James M. Bardeen

James M. Bardeen (1980)

James Maxwell Bardeen (born May 9, 1939) is an American physicist, well known for his work in general relativity, particularly his role in formulating the laws of black hole mechanics. He also discovered the Bardeen vacuum, an exact solution of the Einstein field equation.

Bardeen graduated from Harvard in 1960 and earned his doctorate at Caltech under the direction of Richard Feynman.^[1] He is a professor emeritus of physics at the University of Washington in Seattle, and a Distinguished Visiting Research Fellow^[2] at Perimeter Institute for Theoretical Physics. In 2012 he was elected to the U.S. National Academy of Sciences.^[3]

Bardeen is the son of two-time Nobel Laureate John Bardeen.^[4] His brother, William A. Bardeen, is also a physicist, and his late sister Elizabeth was married to Thomas J. Greytak, a physicist at MIT.

Notes

↑ Bardeen, James Maxwell - CaltechTHESIS
↑ "James Bardeen". Perimeter Institute for Theoretical Physics. Perimeter Institute for Theoretical Physics. Retrieved 12 January 2016.
↑ James Bardeen, Array of Contemporary American Physicists
↑ Hoddeson, Lillian; Daitch, Vicki (2002). True genius: the life and science of John Bardeen : the only winner of two Nobel Prizes in physics. Joseph Henry Press. p. 93. ISBN 978-0-309-08408-6.

External links

James Bardeen, Perimeter Institute homepage
Publications of James Maxwell Bardeen in the database SPIRES
arXiv.org preprints for J. Bardeen
search on author James Bardeen from Google Scholar

Relativity

Special
relativity

Background	Principle of relativity Special relativity
Foundations	Frame of reference Speed of light Hyperbolic orthogonality Rapidity Maxwell's equations
Formulation	Galilean relativity Galilean transformation Lorentz transformation
Consequences	Time dilation Relativistic mass Mass–energy equivalence Length contraction Relativity of simultaneity Relativistic Doppler effect Thomas precession Relativistic disks
Spacetime	Light cone World line Spacetime diagram Biquaternions Minkowski space

General
relativity

Background	Introduction Mathematical formulation
Fundamental concepts	Special relativity Equivalence principle World line Riemannian geometry Minkowski diagram Penrose diagram
Phenomena	Black hole Event horizon Frame-dragging Geodetic effect Lenses Singularity Waves Ladder paradox Twin paradox Two-body problem
Equations	ADM formalism BSSN formalism Einstein field equations Geodesic equation Friedmann equations Linearized gravity Post-Newtonian formalism Raychaudhuri equation Hamilton–Jacobi–Einstein equation Ernst equation
Advanced theories	Brans–Dicke theory Kaluza–Klein Mach's principle Quantum gravity
Solutions	Schwarzschild (interior) Reissner–Nordström Gödel Kerr Kerr–Newman Kasner Taub–NUT Milne Robertson–Walker pp-wave van Stockum dust Weyl−Lewis−Papapetrou

Scientists

Einstein field equations:

G_{\mu \nu }+\Lambda g_{\mu \nu }={8\pi G \over c^{4}}T_{\mu \nu }

and their analytical solution by Ernst equation:

\displaystyle \Re (u)(u_{rr}+u_{r}/r+u_{zz})=(u_{r})^{2}+(u_{z})^{2}.

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