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Evolving relativistic fluid spacetimes using pseudospectral methods and finite differencing

Duez, Matthew D. and Kidder, Lawrence E. and Teukolsky, Saul A. (2007) Evolving relativistic fluid spacetimes using pseudospectral methods and finite differencing. . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20190828-112436025

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Abstract

We present a new code for solving the coupled Einstein-hydrodynamics equations to evolve relativistic, self-gravitating fluids. The Einstein field equations are solved on one grid using pseudospectral methods, while the fluids are evolved on another grid by finite differencing. We discuss implementation details, such as the communication between the grids and the treatment of stellar surfaces, and present code tests.


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
https://arxiv.org/abs/gr-qc/0702126arXivDiscussion Paper
ORCID:
AuthorORCID
Duez, Matthew D.0000-0002-0050-1783
Kidder, Lawrence E.0000-0001-5392-7342
Teukolsky, Saul A.0000-0001-9765-4526
Additional Information:This work was supported in part by a grant from the Sherman Fairchild Foundation, by NSF grants DMS-0553677, PHY-0354631, and NASA grant NNG05GG51G.
Funders:
Funding AgencyGrant Number
Sherman Fairchild FoundationUNSPECIFIED
NSFDMS-0553677
NSFPHY-0354631
NASANNG05GG51G
Record Number:CaltechAUTHORS:20190828-112436025
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190828-112436025
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:98316
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:28 Aug 2019 18:28
Last Modified:09 Mar 2020 13:18

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