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Plasma turbulence is ubiquitous in space and astrophysical plasmas, playing an important role in plasma energization, but the physical mechanisms leading to dissipation of the turbulent energy remain to be definitively identified. Kinetic…

Solar and Stellar Astrophysics · Physics 2016-12-06 Tak Chu Li , Gregory G. Howes , Kristopher G. Klein , Jason M. TenBarge

TeV BL Lacertae objects require extreme relativistic bulk motion in the gamma-ray emission region, but at the VLBI scale their radio knots hardly move. The same sources show evidence, in radio, of a structure made of a fast spine plus a…

Astrophysics · Physics 2010-04-06 G. Ghisellini , F. Tavecchio , M. Chiaberge

Gamma rays from TeV blazars have been detected by ground-based experiments for more than two decades. We have collected the most extensive set of archival spectra from these sources in order to constrain the processes affecting gamma-ray…

Cosmology and Nongalactic Astrophysics · Physics 2015-08-26 Jonathan Biteau , David A. Williams

TeV blazars are known as prominent nonthermal emitters across the entire electromagnetic spectrum with their photon power peaking in the X-ray and TeV bands. If distant, absorption of gamma-ray photons by the extragalactic background light…

Astrophysics · Physics 2009-08-07 A. Reimer , L. Costamante , G. Madejski , O. Reimer , D. Dorner

Fermi has been instrumental in constraining the luminosity function and redshift evolution of gamma-ray bright blazars. This includes limits upon the spectrum and anisotropy of the extragalactic gamma-ray background (EGRB), redshift…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-16 Avery E. Broderick , Christoph Pfrommer , Ewald Puchwein , Philip Chang

We investigate the hot electrons generated from two-plasmon decay (TPD) instability driven by laser pulses with intensity modulated by a frequency $\Delta \omega_m$. Our primary focus lies on scenarios where $\Delta \omega_m$ is on the same…

Plasma Physics · Physics 2023-11-28 C. Yao , J. Li , L. Hao , R. Yan , C. Wang , A. Lei , Y-K. Ding , J. Zheng

The arrival directions of Galactic cosmic rays exhibit anisotropies up to the level of one per-mille over various angular scales. Recent observations of TeV-PeV cosmic rays show that the dipole anisotropy has a strong energy dependence with…

High Energy Astrophysical Phenomena · Physics 2019-05-22 Markus Ahlers

We apply an inverse Compton $e^\pm$ pair cascade model for $\gamma$-ray production in massive binary system LSI +61$^{\rm o}$ 303 assuming that electrons are accelerated already inside the inner part of the jet launched by the compact…

Astrophysics · Physics 2009-11-11 W. Bednarek

Using the cosmic ray (CR) data available in the energy interval $(10 - 2 \times 10^{7})$ GeV/particle, we have calculated the profile of the primary $\gamma$-ray spectrum produced by the interaction of these CR with thermal nuclei of the…

Astrophysics · Physics 2009-10-30 G. A. Medina Tanco , E. M. de Gouveia Dal Pino

Sustained ELM mitigation has been achieved using RMPs with a toroidal mode number of n=4 and n=6 in lower single null and with n=3 in connected double null plasmas on MAST. The ELM frequency increases by up to a factor of eight with a…

Collisionless coupling between super Alfv\'{e}nic ions and an ambient plasma parallel to a background magnetic field is mediated by a set of electromagnetic ion/ion-beam instabilities including the resonant right hand instability (RHI). To…

Several cosmic-ray observatories have provided a high accuracy map of the sky at TeV--PeV energies. The data reveals an O(0.1%) deficit from north galactic directions that peaks at 10 TeV and then evolves with the energy, together with…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Eduardo Battaner , Joaquin Castellano , Manuel Masip

Lately a specific kind of blazars drew the attention of the gamma-ray astronomy community: the extreme TeV BL Lacs, blazars that present an extremely energetic and hard emission at very high-energy. Explaining their features is still an…

High Energy Astrophysical Phenomena · Physics 2022-10-12 Alberto Sciaccaluga , Fabrizio Tavecchio

We study mechanisms of multi-wavelength emissions (X-ray, GeV and TeV gamma-rays) from the gamma-ray binary LS~5039. This paper is composed of two parts. In the first part, we report on results of observational analysis using four year data…

High Energy Astrophysical Phenomena · Physics 2015-06-22 J. Takata , Gene C. K. Leung , P. H. T. Tam , A. K. H. Kong , C. Y. Hui , K. S. Cheng

A scenario in which cosmic rays (CRs) above $10^{20}{\rm eV}$ are produced by cosmological gamma-ray bursts (GRBs) is consistent with observations provided that deflections by the inter-galactic magnetic field (IGMF) delay and spread the…

Astrophysics · Physics 2009-10-28 Eli Waxman , Paolo Coppi

Distant BL Lacertae objects emit $\gamma$ rays which interact with the extragalactic background light (EBL), creating electron-positron pairs, and reducing the flux measured by ground-based imaging atmospheric Cherenkov telescopes (IACTs)…

High Energy Astrophysical Phenomena · Physics 2015-11-18 Justin D. Finke , Luis C. Reyes , Markos Georganopoulos , Kaeleigh Reynolds , Marco Ajello , Stephen J. Fegan , Kevin McCann

The potential association between Tidal Disruption Events (TDEs) and high-energy astrophysical neutrinos implies the acceleration of cosmic rays. These accelerated particles will initiate electromagnetic (EM) cascades spanning from keV to…

High Energy Astrophysical Phenomena · Physics 2023-10-06 Chengchao Yuan , Walter Winter

Very high energy gamma-rays from blazars traversing cosmological distances through the metagalactic radiation field can convert into electron-positron pairs in photon-photon collisions. The converted gamma-rays initiate electromagnetic…

Astrophysics · Physics 2009-11-13 Tanja M. Kneiske , Karl Mannheim

Be/$\gamma$-ray binaries comprise a confirmed or presumptive pulsar orbiting a Be star and emit luminous $\gamma$-rays. Non-thermal emissions are thought to arise from synchrotron radiation and inverse-Compton (IC) scattering in the shock…

High Energy Astrophysical Phenomena · Physics 2022-02-21 A. M. Chen , J. Takata

The effects of a radiation field (RF) on the unstable modes developed in relativistic electron beam--plasma interaction are investigated assuming that $\omega_{0} >\omega_{p}$, where $\omega_{0}$ is the frequency of the RF and $\omega_{p}$…

Plasma Physics · Physics 2015-06-04 Hrachya B. Nersisyan , Claude Deutsch