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Manuela Campanelli

Rochester Institute of Technology

Stellar Astronomy and Astrophysics


Dennis B. Bowen, Vassilios Mewes, Scott C. Noble, Mark Avara, Manuela Campanelli, and Julian H. Krolik (2019): Quasi-periodicity of Supermassive Binary Black Hole Accretion Approaching Merger, The Astrophysical Journal, The American Astronomical Society, Vol 879, Num 2, pp76


Dennis B. Bowen, Vassilios Mewes, Manuela Campanelli, Scott C. Noble, Julian H. Krolik, and Miguel Zilhão (2018): Quasi-periodic Behavior of Mini-disks in Binary Black Holes Approaching Merger, The Astrophysical Journal Letters, The American Astronomical Society, Vol 853, Num 1, ppL17
James Healy, Jacob Lange, Richard O'Shaughnessy, Carlos Lousto, Manuela Campanelli, Andrew Williamson, Yosef Zlochower, Juan Calderon Bustillo, James Clark, Christopher Evans, D. Ferguson, Sudarshan Ghonge, Karan Jani, Bhavesh Khamesra, Pablo Laguna, Deirdre M. Shoemaker, Alyssa Garcia, Michael Boyle, Daniel Hemberger, Lawrence Kidder, Prayush Kumar, Geoffrey Lovelace, Harald Pfeiffer, Mark Scheel, and Saul Teukolsky (2018): Targeted Numerical Simulations of Binary Black Holes for GW170104, Physical Review D, American Physical Society (APS), Vol 97, Num 6, pp064027
Stéphane d'Ascoli, Scott C. Noble, Dennis B. Bowen, Manuela Campanelli, Julian H. Krolik, and Vassilios Mewes (2018): Electromagnetic Emission from Supermassive Binary Black Holes Approaching Merger, The Astrophysical Jounral, The American Astronomical Society, Vol 865, Num 2, pp140


Bowen, D., M. Campanelli, J. Krolik, V. Mewes, S. Noble (2017): Relativistic Dynamics and Mass Exchange in Binary Black Hole Mini-disks, The Astrophysical Journal, The American Astronomical Society, Vol 838, Num 1, pp42
James Healy and Carlos O Lousto and Yosef Zlochower and Manuela Campanelli (2017): The RIT binary black hole simulations catalog, Classical and Quantum Gravity, IOP Publishing Ltd, Vol 34, Num 22, pp224001
Carlos O. Lousto, Yosef Zlochower, and Manuela Campanelli (2017): Modeling the Black Hole Merger of QSO 3C 186, The Astrophysical Journal Letters, The American Astronomical Society, Vol 841, Num 2, ppL28
Lange, J., O'Shaughnessy, R., Boyle, M., Calderón Bustillo, J., Campanelli, M., Chu, T., Clark, J. A., Demos, N., Fong, H., Healy, J., Hemberger, D. A., Hinder, I., Jani, K., Khamesra, B., Kidder, L. E., Kumar, P., Laguna, P., Lousto, C. O., Lovelace, G., Ossokine, S., Pfeiffer, H., Scheel, M. A., Shoemaker, D. M., Szilagyi, B., Teukolsky, S. and Zlochower, Y. (2017): Parameter Estimation Method That Directly Compares Gravitational Wave Observations to Numerical Relativity, Physical Review D, American Physical Society (APS), Vol 96, Num 10, pp104041


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(2016): Directly Comparing GW150914 with Numerical Solutions of Einstein's Equations for Binary Black Hole Coalescence, Physical Review D, American Physical Society (APS), Vol 94, Num 6, pp064035
Geoffrey Lovelace, Carlos O. Lousto, James Healy, Mark A. Scheel, Alyssa Garcia, Richard O’Shaughnessy, Michael Boyle, Manuela Campanelli, Daniel A. Hemberger, Lawrence E. Kidder, Harald P. Pfeiffer, Béla Szilágyi, Saul A. Teukolsky, and Yosef Zlochower (2016): Modeling the source of GW150914 with targeted numerical-relativity simulations, Classical and Quantum Gravity, IOP Publishing Ltd, Vol 33, Num 24, pp244002
Yosef Zlochower, Hiroyuki Nakano, Bruno C. Mundim, Manuela Campanelli, Scott Noble, and Miguel Zilhão (2016): Inspiraling Black-Hole Binary Spacetimes: Challenges in Transitioning from Analytical to Numerical Techniques, Physical Review D, American Physical Society (APS), Vol 93, Num 12, pp124072


Miguel Zilhão, Scott C. Noble, Manuela Campanelli, Yosef Zlochower (2015): Resolving the Relative Influence of Strong Field Spacetime Dynamics and MHD on Circumbinary Disk Physics, Physical Review D, American Physical Society (APS), Vol 91, Num 2, pp024034
Hotaka Shiokawa, Julian H. Krolik, Roseanne M. Cheng, Tsvi Piran, and Scott C. Noble (2015): General Relativistic Hydrodynamic Simulation of Accretion Flow from a Stellar Tidal Disruption, ApJ, The American Astronomical Society, Vol 804, Num 2, pp85


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New Simulation Sheds Light on Spiraling Supermassive Black Holes

Oct 2, 2018

For the first time, a new computer simulation that fully incorporates the physical effects of Einstein's general theory of relativity shows that gas in such systems will glow predominantly in ultraviolet and X-ray light.


Supermassive black hole model predicts characteristic light signals at cusp of collision

Feb 14, 2018

A new simulation of supermassive black holes--the behemoths at the centers of galaxies--uses a realistic scenario to predict the light signals emitted in the surrounding gas before the masses collide, said Rochester Institute of Technology researchers.


Supercomputing Black Hole Mergers with Blue Waters

May 6, 2015

The observation of supermassive black holes on the verge of merger has numerous exciting consequences for our understanding of galactic evolution, black hole demographics, plasmas in strong-field gravity, and general relativity. Near black holes not only gravity is so extreme to generate observable gravitational waves, but accretion of magnetized, relativistic gas can lead to very powerful observable electromagnetic signals that astronomers are searching for. The collision of supermassive black holes is so powerful tat it is also believed to be responsible of the launching of powerful jets across the universe. The mathematics involved in simulating these events is very sophisticated because one has to solve the equations of Einstein’s general relativity and magneto-hydrodynamics all together. The problem also requires very advanced supercomputers running programs on tens of thousands of CPUs simultaneously, and the use of sophisticated techniques for data extraction and visualization. Petascale numerical simulation is therefore the only tool available to accurately model these systems. Fortunately, thanks to new developments in the field of numerical relativity, we can now simulate and visualize the innermost workings of these violent astrophysical phenomena.


PRAC winners represent a range of disciplines

Apr 21, 2010

Petascale Computing Resource Allocations (PRAC awards) from the National Science Foundation allow research teams to work closely with the Blue Waters project team in preparing their codes. The codes and projects address key challenges faced by our society and explore fundamental scientific and engineering problems. These multiyear collaborations include help porting and re-engineering existing applications. In some cases, the teams will build entirely new applications based on new programming models. Current projects—18 representing about 30 institutions—represent a wide range of scientific disciplines. They will drive scientific discovery for years to come.


Astrophysicists, cosmologists to tap power of Blue Waters

Mar 18, 2010

Blue Waters is expected to be the most powerful supercomputer in the world for open scientific research when it comes online at Illinois in 2011. Scientists and engineers who are eager to tap this sustained-petaflop powerhouse for breakthrough research are already working closely with the Blue Waters project team to prepare their codes. The National Science Foundation provides Petascale Computing Resource Allocations (PRAC awards) to support these collaborations, which include help porting and re-engineering existing applications and in some cases building entirely new applications based on new programming models. Current PRAC projects—18 representing about 30 institutions—represent a wide range of scientific disciplines: biology and health, weather and climate, earthquakes and geophysics, and cosmology and our universe.