James Wellington Truran Jr. (born July 12, 1940, Brewster, New York[1] – March 5, 2022) was an American physicist, known for his research in nuclear astrophysics.[2]
He did important research on "novae, supernovae, nucleosynthesis, and galactic chemical evolution through the application of nuclear physics to astrophysics."[6] His Ph.D. thesis and subsequent research led to accurate prediction of the production of the 56Ni in Type Ia supernovae. Radioactive decay of 56Ni through 56Co to 56Fe produces high-energy photons, which dominate the energy output of Type Ia supernova ejecta at intermediate to late times.[7]
Truran's research includes s-processes in stars, carbon explosion models of Type Ia supernovae, and r-processes in metal-poor stars. He was involved in the development of the FLASH simulation code for thermonuclear supernova explosions.
Truran was a member of the AURA "HST and Beyond" Committee,[10] which in 2017 received the Carl Sagan Memorial Award. In 2020, he received the Laboratory Astrophysics Prize of the American Astronomical Society's Laboratory Astrophysics Division (LAD) "for his theoretical work on early star formation and the nucleosynthesis history of the universe, as well as for his seminal contributions to the study of astrophysical thermonuclear explosions, nucleosynthesis, and the use of nuclear-decay chronometers to determine ages of stellar and terrestrial matter."[11] He was awarded in 2021 the Hans A. Bethe Prize for "distinguished contributions across the breadth of nuclear astrophysics, Galactic chemical evolution and cosmochronology."[12]
Upon his death he was survived by his widow, three daughters, four grandchildren, and one great-grandchild.[3]
Iben, I. Jr.; Kaler, J. B.; Truran, J. W.; Renzini, A. (1983). "On the evolution of those nuclei of planetary nebulae that experience a final helium shell flash". The Astrophysical Journal. 264: 605. Bibcode:1983ApJ...264..605I. doi:10.1086/160631.
Gehrz, Robert D.; Truran, James W.; Williams, Robert E.; Starrfield, Sumner (1998). "Nucleosynthesis in Classical Novae and Its Contribution to the Interstellar Medium". Publications of the Astronomical Society of the Pacific. 110 (743): 3–26. Bibcode:1998PASP..110....3G. doi:10.1086/316107. S2CID121557552.
Cowan, John J.; Sneden, Christopher; Burles, Scott; Ivans, Inese I.; Beers, Timothy C.; Truran, James W.; Lawler, James E.; Primas, Francesca; Fuller, George M.; Pfeiffer, Bernd; Kratz, Karl-Ludwig (2002). "The Chemical Composition and Age of the Metal-poor Halo Star BD +17o3248". The Astrophysical Journal. 572 (2): 861–879. arXiv:astro-ph/0202429. Bibcode:2002ApJ...572..861C. doi:10.1086/340347. S2CID119503888.
Sneden, Christopher; Cowan, John J.; Lawler, James E.; Ivans, Inese I.; Burles, Scott; Beers, Timothy C.; Primas, Francesca; Hill, Vanessa; Truran, James W.; Fuller, George M.; Pfeiffer, Bernd; Kratz, Karl-Ludwig (2003). "The Extremely Metal-poor, Neutron Capture–rich Star CS 22892-052: A Comprehensive Abundance Analysis". The Astrophysical Journal. 591 (2): 936–953. arXiv:astro-ph/0303542. Bibcode:2003ApJ...591..936S. doi:10.1086/375491. S2CID11466782.
^ ab"APS Fellow Archive". American Physical Society. (search on year=1987 and institution=University of Chicago)
^Truran, James W. (2006). "Supernova Explosions, Nucleosynthesis, and Cosmic Chemical Evolution". AIP Conference Proceedings. 848 (1). American Institute of Physics: 281–290. Bibcode:2006AIPC..848..281T. doi:10.1063/1.2347992.