Accès ouvert
2026
article
OpenAlex
Keyan Gootkin, Colby C. Haggerty, Damiano Caprioli, Zachary Davis
Abstract Collisionless, turbulent plasmas surround the Earth, from the magnetosphere to the intergalactic medium, and the fluctuations within them affect nearly every field in the space sciences, from space weather forecasts to theories of galaxy formation. Where turbulent motions become supersonic, their …
us
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Accès ouvert
2026
article
OpenAlex
Zachary Davis, Luca Comisso, Colby C. Haggerty, Joonas Nättilä
Abstract Coherent structures created through turbulent cascades play a key role in energy dissipation and particle acceleration. In this work, we investigate both current and vorticity sheets in 3D particle-in-cell simulations of decaying relativistic turbulence in pair plasma by training a self-organizing …
us, fi
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Accès ouvert
2025
preprint
OpenAlex
Zachary Davis, Luca Comisso, Colby C. Haggerty, Joonas Nättilä
Coherent structures created through turbulent cascades play a key role in energy dissipation and particle acceleration. In this work, we investigate both current and vorticity sheets in 3D particle-in-cell simulations of decaying relativistic turbulence in pair plasma by training a self-organizing map …
Accès ouvert
2025
article
OpenAlex
D. Desai, Colby C. Haggerty, Benjamin J. Shappee, Michael A. Tucker et autres
ABSTRACT The light curves of radioactive transients, such as supernovae and kilonovae, are powered by the decay of radioisotopes, which release high-energy leptons through $\beta ^+$ and $\beta ^-$ decays. These leptons deposit energy into the expanding ejecta. As the ejecta density …
us, fr, au, es
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Accès ouvert
2024
article
OpenAlex
Carlos A. Giai, Colby C. Haggerty, Michael A. Shay, P. A. Cassak et autres
Abstract In magnetic reconnection, the ion bulk outflow speed and ion heating have been shown to be set by the available reconnecting magnetic energy, i.e., the energy stored in the reconnecting magnetic field (B r ). However, recent simulations, observations, and theoretical …
Accès ouvert
2024
article
OpenAlex
Zachary Davis, Jesús M. Rueda‐Becerril, Dimitrios Giannios
Abstract A wide range of astrophysical sources exhibit extreme and rapidly varying electromagnetic emission indicative of efficient nonthermal particle acceleration. Understanding these sources often involves comparing data with a broad range of theoretical scenarios. To this end, it is beneficial to have …
us
(code pays fourni par la source)
Accès ouvert
2024
preprint
OpenAlex
Zachary Davis, Jesús M. Rueda‐Becerril, Dimitrios Giannios
A wide range of astrophysical sources exhibit extreme and rapidly varying electromagnetic emission indicative of efficient non-thermal particle acceleration. Understanding these sources often involves comparing data with a broad range of theoretical scenarios. To this end, it is beneficial to have tools …
Accès ouvert
2024
article
OpenAlex
Zachary Davis, Luca Comisso, Dimitrios Giannios
Abstract Kinetic simulations of relativistic turbulence have significantly advanced our understanding of turbulent particle acceleration. Recent progress has highlighted the need for an updated acceleration theory that can account for particle acceleration within the plasma’s coherent structures. Here, we investigate how intermittency …
us
(code pays fourni par la source)
Accès ouvert
2023
preprint
OpenAlex
Zachary Davis, Luca Comisso, Dimitrios Giannios
Kinetic simulations of relativistic turbulence have significantly advanced our understanding of turbulent particle acceleration. Recent progress has highlighted the need for an updated acceleration theory that can account for acceleration within the plasma's coherent structures. Here, we investigate how turbulent intermittency models …
Accès ouvert
2022
article
OpenAlex
Zachary Davis, Jesús M. Rueda‐Becerril, Dimitrios Giannios
ABSTRACT Recently, particle-in-cell (PIC) simulations have shown that relativistic turbulence in collisionless plasmas can result in an equilibrium particle distribution function where turbulent heating is balanced by radiative cooling of electrons. Strongly magnetized plasmas are characterized by higher energy peaks and broader …
us
(code pays fourni par la source)