English
Related papers

Related papers: ExHaLe-jet: An extended hadro-leptonic jet model f…

200 papers

We present a model to estimate the synchrotron radio emission generated in microquasar (MQ) jets due to secondary pairs created via decay of charged pions produced in proton-proton collisions between stellar wind ions and jet relativistic…

Astrophysics · Physics 2009-06-23 P. Bordas , J. M. Paredes , V. Bosch-Ramon , M. Orellana

The spectra of blazars form a sequence which can be parametrized in term of their observed bolometric luminosity. At the most powerful extreme of the sequence we find objects whose jet power can rival the power extracted by accretion, while…

Astrophysics · Physics 2007-05-23 G. Ghisellini

In this paper we develop the jet model of Potter & Cotter (2012) to include a magnetically dominated accelerating parabolic base transitioning to a slowly decelerating conical jet with a geometry set by recent radio observations of M87. We…

High Energy Astrophysical Phenomena · Physics 2015-06-12 William J. Potter , Garret Cotter

Relativistic plasma flows from the jets of black hole binary systems consist the environment of multiple particle production and radiation emission including neutrinos and gamma-rays. We implement a hadronic model based on $p-p$…

High Energy Astrophysical Phenomena · Physics 2022-10-05 Theodora V. Papavasileiou , Odysseas T. Kosmas , Ioannis Sinatkas

The production in high-energy hadron collisions of a pair of jets with large rapidity separation is studied in an improved BFKL formalism. By recasting the analytic solution of the BFKL equation as an explicit order-by-order sum over…

High Energy Physics - Phenomenology · Physics 2016-08-25 Lynne H. Orr , W. J. Stirling

There is a large variety in the models explaining blazar flares. Here, we study the flare profile induced by a moving and expanding blob with special emphasize on the gamma-gamma pair production. We first develop a simple semi-analytical…

High Energy Astrophysical Phenomena · Physics 2023-02-01 Michael Zacharias

With their jet pointing towards us, blazars are ideal tools to study the physics and structure of extragalactic jets. Their powerful jets are cosmic particle accelerators and are alleged to be one of the production sites of the high-energy…

High Energy Astrophysical Phenomena · Physics 2025-11-25 Claudia M. Raiteri

The origin of high-energy emission in blazars jets (i.e., leptonic versus hadronic) has been a long-standing matter of debate. Here, we focus on one variant of hadronic models where proton synchrotron radiation accounts for the observed…

High Energy Astrophysical Phenomena · Physics 2020-04-28 I. Liodakis , M. Petropoulou

The beaming pattern of radiation emitted by a relativistically moving source like jets in microquasars, AGN and GRBs, is a key issue for understanding of acceleration and radiation processes in these objects. In this paper we introduce a…

High Energy Astrophysical Phenomena · Physics 2018-05-30 S. R. Kelner , E. Lefa , F. M. Rieger , F. A. Aharonian

Multifrequency polarimetry, recently extended to the X-ray band thanks to the Imaging X-ray Polarimetry Explorer (IXPE) satellite, is an essential tool for understanding blazar jets. High-frequency-peaked BL Lacs (HBLs) and extreme…

High Energy Astrophysical Phenomena · Physics 2025-07-23 Alberto Sciaccaluga , Agnese Costa , Fabrizio Tavecchio , Gianluigi Bodo , Paolo Coppi , Stella Boula

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 consider the emission processes in the large-scale jets of powerful quasars based on the results obtained with the VLA, Spitzer, Hubble, and Chandra. We show that two well-known jets, 3C 273 and PKS 1136-135, have two distinct spectral…

Astrophysics · Physics 2011-03-10 Yasunobu Uchiyama

Blazars, a class of active galaxies whose jets are relativistic and collimated flows of plasma directed along the line of sight and are prone to a slew of magneto-hydrodynamic (MHD) instabilities. We aim to study the interplay of radiation…

High Energy Astrophysical Phenomena · Physics 2023-03-22 Sriyasriti Acharya , Bhargav Vaidya , Indu Kalpa Dihingia , Sushmita Agarwal , Amit Shukla

Galactic black-hole X-ray binaries emit a compact, optically thick, mildy relativistic radio jet when they are in the hard and hard-intermediate states. In a series of papers, we have developed a jet model and have shown, through Monte…

High Energy Astrophysical Phenomena · Physics 2017-10-25 P. Reig , N. Kylafis

About one thousand extragalactic large-scale jets are known, and a few tens of them are confirmed sources of infrared, optical, or X-ray photons. Multiwavelength emission comming directly from these outflows is always non-thermal in origin.…

Astrophysics · Physics 2016-08-30 L. Stawarz

Single particles and jets in deeply inelastic scattering at low x are measured with the H1 detector in the region away from the current jet and towards the proton remnant, known as the forward region. Hadronic final state measurements in…

High Energy Physics - Experiment · Physics 2010-03-25 C. Adloff

We study jet physics in the high energy regime of QCD. Based on the NLO BFKL equation, we construct a vertex for the production of a jet at central rapidity in k_T-factorization. A jet algorithm is introduced, and we take special care of…

High Energy Physics - Phenomenology · Physics 2007-05-23 Florian Schwennsen

In the modelling of blazars and other radiating plasma flows, correctly evolving in time a series of kinetic equation coupled for different particle species is a computationally challenging problem. In this paper we introduce the code Katu,…

High Energy Astrophysical Phenomena · Physics 2021-04-19 Bruno Jiménez Fernández , Hendrik van Eerten

We propose a jet model for the low/hard state of Galactic black-hole X-ray sources that can explain the energy spectra from radio to X-rays. The model assumes that i) there is a magnetic field along the axis of the jet; ii) the electron…

Astrophysics · Physics 2009-11-10 Dimitrios Giannios

In this work we present a new jet model for the non-thermal broadband emission of low-mass microquasars. We calculate the contribution of relativistic particles, primary electrons and protons as well as secondary muons, charged pions and…

High Energy Astrophysical Phenomena · Physics 2015-03-19 Gabriela S. Vila , Gustavo E. Romero