Tom Abel
Tom Abel (born 1970) is a German cosmologist who first simulated the collapse of a metal-free massive star that belongs to the first generation of stars in the Universe. This work was done in collaboration with Greg L. Bryan and Michael L. Norman and was published in Science magazine (2002, 295, 93). He received his Doctor of Philosophy from Ludwig Maximilian University of Munich in 2000.
He is a Professor of Physics at Stanford University in Palo Alto, California and of Particle Physics and Astrophysics at SLAC National Accelerator Laboratory and from 2013 to 2018 served as Director of the Kavli Institute for Particle Astrophysics and Cosmology.[1]
Background
Abel was born in rural Lower Bavaria, Germany.[2]
Work
His primary interests are:
- Primordial star formation
- Cosmological structure formation and reionization
- Astrophysical fluid dynamics
- Radiative transfer
gollark: I do all my 3D printing in CC anyway.
gollark: `paßtebin`?
gollark: No, but I was, as I said, considering smaller autoMELON™ stations.
gollark: You could also use a colourful lamp.
gollark: So this is some sort of autonomous snack vendinator?
References
- "Curriculum Vitae" (PDF). tomabel.org. Abel's personal website. Retrieved 20 April 2016.
- "Tom Abel » About Me". tomabel.org. Abel's personal website. Retrieved 11 September 2015.
External links
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.