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Department of Physics
People

Robert Vernon Wagoner

Professor of Physics, Emeritus

Robert Vernon Wagoner 

Room 320
Varian Physics Bldg
382 Via Pueblo Mall
Stanford, CA 94305-4060
 

tel 650-723-4561

Email:
wagoner@stanford.edu

Research Interests

Various topics in gravitational astrophysics. Oscillations of accretion disks around black holes, and other signatures of very strong gravitational fields. Sources of gravitational radiation, and their detection by LIGO and other facilities. Scalar-tensor theories of gravitation. Physics of the early universe.

Black HoleThis is a computer-generated view of a black hole and its surrounding accretion disk, produced by my former Ph.D. student Chris Perez. The black hole is rotating with an angular momentum 50% of the maximum possible, aligned 30 degrees from the line of sight. The accretion disk is rotating in the same direction in the equatorial plane of the black hole. The intensity (at a fixed wavelength) is color coded from blue (maximum) to red (minimum).


Biography

Robert V. Wagoner's scientific direction was established rather suddenly in 1960, when he attended a series of lectures on cosmology by the British astrophysicist Fred Hoyle. At the time, Wagoner was a mechanical engineering undergraduate at Cornell University, receiving his B.M.E. in 1961. Born and raised in Teaneck, New Jersey, his other major interest was golf, leading to a position on the Cornell team. 

He switched to physics while at Stanford University, receiving an M.S. in engineering science in 1962 and a Ph.D. in physics in 1965. He then worked as a postdoctoral fellow at Caltech, collaborating with William A. Fowler and Hoyle on the definitive calculation of the abundances of the elements produced in the primordial universe. After three years, he returned to Cornell as a faculty member in the astronomy department. Five years later, he returned to Stanford's physics department, where he is a professor of physics and a member of the Kavli Institute for Particle Astrophysics and Cosmology.

His academic honors include Sloan Foundation and Guggenheim Foundation Fellowships. In 1976 he was a Sherman Fairchild Distinguished Scholar at Caltech and in 1978 he was the George Ellery Hale Distinguished Visiting Professor at the University of Chicago. Wagoner was also a Visiting Fellow at the Institute of Theoretical Astronomy in Cambridge, England during the summers of 1967 and 1971. He is a Fellow of the American Physical Society. 

Professor Wagoner's recent research in theoretical astrophysics focuses on strong gravitational fields in the universe (black holes and neutron stars). This includes relativistic diskoseismology: using the oscillations of the surrounding accretion disk to probe the nature of the central mass. It also includes studies of potential sources of gravitational radiation that may be detected by upcoming facilities such as LIGO. He has also investigated the use of supernovae to determine cosmological distances, and has studied alternative theories of gravitation. 

He lives on the Stanford campus with his wife Stephanie, and has two daughters (Alexa and Shannon) from a previous marriage. His athletic interest evolved from golf to running (five marathons), but has now reversed. 


Selected Publications


Recent Graduate Students


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