Stuart L. Shapiro

Professor

Biography

Professor Stuart Shapiro received an A.B in astronomy from Harvard in 1969 and M.A. and Ph.D. degrees in astrophysical sciences from Princeton University in 1971 and 1973, respectively. He went from research associate to full professor of astronomy and physics at Cornell University (1973-1995) before relocating to the University of Illinois in 1996.

Professor Shapiro has broad research interests that span many areas of theoretical astrophysics and general relativity theory, including the physics of black holes and neutron stars, gravitational collapse, the generation of gravitational waves, and the dynamics of large N-body dynamical systems. His research emphasizes the use of supercomputers to solve long-standing, fundamental problems in numerical relativity and computational astrophysics. Shapiro has worked on the theory of accretion onto compact objects, relativistic stellar dynamics, gravitational collapse, binary black hole and neutron star inspiral and coalescence, the generation of gravitational waves, the formation of black holes, Big-Bang nucleosynthesis and neutrino astrophysics, to name a few topics. Some of his most important simulations include the emitted radiation spectrum from gas accreting onto black holes and neutron stars, the disruption and consumption of stars in star clusters containing a central supermassive black hole, the formation of a supermassive black hole at the center of a galaxy or quasar from the collapse of a relativistic collisionless gas, the head-on collision and merger of two black holes, and the gravitational wavetrain from the late inspiral of coalescing binary neutron stars. He merged the fields of stellar dynamics and numerical relativity, a development which led to the simulation of the catastrophic collapse of an unstable, relativistic cluster to a black hole, the demonstration that toroidal black holes can arise as transients during gravitational collapse, and the possibility that naked singularities might form during the collapse of collisionless matter from reasonable initial conditions, thereby violating cosmic censorship. Long interested in the future detection of gravitational waves by laser interferometers like LIGO and LISA, Shapiro and his group are working on the theory of gravitational wave generation and the identification of promising astrophysical sources.

Professor Shapiro's deep interest in training young scientists has given him a reputation as an inspiring and effective classroom teacher and research advisor. He has created and taught over a dozen courses in physics and astrophysics. The textbook that he coauthored, Black Holes, White Dwarfs and Neutron Stars: The Physics of Compact Objects (John Wiley, 1983) is a standard in the field. His research has led him to develop numerous videos of his computer simulations, which offer both great technical insight to experts and qualitative understanding to non-specialists. He leads a vibrant group of graduate students and postdocs working in theoretical astrophysics and general relativity. For over two decades he has trained an expert team of advanced undergraduates doing research in theoretical astrophysics and general relativity by means of supercomputer simulation and visualization. His undergraduate research program is among the most successful in the nation; members of his team are highly sought after by the most select graduate programs in physics, astronomy, computer science, and related areas.

Research Statement

With my group I will pursue research in general relativity and theoretical astrophysics funded by my NSF and NASA grants. Our area of focus will be tackling problems involving general relativity, the generation of gravitational radiation, relativistic hydrodynamics, and relativistic magnetohydrodynamics. A common thread uniting the different theoretical topics is the crucial role of gravitation, especially relativistic gravitation. Compact objects provide the principal forum, and the dynamics of matter in a strong gravitational field is a major theme. Some of the topics for investigation include the inspiral and coalescence of compact binaries (binary black holes, binary neutron stars, binary black hole--neutron stars and binary white dwarf-neutron stars), the generation of gravitational waves from binaries and othe rpromising astrophysical sources and the accompanying electromagnetic signals, gravitational collapse, the stability of rotating, relativistic stars and the evolution and final fate of unstable stars, gamma-ray burst sources, and circumbinary disks around merging supermassive black holes in the cores of galaxies and quasars. Most of these topics represent long-standing, fundamental problems in theoretical physics requiring large-scale computation for solution. Hence the approach involves to a significant degree large-scale computations on parallel machines, as well as analytical modeling. Many of the numerical calculations employ the state-of-the-art computational and visualization resources of the UIUC's National Center for Supercomputing Applications (NCSA), including Blue Waters. They comprise both initial value and evolution computations and treat vacuum spacetimes containing black holes as sell as spacetimes containing realistic matter sources, magnetic fields and both electromagnetic and neutrino radiation. The results have important implications for astronomical observations, including those planned for gravitational wave interferometers, such as the Advanced LIGO/VIRGO network, GEO, KAGRA and eLISA, and for telescopes that will measure transient optical events, such as the LSST.

Research Honors

  • Amity High School Hall of Honor (2006)
  • Fellow, Institute of Physics, U.K. (2004)
  • Fellow, American Physical Society (1998)
  • Offered Beatrice Tinsley Visiting Professor of Astronomy, Univ. Texas (1996)
  • First Prize, IBM Supercomputing Competition (1991)
  • Forefronts of Large-Scale Computation Award (1990)
  • IBM Supercomputing Competition Award (1990)
  • John Simon Guggenheim Memorial Foundation Fellowship (1989-90)
  • Association of American Publishers Award (1984)
  • Alfred P. Sloan Research Fellowship (1979)

Semesters Ranked Excellent Teacher by Students

SemesterCourseOutstanding
Spring 2016PHYS 516
Spring 2012PHYS 516

Selected Articles in Journals

  • Z. B. Etienne, Y. T. Liu, V. Paschalidis and S. L. Shapiro, "General Relativistic Simulations of Black Hole-Neutron Star Mergers: Effects of Magnetic Fields", Phys. Rev. D., 85, 064029/1-30 (2012).
  • Z. B. Etienne, V. Paschalidis, Y. T. Liu, and S. L. Shapiro, "Relativistic MHD in Dynamical Spacetimes: Improved EM Gauge Condition for AMR Grids", Phys. Rev. D., 85, 024013/1-10 (2012).
  • A. N. Staley, T.W. Baumgarte, J. D. Brown, B. D. Farris and S. L. Shapiro, "Oppenheimer-Snyder Collapse in Moving-Puncture Coordinates", Classical and Quantum Gravity, 29, 015003/1-17 (2012).
  • V. Paschalidis, Y. T. Liu, Z. B. Etienne and S. L. Shapiro, "Merger of Binary White Dwarf-Neutron Stars: Simulations in Full General Relativity", Phys. Rev. D., 84, 104032/1-24 (2011).
  • T.W. Baumgarte and S. L. Shapiro, "Binary Black Hole Mergers", Physics Today, 64, Issue 10, 32-37 (2011). (Feature article and front cover)

Related news

  • Research

In less than the blink of an eye Einstein’s theory of relativity is on its way to becoming just another science fact. Scientists observed gravitational waves—ripples in the fabric of spacetime for the second time—and researchers at the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign were part of the Ligo collaboration identifying the event.

Congratulations to the LIGO Scientific Collaboration on its historic discovery, the observation of gravitational waves! Your friends and colleagues at Physics Illinois are celebrating the spacetime ripples with you!

For the first time, scientists have observed ripples in the fabric of spacetime called gravitational waves, arriving at the earth from a cataclysmic event in the distant universe. This confirms a major prediction of Albert Einstein’s 1915 general theory of relativity and opens an unprecedented new window onto the cosmos.

Stuart Shapiro, a professor of physics and astronomy at Illinois, was appointed an NCSA research scientist by NCSA founder Larry Smarr two decades ago. A leading expert in the theory that underpinned the search for gravitational waves, Shapiro has developed software tools that can simulate on NCSA supercomputers like Blue Waters the very binary black hole merger and gravitational waves now detected by LIGO. Shapiro said he is thrilled by the discovery.

Shapiro comments on LIGO's discovery: "This presents the strongest confirmation yet of Einstein's theory of general relativity and the cleanest evidence to date of the existence of black holes. The gravitational waves that LIGO measures can only be generated by merging black holes – exotic relativistic objects from which nothing, including light, can escape from their interior."

  • Research
  • Astrophysics/Cosmology
  • Astrophysics

One of the principal strategies to indirectly detect dark matter is to search for the photons produced when it annihilates. Such searches look for gamma rays or x rays in regions of the sky where dark matter is known to be abundant. Professors Jessie Shelton, Stuart Shapiro, and Brian Fields at the University of Illinois at Urbana–Champaign have proposed to look inside dark matter spikes induced by the gravitational pull of supermassive black holes. Such measurements could test so called p-wave dark matter models.