Journal
CLASSICAL AND QUANTUM GRAVITY
Volume 34, Issue 22, Pages -Publisher
IOP Publishing Ltd
DOI: 10.1088/1361-6382/aa91b1
Keywords
binary black holes; numerical general relativity; simulations
Categories
Funding
- NSF [PHY-1607520, PHY-1707946, ACI-1550436, OCI-1515969, AST-1516150, ACI-1516125, AST-1028087, PHY-0722703, DMS-0820923, PHY-1229173]
- Blue Waters sustained-petascale computing NSF [OCI-1515969, OCI-0725070, ACI-1238993]
- Direct For Computer & Info Scie & Enginr
- Office of Advanced Cyberinfrastructure (OAC) [1516125] Funding Source: National Science Foundation
- Direct For Mathematical & Physical Scien
- Division Of Physics [1607520] Funding Source: National Science Foundation
- Office of Advanced Cyberinfrastructure (OAC)
- Direct For Computer & Info Scie & Enginr [1550436] Funding Source: National Science Foundation
Ask authors/readers for more resources
The RIT numerical relativity group is releasing a public catalog of black-hole-binary waveforms. The initial release of the catalog consists of 126 recent simulations that include precessing and nonprecessing systems with mass ratios q = m(1)/m(2) in the range 1/6 <= q <= 1. The catalog contains information about the initial data of the simulation, the waveforms extrapolated to infinity, as well as information about the peak luminosity and final remnant black hole properties. These waveforms can be used to independently interpret gravitational wave signals from laser interferometric detectors and the remnant properties to model the merger of black-hole binaries from initial configurations.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available