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franco_vazza
franco_vazza
@franco_vazza@mastodon.social  ·  activity timestamp yesterday

A few highlights from lecture yesterday at Nordita, about numerical techniques to evolve magnetic fields in cosmological simulations and (try to) simulate small-scale dynamo amplification.

Message 1. there is no best method for all needs: it depends
Message 2: they all are anyway wrong as they probe a different regime of plasma than is in nature - the best we can do is to hope we can extrapolate results to the right regime.

(with quote by @jaztrophysicist ) #astronomy #astrophysics #science

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quote from Rincon+19: " due to computing power limitations implying finite numerical resolutions, most virtual MHD fluids of computer simulations have 0.1<Pm<10. Hence, it is and will remain impossible in a foreseeable future to simulate magnetic-field amplification in any kind of regime found in nature. The best we can hope for is that simulations of largish or smallish Pm regimes can provide glimpses of the asymptotic dynamics"
quote from Rincon+19: " due to computing power limitations implying finite numerical resolutions, most virtual MHD fluids of computer simulations have 0.1<Pm<10. Hence, it is and will remain impossible in a foreseeable future to simulate magnetic-field amplification in any kind of regime found in nature. The best we can hope for is that simulations of largish or smallish Pm regimes can provide glimpses of the asymptotic dynamics"
quote from Rincon+19: " due to computing power limitations implying finite numerical resolutions, most virtual MHD fluids of computer simulations have 0.1<Pm<10. Hence, it is and will remain impossible in a foreseeable future to simulate magnetic-field amplification in any kind of regime found in nature. The best we can hope for is that simulations of largish or smallish Pm regimes can provide glimpses of the asymptotic dynamics"
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