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pro vyhledávání: '"Sandhya Jagannathan"'
Astrophysical magnetic fields decay primarily via two processes namely, ambipolar diffusion and turbulence. Constraints on the strength and the spectral index of non-helical magnetic fields have been derived earlier in the literature through the effe
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https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d915537622f017fd78a687efa1859d25
Magnetic fields have been observed in galaxy clusters with strengths of the order of $\sim \mu$G. The non-thermal pressure exerted by magnetic fields also contributes to the total pressure in galaxy clusters and can in turn affect the estimates of th
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https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1b3116a9a8a7116964b1799060b7fa31
http://arxiv.org/abs/1909.07847
http://arxiv.org/abs/1909.07847
Models of inflationary magnetogenesis with a coupling to the electromagnetic action of the form $f^2 F_{\mu\nu}F^{\mu\nu}$, are known to suffer from several problems. These include the strong coupling problem, the back reaction problem and also stron
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https://explore.openaire.eu/search/publication?articleId=doi_dedup___::608bb09e8ecc6d5b3a964b3b76a7c881