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CTTK: a new method to solve the initial data constraints in numerical relativity

Abstract:
This review is an up-to-date account of the use of numerical relativity to study dynamical, strong-gravity environments in a cosmological context. First, we provide a gentle introduction into the use of numerical relativity in solving cosmological spacetimes, aimed at both cosmologists and numerical relativists. Second, we survey the present body of work, focusing on general relativistic simulations, organised according to the cosmological history—from cosmogenesis, through the early hot Big Bang, to the late-time evolution of the universe. We discuss the present state-of-the-art, and suggest directions in which future work can be fruitfully pursued
Publication status:
Published
Peer review status:
Peer reviewed

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Files:
Publisher copy:
10.1088/1361-6382/acb883

Authors

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Institution:
University of Oxford
Role:
Author
ORCID:
0000-0001-9584-5791
More by this author
Institution:
University of Oxford
Role:
Author
ORCID:
0000-0001-8841-1522
More by this author
Role:
Author
ORCID:
0000-0002-6227-9540


More from this funder
Funder identifier:
10.13039/100010663
Grant:
693024
More from this funder
Funder identifier:
10.13039/501100000271
Grant:
ST/V003240/1


Publisher:
IOP Publishing
Journal:
Classical and Quantum Gravity More from this journal
Volume:
40
Issue:
7
Pages:
075003-075003
Publication date:
2023-02-02
DOI:
EISSN:
1361-6382
ISSN:
0264-9381


Language:
English
Keywords:
Pubs id:
1334303
Local pid:
pubs:1334303
Source identifiers:
W4318948406
Deposit date:
2026-05-05
ARK identifier:
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