Faculty Type: 
Active Faculty
Title: 
Professor
Address: 

Varian Physics Bldg.
382 Via Pueblo Mall
Stanford, CA 94305-4060

Phone Number: 
650-723-3834
Contact Email: 
Support Staff: 

What are the basic degrees of freedom and interactions underlying gravitational and particle physics?  What is the mechanism behind the initial seeds of structure in the universe, and how can we test it using cosmological observations?  Is there a holographic framework for cosmology that applies throughout the history of the universe, accounting for the effects of horizons and singularities?  What new phenomena arise in quantum field theory in generic conditions such as finite density, temperature, or in time dependent backgrounds?

Professor Silverstein attacks basic problems in several areas of theoretical physics.  She develops concrete and testable mechanisms for cosmic inflation, accounting for its sensitivity to very high energy physics. This has led to a fruitful interface with cosmic microwave background research, contributing to a more systematic analysis of its observable phenomenology.
Professor Silverstein also develops mechanisms for breaking supersymmetry and for stabilizing the extra dimensions of string theory to model the immense hierarchies between the cosmological horizon, electroweak, and Planck scales in nature. In addition, Professor Silverstein uses the ultraviolet completion of gravity afforded by string theory to address questions of quantum gravity, such as singularity resolution and the physics of black hole and cosmological horizons.  Professor Silverstein also uses modern techniques in quantum field theory to model strongly coupled phenomena motivated by measurements in condensed matter physics.

Current areas of focus:
- UV complete mechanisms and systematics of cosmic inflation, including string-theoretic versions of large-field inflation (with gravity wave CMB signatures) and novel mechanisms involving inflaton interactions (with non-Gaussian signatures in the CMB)
- Concrete holographic models of de Sitter expansion in string theory, aimed at upgrading the AdS/CFT correspondence to cosmology
- Mechanisms for non-Fermi liquid transport and $2k_F$ singularities from strongly coupled finite density quantum field theory
- Mechanisms by which the extra degrees of freedom in string theory induce transitions and duality symmetries between spaces of different topology and dimensionality

Career History

  • Education A.B., Physics, Harvard University, 1992.
  • Ph.D., Physics, Princeton University, 1996
  • Postdoctoral Associate, Rutgers University, 1996 - 1997.
  • MacArthur Fellow, 1999
  • 1999 Sloan Fellowship and DOE Outstanding Junior Investigator Award
  • 1999 Member, Institute for Advanced Study
  • 1999 Bergmann Memorial Award
  • Associate Member, Canadian Institute for Advanced Research,
  • Cosmology and Gravity program, 2004-present
  • Assistant Professor, SLAC, Stanford, 1997 - 2001.
  • Associate Professor, SLAC, Stanford, 2001 - 2006.
  • Professor, SLAC, Stanford, 2006-present
  • Kavli Institute for Theoretical Physics and Department of Physics, UC Santa Barbara, 2009-10

Recent Students

  • Yun Song (on to Oxford)
  • Allan Adams (on to Harvard)
  • Michal Fabinger (on to Harvard)
  • Alex Saltman (on to Columbia)
  • David Starr (on to Goldman Sachs)
  • Daniel Green (on to IAS)
  • Xi Dong
  • Bart Horn