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Related papers: A pair plasma model for PKS 0208-512

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Annihilation of light dark matter of $m_{\rm DM} \approx (10-40)$ GeV into the Standard Model fermions has been suggested as a possible origin of the gamma-ray excess at GeV energies in the Fermi-LAT data. In this paper, we examine possible…

High Energy Physics - Phenomenology · Physics 2015-06-19 Kyoungchul Kong , Jong-Chul Park

We consider vacuum polarization effects in the one-photon annihilation channel within a kinetic description of the e+ e- plasma produced from the vacuum in the focal spot of counter-propagating laser beams. This entails essential changes in…

Plasma Physics · Physics 2010-12-03 S. A. Smolyansky , D. B. Blaschke , A. V. Chertilin , G. Roepke , A. V. Tarakanov

There is convincing observational evidence for an increasing cosmic-ray positron-to-electron ratio at energies larger than $\sim 10$~GeV, at odds with expectations from secondary positron production. The most recent AMS-02 data exhibit an…

High Energy Physics - Phenomenology · Physics 2019-03-21 Stefano Profumo , Farinaldo Queiroz , Clarissa Siqueira

The ionizing fluxes from quasars and other active galactic nuclei (AGN) are critical for interpreting the emission-line spectra of AGN and for photoionization and heating of the intergalactic medium. Using ultraviolet spectra from the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 J. Michael Shull , Matthew Stevans , Charles W. Danforth

A highly intense femtosecond laser pulse incident on a plasma target of supercritical density, gives rise to reflected high-order harmonics of the laser frequency. The radiation model adopted here considers Brunel electrons -those…

Plasma Physics · Physics 2015-06-19 R. Ondarza-Rovira , T. J. M. Boyd

The excesses in the electron and positron spectra observed by many experiments, such as PAMELA and AMS-02, have sparked significant theoretical investigation. It is not easy to distinguish the two primary hypotheses dark matter…

High Energy Astrophysical Phenomena · Physics 2024-11-07 Xing-Jian Lv , Xiao-Jun Bi , Kun Fang , Peng-Fei Yin , Meng-Jie Zhao

We report a detailed analysis of $\gamma$-ray data of 2FGL J0509.9+1802 observed by the Large Area Telescope on board {\it Fermi} satellite, especially focusing on April 2013 when extraordinary $\gamma$-ray variability has been detected.…

High Energy Astrophysical Phenomena · Physics 2015-06-22 N. H. Liao , J. M Bai

In gamma-ray binaries such as LS 5039 a large number of electron-positron pairs are created by the annihilation of primary very high energy (VHE) gamma-rays with photons from the massive star. The radiation from these particles contributes…

High Energy Astrophysical Phenomena · Physics 2017-04-12 Benoit Cerutti , Guillaume Dubus , Gilles Henri

Context. The origin of blazar variability, seen from radio up to gamma rays, is still a heavily debated matter and broadband flares offer a unique testbed towards a better understanding of these extreme objects. Such an energetic outburst…

High Energy Astrophysical Phenomena · Physics 2016-05-11 V. Karamanavis , L. Fuhrmann , E. Angelakis , I. Nestoras , I. Myserlis , T. P. Krichbaum , J. A. Zensus , H. Ungerechts , A. Sievers , M. A. Gurwell

A combined interpretation of the CALET $e^+\, +\, e^-$ spectrum up to 3 TeV and the AMS-02 positron spectrum up to 500 GeV was performed and the results are discussed. To parametrize the background electron flux, we assume a smoothly broken…

High Energy Astrophysical Phenomena · Physics 2018-10-23 S. Bhattacharyya , H. Motz , Y. Asaoka , S. Torii

The interaction of TeV photons from blazars with the extragalactic background light produces a relativistic beam of electron-positron pairs streaming through the intergalactic medium (IGM). The fate of the beam energy is uncertain. By means…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Lorenzo Sironi , Dimitrios Giannios

In the following work, we compute the positron production from branon dark matter annihilations in order to constrain extra-dimensional theories. By having assumed that the positron fraction measured by AMS-02 is well explained just with…

High Energy Physics - Phenomenology · Physics 2019-02-13 Jose A. R. Cembranos , Alvaro de la Cruz-Dombriz , Peter K. S. Dunsby , Miguel Mendez-Isla

Millisecond pulsars (MSPs) are prolific GeV $\gamma\text{-ray}$ emitters, and nearly 80\% of Fermi-LAT MSPs reside in compact binaries. We demonstrate that the companions in these compact MSPs binaries are also 511 keV annihilation line…

High Energy Astrophysical Phenomena · Physics 2025-09-05 Zachary Metzler , Zorawar Wadiasingh

The origin of the multiwavelength emission from PKS 0502+049 neighboring the first cosmic neutrino source TXS 0506+056 is studied using the data observed by Fermi-LAT and Swift UVOT/XRT. This source was in a flaring state in the considered…

High Energy Astrophysical Phenomena · Physics 2019-02-13 N. Sahakyan

Here we present a new approach for constraining luminous blazars, incorporating fully time-dependent and self-consistent modeling of bright gamma-ray flares of PKS1510-089 resolved with Fermi-LAT, in the framework of the internal shock…

High Energy Astrophysical Phenomena · Physics 2015-09-09 Shinya Saito , Lukasz Stawarz , Yasuyuki Tanaka , Tadayuki Takahashi , Marek Sikora , Rafal Moderski

Observations of cosmic rays are a sensitive probe of dark matter annihilation in our Galaxy. In this article we present an analysis of the AMS-02 antiproton data, reducing cosmic-ray propagation uncertainties by fitting at the same time…

High Energy Astrophysical Phenomena · Physics 2018-04-23 Alessandro Cuoco , Jan Heisig , Michael Korsmeier , Michael Krämer

A sophisticated analysis of EGRET data has found evidence for gamma-ray emission from the galactic halo. I entertain the possibility that part of the EGRET signal is due to WIMP annihilations in the halo. I show that a viable candidate with…

Astrophysics · Physics 2007-05-23 Paolo Gondolo

We investigate a magnetized plasma in which injected high energy gamma-rays annihilate on a soft photon field, that is provided by the synchrotron radiation of the created pairs. For a very wide range of magnetic fields, this process…

Astrophysics · Physics 2010-11-11 L. Stawarz , J. G. Kirk

We aim at analyzing the (sub-)millimeter emission in a nearby blazar, PKS 0521-365 , to study the synchrotron and thermal emission in the different components detected at low frequency. We analyze the archive public data of the ALMA Cycle 0…

Astrophysics of Galaxies · Physics 2016-02-03 S. Leon , P. C. Cortes , M. Guerard , E. Villard , T. Hidayat , B. Ocana Flaquer , B. Vila-Vilaro

GRS 1758-258 and 1E 1740.7-2942 are two long-known persistent black hole binaries in the Galactic Center region. Using INTEGRAL's extensive monitoring of the Galactic Center and Bulge, we studied their temporal and spectral evolutions in…

High Energy Astrophysical Phenomena · Physics 2025-02-25 James Rodi , Angela Bazzano , Pietro Ubertini
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