Award Abstract # 1550436
SI2-SSI: Collaborative Research: Einstein Toolkit Community Integration and Data Exploration

NSF Org: OAC
Office of Advanced Cyberinfrastructure (OAC)
Recipient: ROCHESTER INSTITUTE OF TECHNOLOGY
Initial Amendment Date: July 11, 2016
Latest Amendment Date: July 8, 2019
Award Number: 1550436
Award Instrument: Continuing Grant
Program Manager: Amy Walton
awalton@nsf.gov
 (703)292-4538
OAC
 Office of Advanced Cyberinfrastructure (OAC)
CSE
 Directorate for Computer and Information Science and Engineering
Start Date: July 1, 2016
End Date: June 30, 2021 (Estimated)
Total Intended Award Amount: $437,521.00
Total Awarded Amount to Date: $437,521.00
Funds Obligated to Date: FY 2016 = $218,761.00
FY 2017 = $72,920.00

FY 2018 = $72,920.00

FY 2019 = $72,920.00
History of Investigator:
  • Manuela Campanelli (Principal Investigator)
    mxcsma@rit.edu
  • Joshua Faber (Co-Principal Investigator)
  • Yosef Zlochower (Co-Principal Investigator)
Recipient Sponsored Research Office: Rochester Institute of Tech
1 LOMB MEMORIAL DR
ROCHESTER
NY  US  14623-5603
(585)475-7987
Sponsor Congressional District: 25
Primary Place of Performance: Rochester Institute of Tech
NY  US  14623-5603
Primary Place of Performance
Congressional District:
25
Unique Entity Identifier (UEI): J6TWTRKC1X14
Parent UEI:
NSF Program(s): COMPUTATIONAL PHYSICS,
Software Institutes
Primary Program Source: 01001617DB NSF RESEARCH & RELATED ACTIVIT
01001718DB NSF RESEARCH & RELATED ACTIVIT

01001819DB NSF RESEARCH & RELATED ACTIVIT

01001920DB NSF RESEARCH & RELATED ACTIVIT
Program Reference Code(s): 7433, 7569, 8009, 8084
Program Element Code(s): 724400, 800400
Award Agency Code: 4900
Fund Agency Code: 4900
Assistance Listing Number(s): 47.070

ABSTRACT

A new astronomy has arrived with the recent detection of gravitational waves. Modeling of sources of gravitational radiation is more than ever a critical necessity in order to interpret the observations. The project Einstein Toolkit has as overarching mission to provide the scientific community with a sustainable software platform of core computational tools for research focused on astrophysical systems endowed with complex multi-scale/multi-physics properties which are governed by Einstein's equations of General Relativity. The central premise of the project Einstein Toolkit is to create a broad and vibrant community of users, a community where interdisciplinary collaborations are the norm and not the exception, a community driving advances in the next generation of high-performance computing cyberinfrastructure. The main objectives of the project Einstein Toolkit are: developing software tools for a radical increase in scientific productivity, achieving sustainability of the software ecosystem, addressing software engineering challenges, and the curation of data from general relativistic numerical simulations.

This project will achieve its goals through two major activity areas. Regarding the software ecosystem and its sustainability, the scheduler that handles the flow of tasks in a problem will be redesigned to be more versatile and to improve its performance. In addition new software modules will be developed to broaden the choices of initial data and matter sources, as well as modules for problems requiring a high degree of experimentation with equations and numerical methodologies. A new general relativistic magneto-hydrodynamics code will also be integrated in the Einstein Toolkit. The second activity area involves building a simulation data repository. The repository will allows user to compare results, contribute data, test innovative ideas and algorithms for gravitational wave data analysis, and to explore or discover new phenomena in sources of gravitational radiation. The broader impact effort in the project Einstein Toolkit will be organized in two major activity areas. The first involves community integration. The project will support a program of ease-of-use on-line tutorials and a workshops/tutorial series. The program will help small groups or individual investigators familiarizing with the codes and modules in the toolkit as well as pathways to become a developer. Regarding outreach and education, the project Einstein Toolkit will enable interdisciplinary training of students and postdocs in numerical relativity, computational astrophysics and computer science. The effort will includes developing a teaching resources bank for educational activities involving computational topics applied to gravitational physics and astrophysics. The educational resources will be suitable for computational courses in general relativity and astrophysics at both the graduate and undergraduate level.

This project is supported by the Division of Advanced Cyberinfrastructure in the Directorate for Computer & Information Science & Engineering and the Physics Division in the Directorate of Mathematical and Physical Sciences.

PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH

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(Showing: 1 - 10 of 44)
Abbott, Benjamin P and others "{Model comparison from LIGO\textendash{}Virgo data on GW170817\textquoteright{}s binary components and consequences for the merger remnant}" Class. Quant. Grav. , v.37 , 2020 , p.045006 10.1088/1361-6382/ab5f7c
Abbott, B. P. and others "Directly comparing GW150914 with numerical solutions of Einstein?s equations for binary black hole coalescence" Phys. Rev. , v.D94 , 2016 , p.064035 10.1103/PhysRevD.94.064035
Abbott, B. P. and others "GW170817: Measurements of neutron star radii and equation of state" Phys. Rev. Lett. , v.121 , 2018 , p.161101 10.1103/PhysRevLett.121.161101
Abbott, B. P. and others "Properties of the binary neutron star merger GW170817" Phys. Rev. , v.X9 , 2019 , p.011001 10.1103/PhysRevX.9.011001
Abbott, B.P. and others "{GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs}" Phys. Rev. X , v.9 , 2019 , p.031040 10.1103/PhysRevX.9.031040
Abbott, R. and others "{GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run}" Phys. Rev. X , v.11 , 2021 , p.021053 10.1103/PhysRevX.11.021053
Abbott, R. and others "{Properties and Astrophysical Implications of the 150 M$_\odot$ Binary Black Hole Merger GW190521}" Astrophys. J. Lett. , v.900 , 2020 , p.L13 10.3847/2041-8213/aba493
Abbott, R. and others "{Properties and Astrophysical Implications of the 150 M$_\odot$ Binary Black Hole Merger GW190521}" Astrophys. J. Lett. , v.900 , 2020 , p.L13 10.3847/2041-8213/aba493
Armengol, Federico G. Lopez and Combi, Luciano and Campanelli, Manuela and Noble, Scott C. and Krolik, Julian H. and Bowen, Dennis B. and Avara, Mark J. and Mewes, Vassilios and Nakano, Hiroyuki "{Circumbinary Disk Accretion into Spinning Black Hole Binaries}" Astrophys. J. , v.913 , 2021 , p.16 10.3847/1538-4357/abf0af
Barlow, Nathaniel S. and Weinstein, Steven J. and Faber, Joshua A. "An asymptotically consistent approximant for the equatorial bending angle of light due to Kerr black holes" Class. Quant. Grav. , v.34 , 2017 , p.135017 10.1088/1361-6382/aa7538
Beachley, Ryne J. and Mistysyn, Morgan and Faber, Joshua A. and Weinstein, Steven J. and Barlow, Nathaniel S. "Accurate closed-form trajectories of light around a Kerr black hole using asymptotic approximants" Class. Quant. Grav. , v.35 , 2018 , p.205009 10.1088/1361-6382/aae0cd, 10.1088/1361-6382/aae7f7
(Showing: 1 - 10 of 44)

PROJECT OUTCOMES REPORT

Disclaimer

This Project Outcomes Report for the General Public is displayed verbatim as submitted by the Principal Investigator (PI) for this award. Any opinions, findings, and conclusions or recommendations expressed in this Report are those of the PI and do not necessarily reflect the views of the National Science Foundation; NSF has not approved or endorsed its content.

This grant is part of a large collaborative effort supported by the NSF to develop of the Einstein Toolkit (einsteintoolkit.org). At RIT, the grant supported the development of a new GRMHD code, SphericalNR, which implements the Einstein-Magnetohydrodynamics equations in curvilinear coordinates. In addition, a new catalog of binary neutron star data was created and distributed with support from this grant. The catalog can be accessed through the collaborative porta: https://compact-binaries.org

SphericalNR includes a novel filtering technique to ameliorate the often severe Courant time limitation associated with numerical evolutions in spherical coordinates. It also includes a higher-order vector potential formalism for the the evolution of the magnetic field. The attached figure shows a snapshot of the evolution of a bar-mode unstable neutron star, as well as the waveform from a distorted black hole.

A postdoctoral researcher and a graduate student were supported via this grant at RIT. In addition, this grant supported undergraduate student researchers in an REU program on multimessenger astrophysics at RIT, and a new course on high-performance computing at RIT was developed that made extensive use of the tookit.

Each year, the Einstein Toolkit consortium holds a workshop and school for new users. At RIT, this workshop and school was held in Summer 2019. The workshop was held in person at RIT and broadcast over bluejeans to an international audience.

 

 


Last Modified: 08/01/2021
Modified by: Manuela Campanelli

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