4.4 Article

The RIT binary black hole simulations catalog

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

Funding

  1. NSF [PHY-1607520, PHY-1707946, ACI-1550436, OCI-1515969, AST-1516150, ACI-1516125, AST-1028087, PHY-0722703, DMS-0820923, PHY-1229173]
  2. Blue Waters sustained-petascale computing NSF [OCI-1515969, OCI-0725070, ACI-1238993]
  3. Direct For Computer & Info Scie & Enginr
  4. Office of Advanced Cyberinfrastructure (OAC) [1516125] Funding Source: National Science Foundation
  5. Direct For Mathematical & Physical Scien
  6. Division Of Physics [1607520] Funding Source: National Science Foundation
  7. Office of Advanced Cyberinfrastructure (OAC)
  8. 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.

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