activity
19952008
most citedThe RAGE radiation-hydrodynamic code

382 citations · 968 across the 12 of their papers we have counts for

collaborators
Showing gr-qcShow all

5 papers · 1 filter

gr-qc2002★ 133 cited

Gravitational Waves from Gravitational Collapse

Kimberly C. B. New

Gravitational wave emission from the gravitational collapse of massive stars has been studied for more than three decades. Current state of the art numerical investigations of coll…

gr-qc2001

Rotational Instabilities and Centrifugal Hangup

Kimberly C. B. New, Joan M. Centrella

One interesting class of gravitational radiation sources includes rapidly rotating astrophysical objects that encounter dynamical instabilities. We have carried out a set of simula…

gr-qc2000★ 14 cited

Three-dimensional adaptive evolution of gravitational waves in numerical relativity

Kimberly C. B. New, Dae-Il Choi, Joan M. Centrella +3

Adaptive techniques are crucial for successful numerical modeling of gravitational waves from astrophysical sources such as coalescing compact binaries, since the radiation typical…

gr-qc1998★ 30 cited

Stable 3-level leapfrog integration in numerical relativity

Kimberly C. B. New, Keith Watt, Charles W. Misner +1

The 3-level leapfrog time integration algorithm is an attractive choice for numerical relativity simulations since it is time-symmetric and avoids non-physical damping. In Newtonia…

gr-qc1997★ 45 cited

The Relative Stability Against Merger of Close, Compact Binaries

Kimberly C. B. New, Joel E. Tohline

The orbital separation of compact binary stars will shrink with time due to the emission of gravitational radiation. This inspiralling phase of a binary system's evolution generall…