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Price is probably best known for a 1972 result now known as [[Price's theorem]]. This is usually informally stated as follows: ''any inhomogeneities in the spacetime geometry outside a black hole will be radiated away''. (Any such inhomogeneities can be quantified as nonzero higher [[multipole moment]]s.) Price's theorem explains how the [[no hair theorem]] is enforced. Price also made pioneering numerical simulations which established (nonrigorously) a precise scenario for the emission of gravitational radiation during the merger of two compact objects (such as two [[black hole]]s). Subsequent work has largely confirmed the scenario which was first developed in his work. These simulations have provided a major impetus for the development of [[gravitational wave]] detectors such as [[LIGO]].
Price is probably best known for a 1972 result now known as [[Price's theorem]]. This is usually informally stated as follows: ''any inhomogeneities in the spacetime geometry outside a black hole will be radiated away''. (Any such inhomogeneities can be quantified as nonzero higher [[multipole moment]]s.) Price's theorem explains how the [[no hair theorem]] is enforced. Price also made pioneering numerical simulations which established (nonrigorously) a precise scenario for the emission of gravitational radiation during the merger of two compact objects (such as two [[black hole]]s). Subsequent work has largely confirmed the scenario which was first developed in his work. These simulations have provided a major impetus for the development of [[gravitational wave]] detectors such as [[LIGO]].


He has done much in development of pedagogical techniques in physics at levels of undergraduate and graduate education. He creates beautiful atlases of relativity.
He has done much in development of pedagogical techniques in physics at levels of . He creates beautiful atlases of relativity.


Price is the coauthor of three well known books in [[general relativity]].
Price is the coauthor of three well known books in [[general relativity]].

Revision as of 12:33, 16 December 2010

Richard H. Price
Born (1943-03-01) March 1, 1943 (age 81)
Nationality American
Alma materStuyvesant High School, Caltech, Cornell University
Known forRelativity and Cosmology
Scientific career
FieldsPhysics
InstitutionsUniversity of Texas at Brownsville, University of Utah
Doctoral advisorKip Thorne

Richard H. Price (born March 1, 1943) is a leading American physicist, well known for his important work in general relativity.

Price graduated from Stuyvesant High School in 1960, and went on to earn a dual degree in physics and engineering from Cornell University in 1965. He earned his Ph.D. in 1971 from Caltech under the supervision of Kip Thorne. He has spent most of his career at the University of Utah, but in 2004 joined Center for Gravitational Wave Astronomy at the University of Texas at Brownsville.

Price is probably best known for a 1972 result now known as Price's theorem. This is usually informally stated as follows: any inhomogeneities in the spacetime geometry outside a black hole will be radiated away. (Any such inhomogeneities can be quantified as nonzero higher multipole moments.) Price's theorem explains how the no hair theorem is enforced. Price also made pioneering numerical simulations which established (nonrigorously) a precise scenario for the emission of gravitational radiation during the merger of two compact objects (such as two black holes). Subsequent work has largely confirmed the scenario which was first developed in his work. These simulations have provided a major impetus for the development of gravitational wave detectors such as LIGO.

He has done much in development of pedagogical techniques in physics at the undergraduate, graduate, and postdoc levels; a significant portion at the University of Utah in Salt Lake City, UT. He creates beautiful atlases of relativity. He continues to teach and do research into his E Meritus career at the University of Texas (UT) at Brownsville.

Price is the coauthor of three well known books in general relativity.

References

  • Lightman, Alan P.; Press, William H.; Price, Richard H.; and Teukolsky, Saul A. (1975). Problem Book in Relativity and Gravitation. Princeton: Princeton University Press. ISBN 0-691-08162-X.{{cite book}}: CS1 maint: multiple names: authors list (link)
  • Thorne, Kip S.; Price, Richard H.; and Macdonald, Douglas A. (1986). Black Holes: the Membrane Paradigm. New Haven: Yale University Press. ISBN 0-300-03770-8.{{cite book}}: CS1 maint: multiple names: authors list (link)
  • Hawking, Stephen W.; Thorne, Kip S.; Novikov, Igor; Ferris, Timothy; Lightman, Alan; Price, Richard H. (2002). The Future of Spacetime. New York, NY: W. W. Norton & Co. ISBN 0-393-02022-3.{{cite book}}: CS1 maint: multiple names: authors list (link)

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