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| 1.
Brandenburg, A., Ghosh, O., Vazza, F., & Neronov, A.: 2026, “Magnetic field spreading from stellar and galactic dynamos into the exterior,” Astrophys. J. 1002, 165
(arXiv:2512.17770, ADS, DOI, HTML, PDF)
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$Date: 2026/09/15 08:13:21 $, $Author: brandenb $, $Revision: 1.12 $