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pro vyhledávání: '"Hatton, Marcus J."'
Nonlinear simulations of neutron star mergers are complicated by the need to represent turbulent dynamics. As we cannot (yet) perform simulations that resolve accurately both the gravitational-wave scale and the smallest scales at which magneto/hydro
Externí odkaz:
http://arxiv.org/abs/2407.18012
Autor:
Hatton, Marcus J., Hawke, Ian
We present a formulation of special relativistic, dissipative hydrodynamics (SRDHD) derived from the well-established M\"uller- Israel-Stewart (MIS) formalism using an expansion in deviations from ideal behaviour. By re-summing the non-ideal terms, o
Externí odkaz:
http://arxiv.org/abs/2405.09495