linkedin post 2022-03-06 05:51:39

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“MAGNETIC FIELDS in AGN are observed from pc scales to Mpc scales, e.g. from the non-thermal filaments in the Galactic centre, VLBI polarimetry of radio galaxy cores, to polarization of jets, and radio lobes. They affect the accretion disk, jet collimation and particle acceleration, and contribute significantly to the pressure inside radio lobes.” (AGN = Active Galactic Nuclei). https://lnkd.in/gTA_aVgT View in LinkedIn
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linkedin post 2022-03-07 05:00:51

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GIANT GRADIENTS. “That precise conservation gives rise to the existence of steady-state linear gradients on the large scale, and the expectation value of the kinetic energy (per particle) connects to temperature through the Boltzmann constant, e.g. with ⟨Ek ⟩ = 32 kB T in the kinetic theory of gases.” https://link.springer.com/content/pdf/10.1007/JHEP07(2019)140.pdf View in LinkedIn
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