Dimitrios Giannios
Physics and Astronomy · Purdue University West Lafayette
Publications
193
Citations
7,749
Est. group size
~1
Recurring co-author estimate
Active years
24
Publishing since 2003
Dimitrios Giannios studies extreme cosmic explosions and high-energy astrophysical processes, particularly gamma-ray bursts (brief, intense flashes of radiation from collapsing stars) and magnetic reconnection (a process where magnetic field energy converts into particle motion and radiation) near black holes and neutron stars. His work combines theoretical modeling and simulations to explain how particles are accelerated to extremely high energies and how this shapes the light and radiation we observe from these events. This research helps astronomers interpret real-world observations of jets, shocks, and turbulent magnetic environments in the universe.
Publication output has been fairly steady over the last decade, with year-to-year fluctuations (a peak around 2019 and a dip in 2025), but recent averages remain consistent with earlier activity.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- Maximum Energy of Particles Accelerated in Gamma-Ray Burst Afterglow Shocks
The Astrophysical Journal · 2026
- The effect of inverse Compton losses on particle acceleration in three-dimensional relativistic reconnection
arXiv (Cornell University) · 2026
- The effect of inverse Compton losses on particle acceleration in three-dimensional relativistic reconnection
arXiv (Cornell University) · 2026
- Maximum Energy of Particles Accelerated in Gamma-Ray Burst Afterglow Shocks
Open MIND · 2026
- Maximum Energy of Particles Accelerated in GRB Afterglow Shocks
arXiv (Cornell University) · 2026
- Thermal Electrons in an Ultra-Relativistic Shock Shape the Optical Afterglow of GRB 250702F
Open MIND · 2026
- Thermal Electrons in an Ultra-Relativistic Shock Shape the Optical Afterglow of GRB 250702F
ArXiv.org · 2026
- Thermal electrons in an ultra-relativistic shock shape the optical afterglow of GRB 250702F
Astronomy and Astrophysics · 2026
- Thermal electrons in an ultra-relativistic shock shape the optical afterglow of GRB 250702F
Springer Link (Chiba Institute of Technology) · 2026
- The Effect of Inverse Compton Losses on Particle Acceleration in Three-dimensional Relativistic Reconnection
The Astrophysical Journal · 2026
- Relativistic Magnetic Reconnection in Astrophysical Plasmas: A Powerful Mechanism of Nonthermal Emission
Annual Review of Astronomy and Astrophysics · 2025
- Maximal Jet Energy of Gamma-Ray Bursts through the Blandford–Znajek Mechanism
The Astrophysical Journal Letters · 2025
- Intermittency and Dissipative Structures Arising from Relativistic Magnetized Turbulence
The Astrophysical Journal · 2024
- Radiative properties of plasmoids and plasmoid mergers in magnetic reconnection
Monthly Notices of the Royal Astronomical Society · 2024
- The role of magnetospheric current sheets in pair enrichment and ultra-high energy proton acceleration in M87*
Journal of Cosmology and Astroparticle Physics · 2024
- Monthly Notices of the Royal Astronomical Society×31
- arXiv (Cornell University)×28
- The Astrophysical Journal×13
- The Astrophysical Journal Letters×8
- Monthly Notices of the Royal Astronomical Society Letters×7
- D. Milisavljević
Physics and Astronomy · Purdue University West Lafayette
- Danny Milisavljevic
Physics and Astronomy · Purdue University West Lafayette
- F. Aros
Physics and Astronomy · Indiana University
- Abigail Polin
Physics and Astronomy · Purdue University West Lafayette
- G. H. Sembroski
Physics and Astronomy · Purdue University West Lafayette
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Jul 20, 2026.
Claim or correct this profile