Donald Ellison

Bio

Professor Ellison received his PhD in 1982 from The Catholic University of America. He spent a year at the Service d’Astrophysique, Saclay, France before taking up a joint postdoctoral position at the University of Maryland and NASA/Goddard Space Flight Center. He joined the faculty of North Carolina State University in 1987. The year 1995 was spent on sabbatical at the Service d’Astrophysique and the Fall semester of 2007 was spent at the Kavli Institute for Particle Astrophysics and Cosmology at Stanford University.

Area(s) of Expertise

Most of Ellison's research has centered on developing theoretical models of particle acceleration mechanisms in astrophysics. He was among the first to recognize the importance of nonlinear effects in diffusive shock acceleration and he developed Monte Carlo computer simulations to investigate this effect. This work has been applied to the production of cosmic raysin supernova remnants as well as to collisionless shocks in the heliosphere. He was also among the first to investigate the effects of efficient particle acceleration in relativistic shocks with applications to gamma-ray bursts. Other research accomplishments associated with shocks include the modeling of the production of strong magnetic turbulence in shocks and the use of particle-in-cell computer simulations to investigate the injection of thermal particles into the diffusive shock acceleration mechanism.

Publications

• X-ray polarization: A view deep inside cosmic ray driven turbulence and particle acceleration in supernova remnants , PHYSICAL REVIEW D (2024)
• Uncovering Magnetic Turbulence in Young Supernova Remnants with Polarized X-Ray Imaging , ASTROPHYSICAL JOURNAL (2020)
• High-energy cosmic rays from compact galactic star clusters: Particle fluxes and anisotropy , ADVANCES IN SPACE RESEARCH (2019)
• High-energy cosmic rays from supernovae in young clusters of massive stars , RENDICONTI LINCEI-SCIENZE FISICHE E NATURALI (2019)
• Monte Carlo modelling of particle acceleration in collisionless shocks with effective mean electric field , INTERNATIONAL CONFERENCE PHYSICA.SPB/2019 (2019)
• Wolf-Rayet stars in young massive star clusters as potential sources of Galactic cosmic rays , INTERNATIONAL CONFERENCE PHYSICA.SPB/2019 (2019)
• Cosmic Ray Production in Supernovae , SPACE SCIENCE REVIEWS (2018)
• Supernovae in compact star clusters as sources of high-energy cosmic rays and neutrinos , ADVANCES IN SPACE RESEARCH (2018)
• High energy neutrinos and gamma-ray emission from supernovae in compact star clusters , HIGH ENERGY GAMMA-RAY ASTRONOMY (2017)
• Nonlinear Monte Carlo model of superdiffusive shock acceleration with magnetic field amplification , PHYSICAL REVIEW E (2017)

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