activity
20152024
most citedA numerical approach for radiative cooling in relativistic outflows

3 citations · 4 across the 4 of their papers we have counts for

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10 papers · 1 filter

astro-ph.HE2024

Tleco: A Toolkit for Modeling Radiative Signatures from Relativistic Outflows

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 so…

astro-ph.HE2022

Balancing Turbulent Heating with Radiative Cooling in Blazars

Zachary Davis, Jesús M. Rueda-Becerril, Dimitrios Giannios

Recently, particle in cell (PIC) simulations have shown that relativistic turbulence in collisionless plasmas can result in an equilibrium particle distribution function where turb…

astro-ph.HE2021

Handing off the outcome of binary neutron star mergers for accurate and long-term post-merger simulations

Federico G. Lopez Armengol, Zachariah B. Etienne, Scott C. Noble +20

We perform binary neutron star (BNS) merger simulations in full dynamical general relativity with IllinoisGRMHD, on a Cartesian grid with adaptive-mesh refinement. After the remnan…

astro-ph.HE2021

HARM3D+NUC: A new method for simulating the post-merger phase of binary neutron star mergers with GRMHD, tabulated EOS and neutrino leakage

Ariadna Murguia-Berthier, Scott C. Noble, Luke F. Roberts +25

The first binary neutron star merger has already been detected in gravitational waves. The signal was accompanied by an electromagnetic counterpart including a kilonova component p…

astro-ph.HE2020

The blazar sequence revised

Jesús M. Rueda-Becerril, Amanda O. Harrison, Dimitrios Giannios

We propose and test a fairly simple idea that could account for the blazar sequence: all jets are launched with similar energy per baryon, independently of their power. For instanc…

astro-ph.HE2020★ 3 cited

A numerical approach for radiative cooling in relativistic outflows

Jesús M. Rueda-Becerril

In high energy astrophysics scenarios such as blazars, GRBs or PWNe, it is highly probable that ultra-relativistic particles interact with photons in their environment through scat…