172 citations
- Institute of Nuclear Physics, Polish Academy of SciencesPL7 papers
- Centre National de la Recherche ScientifiqueFR5 papers
- Max Planck Institute for Nuclear PhysicsDE5 papers
- Jagiellonian UniversityPL4 papers
- CEA Paris-SaclayFR3 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR3 papers
- Deutsches Elektronen-Synchrotron DESYDE3 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR3 papers
- Maj Institute of PharmacologyPL3 papers
- Polish Academy of SciencesPL3 papers
- Universität HamburgDE3 papers
- Université Paris CitéFR3 papers
16 papers
Particle acceleration at recollimation shocks in sub-relativistic jets. A model for jets in Seyfert Galaxies, Microquasars and Protostellar Systems
Enrico Peretti, Elena Amato, Silvio Sergio Cerri +3
Growing observational evidence suggests that subrelativistic (SR) astrophysical jets may accelerate particles at slowly evolving standing shocks. Recollimation shocks (RCS) are exp…
The environment of TeV halo progenitors
Lioni-Moana Bourguinat, Carmelo Evoli, Pierrick Martin +1
TeV haloes are extended sources of very-high-energy gamma rays found around some middle-aged pulsars. The emission spanning several tens of parsecs suggests an efficient confinemen…
Extended TeV Halos May Commonly Exist around Middle-Aged Pulsars
A. Albert, R. Alfaro, C. Alvarez +81
Extended gamma-ray emission around isolated pulsars at TeV energies, also known as TeV halos, have been found around a handful of middle-aged pulsars. The halos are significantly m…
Performance and radiation damage mitigation strategy for silicon photomultipliers on LEO space missions
L. Burmistrov, S. Davarpanah, M. Heller +13
Space missions require lightweight, low-power consuming, radiation-tolerant components. Silicon photomultipliers are increasingly used for detecting near-UV, optical, and infrared…
Weak bosons as partons below 10 TeV partonic center-of-momentum
Innes Bigaran, Richard Ruiz
We investigate the modeling of weak boson number densities for leptons and hadrons in practical calculations in the Standard Model. In the framework of the Effective Approximat…
Testing the Molecular Cloud Paradigm for Ultra-High-Energy Gamma Ray Emission from the Direction of SNR G106.3+2.7
R. Alfaro, C. Alvarez, J. C. Arteaga-Velázquez +87
Supernova remnants (SNRs) are believed to be capable of accelerating cosmic rays (CRs) to PeV energies. SNR G106.3+2.7 is a prime PeVatron candidate. It is formed by a head region,…