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Core-collapse supernovae are found in galaxies with ongoing star-formation. In a starburst galaxy hosting an active galactic nucleus with a relativistic jet, supernovae can take place inside the jet. The collision of the supernova ejecta…

High Energy Astrophysical Phenomena · Physics 2019-02-20 F. L. Vieyro , V. Bosch-Ramon , N. Torres-Albà

Despite their different nature and physics, blazars and gamma-ray bursts have in common very powerful relativistic jets, which make them the most luminous sources in the Universe. The energy extraction from the central compact object, the…

High Energy Astrophysical Phenomena · Physics 2015-12-15 Elena Pian

The radiation observed by blazars is believed to originate from the transformation of bulk kinetic energy of relativistic jets into random energy. A simple way to achieve this is to have an intermittent central power source, producing…

Astrophysics · Physics 2007-05-23 Gabriele Ghisellini

The production rate of compact objects, i.e. neutron stars (NS) and black holes (BH), in active galactic nuclei (AGN) and quasars (QSO), where the frequent supernova explosion is used to explain the high metallicity, is very high due to the…

Astrophysics · Physics 2009-10-31 K. S. Cheng , Jian-Min Wang

Highly relativistic jets from merger and accretion induced collapse of compact stellar objects, which may produce the cosmological gamma ray bursts (GRBs), are also very efficient and powerful cosmic ray accelerators. The expected…

Astrophysics · Physics 2007-05-23 Arnon Dar

Various aspects of the high-energy emission from relativistic jets associated wi th compact astrophysical systems are reviewed. The main leptonic and hadronic processes responsible for the production of high-energy $\gamma$-rays, very-high…

Astrophysics · Physics 2008-11-26 Amir Levinson

The relativistic outflows from gamma-ray bursts are now thought to be narrowly collimated into jets. After correcting for this jet geometry there is a remarkable constancy of both the energy radiated by the burst and the kinetic energy…

Astrophysics · Physics 2009-11-10 D. A. Frail

Recent observations suggest that gamma ray bursts (GRBs) and their afterglows are produced in star formation regions in distant galaxies by highly relativistic jets that happen to point in our direction. Relativistic beaming collimates the…

Astrophysics · Physics 2007-05-23 Arnon Dar

Relativistic jets are one of the most powerful manifestations of the release of energy related to the supermassive black holes at the centre of active galactic nuclei (AGN). Their emission is observed across the entire electromagnetic…

High Energy Astrophysical Phenomena · Physics 2015-04-14 M. Orienti

Gamma-ray bursts are short-lived, luminous explosions at cosmological distances, thought to originate from relativistic jets launched at the deaths of massive stars. They are among the prime candidates to produce the observed cosmic rays at…

High Energy Astrophysical Phenomena · Physics 2015-10-15 Mauricio Bustamante , Philipp Baerwald , Kohta Murase , Walter Winter

Gamma-ray emission from AGN provides us with unprecedented insights into the physics of extragalactic jets. The emission from these jets fits naturally into the existing theoretical framework of relativistic jets as inferred from parsec…

Astrophysics · Physics 2009-11-06 G. V. Bicknell , S. J. Wagner , B. A. Groves

Typical observational gamma-ray burst (GRB) spectra are discussed and, in this connection, what is the origin of the compactness problem and how it was solved at first. If the threshold for $e^{-}e^{+}$ pair production depends on an angle…

Fermi Gamma ray Space Telescope measurements of spectra, variability time scale, and maximum photon energy give lower limits to the apparent jet powers and, through gammagamma opacity arguments, the bulk Lorentz factors of relativistic…

High Energy Astrophysical Phenomena · Physics 2010-12-01 Charles D. Dermer , Soebur Razzaque

We examine the possibility that energetic Standard Model particles contained in the jets produced by active galactic nuclei (AGN) may scatter off of the dark matter halo which is expected to surround the AGN. In particular, if there are…

High Energy Physics - Phenomenology · Physics 2015-05-30 Jinrui Huang , Arvind Rajaraman , Tim M. P. Tait

We point out that the bursts of photons with the energy of the axion mass may appear coincidentally with gamma ray bursts if the gamma ray bursts are caused by collisions between neutron stars and axionic boson stars. In this mechanism,…

High Energy Physics - Phenomenology · Physics 2007-05-23 Aiichi Iwazaki

We believe that the radiation we receive from Gamma-Ray Bursts (GRBs) and radio loud Active Galacti Nuclei (AGNs) originates from the transformation of bulk relativistic motion into random energy. Mechanisms to produce, collimate and…

Astrophysics · Physics 2009-11-10 G. Ghisellini

We present a model in which AGN jets are described by a dense series of plasma blobs, distributed in masses and velocities. The blobs expand and collide, and ultimately form a continuous jet flow as observed on larger scales. When blobs…

High Energy Astrophysical Phenomena · Physics 2010-07-27 Jörg P. Rachen , Max Häberlein , Felix Reimold , Thomas Krichbaum

Gamma-Ray Bursts (GRBs) are extra-galactic and extremely energetic transient emissions of gamma rays, which are thought to be associated with the death of massive stars or the merger of compact objects in binary systems. Their huge…

High Energy Astrophysical Phenomena · Physics 2016-07-20 F. Piron

We discuss the possibility that gamma-ray bursts may result from cosmological relativistic blob emitting neutron star jets that precess past the line of sight. Beaming reduces the energy requirements, so that the jet emission can last…

Astrophysics · Physics 2009-10-28 Eric G. Blackman , Insu Yi , George B. Field

Black holes generate collimated, relativistic jets which have been observed in gamma-ray bursts (GRBs), microquasars, and at the center of some galaxies (active galactic nuclei; AGN). How jet physics scales from stellar black holes in GRBs…

High Energy Astrophysical Phenomena · Physics 2013-01-04 Rodrigo S. Nemmen , Markos Georganopoulos , Sylvain Guiriec , Eileen T. Meyer , Neil Gehrels , Rita M. Sambruna