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Carlos Lousto
Born	Carlos Lousto Buenos Aires, Argentina
Occupation	Professor of Mathematical Sciences (SMS) and Astrophysical Sciences and Technology (AST), Rochester Institute of Technology (RIT)
Education	Ph.D: Astronomy, University of La Plata. Physics, University of Buenos Aires

Overview

Carlos Lousto (/ˈluːstɔː/; born in Argentina) is a Professor in the School of Mathematical Sciences in Rochester Institute of Technology, known for his work on black hole collisions.

Professional Career

Lousto is a professor in the RIT's School of Mathematical Sciences and co-director of the Center for Computational Relativity and Gravitation. He holds two PhDs, one in Astronomy (studying accretion disks around black holes and the structure of neutron stars) from the University of La Plata, and one in Physics from University of Buenos Aires (on Quantum Field Theory in curved spacetimes).

Carlos Lousto has an extensive research experience which ranges from observational astronomy to black hole perturbation theory and numerical relativity to string theory and quantum gravity. He has authored and co-authored over 150 papers, including several reviews and book chapters. His research is funded by [NSF] and NASA grants and supercomputing allocations in national labs.

Lousto is a key author of the breakthrough on binary black hole simulations and his research discovered that supermassive black holes can be ejected from most galaxies at speeds of up to 5000km/s. He recently perfomed challenging simulations of small mass ratio black hole binaries up to 100:1 and at separations up to 100M and for flip-flopping black holes. Lousto has designed the Funes (UTB), NewHorizon, and BlueSky (RIT) supercomputer clusters to perform binary black hole simulations and used them to support the first detection of gravitational waves from the merger of two black holes.

Distinctions

In 1991 Was honored with an [Alexander von Humboldt foundation] fellowship.

In 2012 Carlos Lousto was distinguished as an American Physical Society Fellow:

• For his important contributions at the interface between perturbation theory and numerical relativity and in understanding how to simulate binary black holes

Selected Bibliography

Highlights per year:

1997 Exact self-consistent solution to semiclassical gravity. Published in Phys. Rev. D 56, 3471

2000 First explicit computation of Self-Force. Published in Phys.Rev.Lett. 84 (2000) 5251-5254

2001 First waveform of BBHs with Lazarus. Published in Phys.Rev.Lett. 87 (2001) 121103

2005 Breakthrough in Numerical Relativity for evolving BBHs. Published in Phys.Rev.Lett. 96 (2006) 111101

2006 The hangup effect in BBHs. Published in Phys.Rev. D74 (2006) 041501

2007 The large recoils in BBHs. Published in Astrophys.J. 659 (2007) L5-L8. Published in Phys. Rev. Lett. 98, 23110

2010 Evolution of 100:1 mass ratio black hole binaries. Published in Phys. Rev. Lett. 106, 041101

2011 The 5000 km/s recoils. Published in Phys.Rev.Lett. 107 (2011) 231102

2015 Flip-Flops. Published in Phys.Rev.Lett. 114 (2015) 141101

2016 Observation of gravitational waves from a binary black hole merger. Published in Phys.Rev.Lett. 116 (2016) 061102

Links

Radio Interview (in spanish)

TV interview (in spanish)