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Lars Bildsten : ウィキペディア英語版 | Lars Bildsten Lars Bildsten (born 1964) is an American astrophysicist, best known for his work on the physics of white dwarfs and their explosions as Type Ia supernovae. He is the sixth director of the Kavli Institute for Theoretical Physics at the University of California, Santa Barbara (UCSB) and a professor in the UCSB Physics Department. ==Biography== Bildsten's undergraduate degree is in engineering physics, from Ohio State University.〔Caltech, 2003-2004 GALCIT Fluids Seminar, ("Lars Bildsten" )〕 Bildsten was a Hertz Foundation fellow and received a Ph.D. in theoretical physics at Cornell University in 1991. He was then a research fellow at Caltech for three years, after which he accepted a faculty appointment at the University of California, Berkeley. Rising from assistant to associate professor, in both the physics and astronomy departments, he moved to UCSB in 1999.〔Kavli Institute for Theoretical Physics, ("Lars Bildsten Biographical Sketch" )〕 In 2010, he was awarded the Wayne Rosing, Simon and Diana Raab chair in theoretical astrophysics. He was named director of the Kavli Institute, succeeding David Gross, in 2012.〔Kavli Foundation, ("Astrophysicist Lars Bildsten Appointed to Endowed Chair at Kavli Institute for Theoretical Physics" )〕 In addition to his university teaching and research, Bildsten has devoted significant effort to strengthening science and engineering education in grades 7-12. A member of the board of directors of Santa Barbara's Dos Pueblos Engineering Academy Foundation, he worked to raise $3 million in funding for a dedicated facility and to support math tutors.〔American Physical Society, ("Lars Bildsten, Candidate for Chair-Elect, Nominating Committee" )〕
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