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Award Abstract # 2031744
Supermassive Black Holes Approaching Merger: Accretion Dynamics, Jets and Electromagnetic Signals

NSF Org: OAC
Office of Advanced Cyberinfrastructure (OAC)
Recipient: ROCHESTER INSTITUTE OF TECHNOLOGY
Initial Amendment Date: May 7, 2020
Latest Amendment Date: May 7, 2020
Award Number: 2031744
Award Instrument: Standard Grant
Program Manager: Edward Walker
edwalker@nsf.gov
 (703)292-4863
OAC
 Office of Advanced Cyberinfrastructure (OAC)
CSE
 Directorate for Computer and Information Science and Engineering
Start Date: September 1, 2020
End Date: August 31, 2023 (Estimated)
Total Intended Award Amount: $9,994.00
Total Awarded Amount to Date: $9,994.00
Funds Obligated to Date: FY 2020 = $9,994.00
History of Investigator:
  • Manuela Campanelli (Principal Investigator)
    mxcsma@rit.edu
  • 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 Technology
1 Lomb Memorial Drive
Rochester
NY  US  14623-5603
Primary Place of Performance
Congressional District:
25
Unique Entity Identifier (UEI): J6TWTRKC1X14
Parent UEI:
NSF Program(s): Leadership-Class Computing
Primary Program Source: 01002021DB NSF RESEARCH & RELATED ACTIVIT
Program Reference Code(s):
Program Element Code(s): 778100
Award Agency Code: 4900
Fund Agency Code: 4900
Assistance Listing Number(s): 47.070

ABSTRACT

For nearly four decades, the National Science Foundation (NSF) has played a leadership role in provisioning advanced cyberinfrastructure capabilities for the Nation's Science and Engineering (S&E) researchers. An important component in this investment is the leadership-class computing program that provides computational and data analytics capabilities at the largest scale to inspire transformative S&E discoveries that would not be possible otherwise. NSF's current leadership-class computing investment supports Frontera, the largest High-Performance Computing (HPC) system on a US academic campus. The Frontera system is deployed and operated by the Texas Advanced Computing Center (TACC) at the University of Texas (UT) at Austin. This travel grant will support the participation of researchers who have been awarded a computer time allocation on the Frontera system at a future Principal Investigator (PI) meeting organized by TACC. The award will also support travel for technical coordination between researchers and the Frontera project to ensure optimal and effective utilization of the Frontera system.

The goal of the PI meeting is to allow Frontera research users, as well as their students, to share scientific results, exchange practical lessons-learned, and present their overall experience from using the Frontera system. In addition to research presentations, the meeting will have ample time, as well as facilitated sessions, to promote increased interaction between Frontera research users and project staff. The outcome of the PI meeting will not only enable the Frontera project to better understand and serve the scientific research community, but also build a community to better represent the unique needs of S&E research that require access to NSF leadership computing facilities. To facilitate deeper coordination beyond the PI meeting, this award will also provide travel support to enable technical coordination between the research user teams and the Frontera project.

This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH

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(Showing: 1 - 10 of 16)
Abbott, R. and Abbott, T. D. and Abraham, S. and Acernese, F. and Ackley, K. and Adams, A. and Adams, C. and Adhikari, R. X. and Adya, V. B. and Affeldt, C. and Agarwal, D. and Agathos, M. and Agatsuma, K. and Aggarwal, N. and Aguiar, O. D. and Aiello, L. "Observation of Gravitational Waves from Two Neutron StarBlack Hole Coalescences" The Astrophysical Journal Letters , v.915 , 2021 https://doi.org/10.3847/2041-8213/ac082e Citation Details
Abbott, R. and Abbott, T. D. and Abraham, S. and Acernese, F. and Ackley, K. and Adams, A. and Adams, C. and Adhikari, R. X. and Adya, V. B. and Affeldt, C. and Agathos, M. and Agatsuma, K. and Aggarwal, N. and Aguiar, O. D. and Aiello, L. and Ain, A. and "GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo during the First Half of the Third Observing Run" Physical Review X , v.11 , 2021 https://doi.org/10.1103/PhysRevX.11.021053 Citation Details
Abbott, R. and Abbott, T. D. and Abraham, S. and Acernese, F. and Ackley, K. and Adams, C. and Adhikari, R. X. and Adya, V. B. and Affeldt, C. and Agathos, M. and Agatsuma, K. and Aggarwal, N. and Aguiar, O. D. and Aich, A. and Aiello, L. and Ain, A. and "Properties and Astrophysical Implications of the 150 M Binary Black Hole Merger GW190521" The Astrophysical Journal , v.900 , 2020 https://doi.org/10.3847/2041-8213/aba493 Citation Details
Cipolletta, F and Kalinani, J V and Giacomazzo, B and Ciolfi, R "Spritz: a new fully general-relativistic magnetohydrodynamic code" Classical and Quantum Gravity , v.37 , 2020 https://doi.org/10.1088/1361-6382/ab8be8 Citation Details
Combi, Luciano and Armengol, Federico G. and Campanelli, Manuela and Ireland, Brennan and Noble, Scott C. and Nakano, Hiroyuki and Bowen, Dennis "Superposed metric for spinning black hole binaries approaching merger" Physical Review D , v.104 , 2021 https://doi.org/10.1103/PhysRevD.104.044041 Citation Details
Combi, Luciano and Lopez Armengol, Federico G. and Campanelli, Manuela and Noble, Scott C. and Avara, Mark and Krolik, Julian H. and Bowen, Dennis "Minidisk Accretion onto Spinning Black Hole Binaries: Quasi-periodicities and Outflows" The Astrophysical Journal , v.928 , 2022 https://doi.org/10.3847/1538-4357/ac532a Citation Details
Combi, Luciano and Yang, Huan and Gutierrez, Eduardo and Noble, Scott_C and Romero, Gustavo_E and Campanelli, Manuela "General relativistic magnetohydrodynamical simulations of accretion flows through traversable wormholes" Physical Review D , v.109 , 2024 https://doi.org/10.1103/PhysRevD.109.103034 Citation Details
Gayathri, V. and Healy, J. and Lange, J. and OBrien, B. and Szczepanczyk, M. and Bartos, I. and Campanelli, M. and Klimenko, S. and Lousto, C. O. and OShaughnessy, R. "Measuring the Hubble Constant with GW190521 as an Eccentric black hole Merger and Its Potential Electromagnetic Counterpart" The Astrophysical Journal , v.908 , 2021 https://doi.org/10.3847/2041-8213/abe388 Citation Details
Gayathri, V. and Healy, J. and Lange, J. and OBrien, B. and Szczepaczyk, M. and Bartos, Imre and Campanelli, M. and Klimenko, S. and Lousto, C. O. and OShaughnessy, R. "Eccentricity estimate for black hole mergers with numerical relativity simulations" Nature Astronomy , v.6 , 2022 https://doi.org/10.1038/s41550-021-01568-w Citation Details
Gutiérrez, Eduardo M. and Combi, Luciano and Noble, Scott C. and Campanelli, Manuela and Krolik, Julian H. and López Armengol, Federico and García, Federico "Electromagnetic Signatures from Supermassive Binary Black Holes Approaching Merger" The Astrophysical Journal , v.928 , 2022 https://doi.org/10.3847/1538-4357/ac56de Citation Details
Ji, Liwei and Mewes, Vassilios and Zlochower, Yosef and Ennoggi, Lorenzo and Armengol, Federico G. and Campanelli, Manuela and Cipolletta, Federico and Etienne, Zachariah B. "Ameliorating the Courant-Friedrichs-Lewy condition in spherical coordinates: A double FFT filter method for general relativistic MHD in dynamical spacetimes" Physical Review D , v.108 , 2023 https://doi.org/10.1103/PhysRevD.108.104005 Citation Details
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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.

The researchers at the Rochester Institute of Technology are conducting pioneering research in the field of merging black holes. Their work aims to enhance our understanding of these cosmic objects and their light emission. By utilizing advanced simulations, they are investigating complex processes such as gas accretion, magnetic field generation, and dynamical spacetime, which are fundamental to the study of merging black holes.

This cutting-edge research is made possible through access to the immensely powerful petascale supercomputer, Frontera, located at the Texas Advanced Computing Center. This computational resource enables the team to carry out simulations on an unprecedented scale, incorporating vast amounts of data and conducting intricate calculations. By accurately replicating the intricate dynamics of merging black holes, the researchers can provide precise predictions of the emitted light,

In addition to analyzing the gas distribution and light emission of merging black holes, the researchers are focused on distinguishing these phenomena from other sources of light in the universe. This differentiation is crucial to the development of unique observation methods that can identify the distinct signature patterns of merging black holes. Ultimately, these findings have the potential to unlock the mysteries of the universe and bring us closer to comprehending the enigmatic nature of black holes. 

Furthermore, thanks to this travel award, the researchers have been able to present their simulations and research findings on the Frontera supercomputer at various national and international conferences, further disseminating their groundbreaking work.

 


Last Modified: 12/27/2023
Modified by: Manuela Campanelli

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