Numerical modeling of laser-driven experiments aiming to demonstrate magnetic field amplification via turbulent dynamo

The universe is permeated by magnetic fields, with strengths ranging from a femtogauss in the voids between the filaments of galaxy clusters to several teragauss in black holes and neutron stars. The standard model behind cosmological magnetic fields is the nonlinear amplification of seed fields via...

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Үндсэн зохиолчид:	Tzeferacos, P, Rigby, A, Bott, A, Bell, A, Bingham, R, Casner, A, Cattaneo, F, Churazov, E, Emig, J, Flocke, N, Fiuza, F, Forest, C, Foster, J, Graziani, C, Katz, J, Koenig, M, Li, C, Meinecke, J, Petrasso, R, Park, H, Remington, B, Ross, J, Ryu, D, Ryutov, D, Weide, K, White, T, Reville, B, Miniati, F, Schekochihin, A, Froula, D, Gregori, G, Lamb, D
Формат:	Journal article
Хэвлэсэн:	AIP Publishing 2017

Numerical modeling of laser-driven experiments aiming to demonstrate magnetic field amplification via turbulent dynamo

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