CORDIS Project
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This research addresses the complex mathematical equations governing the motion of fluid bodies in a gravitational context. The goal is to develop new computational methods for simulating neutron star interactions and gravitational waves.
The motion of strongly gravitating fluid bodies is described by the Euler-Einstein system of partial differential equations, combining fluid dynamics with general relativity.
Centuries after their advent, the solution to these equations remains mathematically and computationally difficult, and the break-down of well-posedness on the boundary interface between fluid and vacuum remains a challenging open problem.
The problem manifests itself in numerical simulations of binary neutron-star inspiral…
Partner organizations (coordinator is shown above), with normalized type and CORDIS activity type. Guests see up to 4 partners.
United States, Urbana
Type: University / higher education
Activity type: Higher or Secondary Education Establishments
SME: No
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