معرفی
Robert Wagoner is Professor of Physics, Emeritus at Stanford University and member of the Kavli Institute for Particle Astrophysics and Cosmology. Educated at Cornell (B.M.E.) and Stanford (M.S., Ph.D. Physics), his research specializes in theoretical astrophysics and cosmology. Pioneering work includes the first complete calculation of primordial element abundances with Fowler and Hoyle. Current research focuses on black hole accretion physics, quasi-periodic oscillations, and supernova morphology.
Research domains include:
- Black hole accretion disk dynamics and oscillation modes
- Cosmological nucleosynthesis and early universe physics
- Gravitational radiation from compact objects
- Observational signatures in active galactic nuclei
- Supernova ejecta and distance measurement techniques
Recent publications demonstrate innovative approaches to measuring cosmological distances through supernova studies and analyzing quasi-periodic oscillations in black hole systems using space telescope data.
۰مقاله منتشرشده
