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pro vyhledávání: '"Comer, Greg L."'
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
Fully non-linear equations of motion for dissipative general relativistic multi-fluids can be obtained from an action principle involving the explicit use of lower dimensional matter spaces. More traditional strategies for incorporating dissipation-l
Externí odkaz:
http://arxiv.org/abs/2008.00945