Newswise — Within the last two decades astronomers have discovered that black holes are ubiquitous in the Universe, that while stellar mass black holes populate galaxies by the millions, each galaxy also hosts a central supermassive black hole that is 10 million to 10 billion times the mass of the Sun. And when matter falls into these black holes they light up, some of them shining so brightly that they can be seen across the Universe. Researchers are trying to understand how the enormous amounts of energy that are emitted from the centers of these active galaxies can shape both their host galaxy as well as the intergalactic medium, an exploration that takes us back to shortly after the big bang when the Universe was only 5% of its current age.

Publications1.Matthew I. Kim, Damian J. Christian, David Garofalo, Jaclyn D'Avanzo, Possible evolution of supermassive black holes from FRI quasars, Monthly Notices of the Royal Astronomical Society, 2016

2. David Garofalo & Chandra B. Singh, Scale-invariant jet suppression across the black hole mass scale, Astrophysics & Space Science, 2016

3. David Garofalo, Matthew I. Kim, Damian J. Christian, Emily Hollingworth, Aaron Lowery, Matthew Harmon, Reconciling AGN-star formation, the Soltan argument, and Meier's paradox, the Astrophysical Journal, 2016

4. David Garofalo, Symmetry and the arrow of time in theoretical black hole astrophysics, Journal of Gravity, 2015

5. David Garofalo, Matthew I. Kim, & Damian J. Christian, Constraints on the radio loud/radio quiet dichotomy from the fundamental plane, Monthly Notices of the Royal Astronomical Society, 2014

6. David Garofalo, The jet-disc connection: evidence for a reinterpretation in radio loud and radio quiet active galactic nuclei, Monthly Notices of the Royal Astronomical Society, 2013

7. David Garofalo, Retrograde versus Prograde Models of Accreting Black Holes, Advances in Astronomy, 2013

8. Masanori Nakamura, David L. Meier & David Garofalo, Magnetohydrodynamic properties of extragalactic jets, Astrophysics & Space Science, 2011

9. Masanori Nakamura, David Garofalo & David L. Meier, A magnetohydrodynamic model of the M87 jet. I. Superluminal Knot Ejections from HST-1 as Trails of Quad Relativistic MHD Shocks, the Astrophysical Journal, 2010

10. David Garofalo & David L. Meier, Misconceptions about general relativity in theoretical black hole astrophysics, Monthly Notices of the Royal Astronomical Society, 2010

11. David Garofalo, Daniel A. Evans & Rita M. Sambruna, The evolution of radio loud active galactic nuclei as a function of black hole spin, Monthly Notices of the Royal Astronomical Society, 2010

12. David Garofalo, Signatures of black hole spin in galaxy evolution, the Astrophysical Journal Letters, 2009

13. David Garofalo, The spin dependence of the Blandford-Znajek effect, the Astrophysical Journal, 2009

14. David Garofalo, Spacetime constraints on accreting black holes, Physical Review D, 2009

15. David Garofalo, Magnetic fields around black holes, PhDT, 2008

16. Chris Reynolds, David Garofalo & Mitch Begelman, Trapping of magnetic flux by the plunge region of a black hole accretion disk, the Astrophysical Journal, 2006

17. Chris Reynolds, Laura W. Brenneman & David Garofalo, Black hole spin in AGN and GBHCs, Astrophysics & Space Science, 2005

18. David Garofalo & Chris Reynolds, Sporadically torqued accretion disks around black holes, the Astrophysical Journal, 2005