Faculty Type: 
Active Faculty
Title: 
Professor
Address: 

Physics and Astrophysics Bldg., Rm. 233
Stanford University
Stanford, CA 94305

Phone Number: 
650-725-7595
Contact Email: 

What are the physical conditions around compact objects? How do they accelerate particles to the highest energies seen?

Professor Romani is interested in the physics of the most extreme objects in the observable universe—neutron stars and black holes—where density, gravitational field and, often, magnetic field reach their maximum measured values. His group makes observations of such objects, using premiere telescopes on the ground and in space, and constructs theoretical models to interpret the remarkable behaviors seen. One particular interest is studying how black holes and neutron stars accelerate particles to energies much higher than those yet produced on Earth and how they generate relativistic outflows in the form of winds and jets.

Current areas of focus:
- Populations of gamma-ray sources
- The origin and evolution of radio pulsars
- Supernovae and their products
- Instrumentation for fast optical variability
- Pulsar timing and gravity wave searches

Career History

  • A.B., 1983, Princeton University
  • Ph.D., 1987, California Institute of Technology
  • TAC Postdoctoral Fellow, University of California at Berkeley, 1987-89
  • Member, Institute of Advanced Study, 1989-91
  • Assistant Professor of Physics, Stanford University, 1991-98
  • Sloan Foundation Fellow 1992-1994
  • Cottrell Scholar 1994-99
  • Gauss Professur -- Universitaet Goettingen, 1997
  • Rossi Prize, AAS 2013
  • Associate Professor of Physics, Stanford University, 1998-2006
  • Professor of Physics, Stanford University, 2006-present
  • Member, American Astronomical Society
  • Member, International Astronomical Union.

Post Doc

  • Matthew Kerr

Graduate Students:

Undergraduate Students

  • Sasha Brownsberger
  • Matt Stadnik