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Related papers: The Blazar Hadronic Code Comparison Project

200 papers

The measured spectral energy distribution and variability time scale are used to determine the radiation and magnetic-field energy densities in the relativistic plasma that forms the gamma-ray emitting jet in the blazar 3C 279. Assuming…

Astrophysics · Physics 2007-05-23 C. D. Dermer , A. Atoyan

We present a numerical code, written in C, which can be used to simulate or to analyze the emission of Blazars over the entire electromagnetic spectrum. Our code can reproduce the following features: synchrotron emission, inverse Compton…

Astrophysics · Physics 2009-11-07 Andrea Tramacere , Gino Tosti

Context: It has been proposed that the origin of the very high-energy photons emitted from high-mass X-ray binaries with jet-like features, so-called microquasars (MQs), is related to hadronic interactions between relativistic protons in…

Astrophysics · Physics 2008-01-15 M. Orellana , P. Bordas , V. Bosch-Ramon , G. E. Romero , J. M. Paredes

We report the results of the search for the high-energy neutrino emission associated with blazar flares, accounting for a possible lag of neutrinos with respect to the electromagnetic emission, either due to the slowness of the proton…

High Energy Astrophysical Phenomena · Physics 2026-02-06 Egor Podlesnyi , Foteini Oikonomou

The theoretical and experimental aspects of particle production from the strong equivalent photon fluxes present at high energy hadron colliders are reviewed. The goal is to show how photons at hadron colliders can improve what we have…

High Energy Physics - Phenomenology · Physics 2010-01-27 Joakim Nystrand

The production of hadronic final states in electron-positron or electron-hadron collisions is induced predominantly by quasi-real photons that were emitted off incoming leptons. In these processes, the photon either enters directly or…

High Energy Physics - Phenomenology · Physics 2026-02-27 Thomas Gehrmann , Peter Meinzinger

We present a model for high-energy emission in microquasars where the energy content of the jets is dominated by relativistic protons. We also include a primary leptonic component. Particles are accelerated up to relativistic energies in a…

Astrophysics · Physics 2009-11-13 Gabriela S. Vila , Gustavo E. Romero

Final states with a vector boson and a hadronic jet allow one to infer the Born-level kinematics of the underlying hard scattering process, thereby probing the partonic structure of the colliding protons. At forward rapidities, the parton…

High Energy Physics - Phenomenology · Physics 2019-06-26 A. Gehrmann-De Ridder , T. Gehrmann , E. W. N. Glover , A. Huss , D. M. Walker

We propose novel numerical schemes based on the Boris method in curved spacetime, incorporating both hadronic and radiative interactions for the first time. Once the proton has lost significant energy due to radiative and hadronic losses,…

High Energy Astrophysical Phenomena · Physics 2025-05-12 Minghao Zou , Hayk Hakobyan , Rostom Mbarek , Bart Ripperda , Fabio Bacchini , Lorenzo Sironi

The high-peaked BL Lac object Pks2155-304 shows high variability at multiwavelengths, i.e. from optical up to TeV energies. A giant flare of around 1 hour at X-ray and TeV energies was observed in 2006. In this context, it is essential to…

High Energy Astrophysical Phenomena · Physics 2016-05-25 Julia K. Becker , Athina Meli , Peter L. Biermann

X-ray bright knots of kpc-scale jets of several radio loud quasars have been an actively discussed issue. Among various models to explain observations, synchrotron radiation from the electron population different from radio to IR emitting…

High Energy Astrophysical Phenomena · Physics 2018-08-01 Masaaki Kusunose , Fumio Takahara

Hadronic antenna patterns provide a tool able to diagnose different patterns of colour flow in large-E_T jet events. They reflect the underlying short-distance dynamics, and are sensitive to colour coherence and interference between the…

High Energy Physics - Phenomenology · Physics 2009-09-11 John Ellis , Valery A. Khoze , W. J. Stirling

The observation of a very-high-energy neutrino by IceCube (IceCube-170922A) and its association with the flaring blazar TXS 0506+056 provided the first multimessenger observations of blazar jets, demonstrating the important role of protons…

High Energy Astrophysical Phenomena · Physics 2021-12-08 Sargis Gasparyan , Damien Bégué , Narek Sahakyan

Many luminous blazars which are associated with quasar-type active galactic nuclei display broad-band spectra characterized by a large luminosity ratio of their high-energy (gamma-ray) and low-energy (synchrotron) spectral components. This…

Cosmology and Nongalactic Astrophysics · Physics 2010-02-02 Marek Sikora , Lukasz Stawarz , Rafal Moderski , Krzysztof Nalewajko , Greg Madejski

The identification of astrophysical sources responsible for high-energy cosmic neutrinos has long been a challenge. A significant milestone was achieved with the blazar TXS 0506+056, which was found to be in a flaring state of high…

High Energy Astrophysical Phenomena · Physics 2025-11-27 Francesco Carenini , Matteo Cerruti

The construction of modern detectors used in high-energy physics experiments is typically guided by modeling with the Geant4 toolkit to evaluate detector performance in terms of geometrical acceptance and detection efficiency. Several…

Instrumentation and Detectors · Physics 2026-01-05 S. D. Savenkov , A. O. Svetlichnyi , I. A. Pshenichnov

Context.Blazars, a sub-category of Active Galactic Nuclei, are characterized by their non-thermal variable emission. This emission extends over the whole electromagnetic spectrum and is a consequence of particle acceleration inside their…

High Energy Astrophysical Phenomena · Physics 2021-12-22 Stella S. Boula , Apostolos Mastichiadis

We re\,examine the theory of hadronic photon-nucleon interactions at the quark-gluon level. The possibility of multiple parton collisions in a single photon-nucleon collision requires an eikonal treatment of the high-energy scattering…

High Energy Physics - Phenomenology · Physics 2014-11-17 K. Honjo , L. Durand , R. Gandhi , I. Sarcevic , H. Pi

In this work, we simulate $\gamma$-rays created in the hadronic jets of the compact object in binary stellar systems known as microquasars. We utilize as main computational tool the $3$-D relativistic magneto-hydro-dynamical code PLUTO…

High Energy Astrophysical Phenomena · Physics 2018-08-02 Odysseas Kosmas , Theodoros Smponias

We model multiwavelength afterglow data from the short Gamma-Ray Burst (GRB) 090510 using a combined leptonic-hadronic model of synchrotron radiation from an adiabatic blast wave. High energy, >100 MeV, emission in our model is dominated by…

High Energy Astrophysical Phenomena · Physics 2010-11-09 Soebur Razzaque