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Related papers: Probing Micro-quasars with TeV Neutrinos

200 papers

We discuss the possibility that microquasar jets may be powerful emitters of TeV neutrinos. We estimate the neutrino fluxes produced by photopion production in the jets of a sample of identified microquasars and microquasar candidates, for…

Astrophysics · Physics 2007-05-23 D. Guetta , C. Distefano , A. Levinson , E. Waxman

It has been proposed recently that Galactic microquasars may be prodigious emitters of TeV neutrinos that can be detected by upcoming km^2 neutrino telescopes. In this paper we consider a sample of identified microquasars and microquasar…

Astrophysics · Physics 2009-11-07 C. Distefano , D. Guetta , E. Waxman , A. Levinson

We consider a compact binary system in which a Wolf-Rayet star supplies matter onto a stellar mass black hole or a neutron star. This matter forms an accretion disk which ejects a jet as observed in Galactic microquasars. A part of the jet…

Astrophysics · Physics 2009-11-11 W. Bednarek

Recent discovery of the afterglow emission from short gamma-ray bursts suggests that binary neutron star or black hole-neutron star binary mergers are the likely progenitors of these short bursts. The accretion of neutron star material and…

Astrophysics · Physics 2011-02-11 Soebur Razzaque , Peter Meszaros

Core collapse of massive stars resulting in a relativistic fireball jet which breaks through the stellar envelope is a widely discussed scenario for gamma-ray burst production. For very extended or slow rotating stars, the fireball may be…

Astrophysics · Physics 2014-10-13 P. Meszaros , E. Waxman

The recent detections of microquasars at energies above a few hundred keV up to the TeV in one case has stimulated a strong interest and raised several questions. How are the MeV, GeV, and even TeV emissions, produced? What are the emission…

High Energy Astrophysical Phenomena · Physics 2017-02-07 Jérôme Rodriguez

Three independent predictions follow from postulating the existence of protons co-accelerated with electrons in extragalactic jets (i) multi-TeV gamma ray emission from nearby blazars, (ii) extragalactic cosmic ray protons up to 10^20 eV,…

Astrophysics · Physics 2009-10-31 Karl Mannheim

To some extent, all Galactic binary systems hosting a compact object are potential `microquasars', so much as all galactic nuclei may have been quasars, once upon a time. The necessary ingredients for a compact object of stellar mass to…

High Energy Astrophysical Phenomena · Physics 2014-11-20 E. Gallo

Neutrinos at energies above TeV can serve as probes of the stellar progenitor and jet dynamics of gamma ray bursts arising from stellar core collapses. They can also probe collapses which do not lead to gamma-rays, which may be much more…

Astrophysics · Physics 2009-11-07 Soebur Razzaque , Peter Meszaros , Eli Waxman

It's generally believed that young and rapidly rotating pulsars are important sites of particle's acceleration, in which protons can be accelerated to relativistic energy above the polar cap region if the magnetic moment is antiparallel to…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Zhi-Xiong Li , Gui-Fang Lin , Wei-Wei Na

We discuss the properties of magnetically dominated jet-like outflows from stellar mass black holes surrounded by debris tori resulting from neutron star disruption. These jets may have narrow cores (along the rotation axis) which are…

Astrophysics · Physics 2015-06-24 P. Meszaros , M. J. Rees

Microquasars are X-ray binaries with relativistic jets. These jets are powerful energy carriers, thought to be fed by accretion, which produce non-thermal emission at different energy bands. To date, several Galactic sources showing…

Astrophysics · Physics 2009-07-23 Valenti Bosch-Ramon , Dmitry Khangulyan

Microquasars, compact binary systems with an accreting stellar-mass black hole or neutron star, are promising candidates for high-energy particle acceleration. Recently, the LHAASO collaboration reported on the detection of $>100$ TeV…

High Energy Astrophysical Phenomena · Physics 2026-01-21 Jose Carpio , Ali Kheirandish , Bing Zhang

Recently, microquasar jets have aroused the interest of many researchers focusing on the astrophysical plasma outflows and various jet ejections. In this work, we concentrate on the investigation of electromagnetic radiation and particle…

High Energy Physics - Phenomenology · Physics 2021-11-02 Th. V. Papavasileiou , O. T. Kosmas , J. Sinatkas

Black holes of stellar mass and neutron stars in binary systems are first detected as hard X-ray sources using high-energy space telescopes. Relativistic jets in some of these compact sources are found by means of multiwavelength…

Astrophysics · Physics 2009-10-31 I. Felix Mirabel , Luis F. Rodriguez

A fraction of core collapse supernovae of type Ib/c are associated with Gamma-ray bursts, which are thought to produce highly relativistic jets. Recently, it has been hypothesized that a larger fraction of core collapse supernovae produce…

Astrophysics · Physics 2009-11-10 Soebur Razzaque , Peter Meszaros , Eli Waxman

Jets associated with Active Galactic Nuclei (AGN) have been observed for almost a century, initially at optical and radio wavelengths. They are now widely accepted as "exhausts" produced electromagnetically by the central, spinning, massive…

High Energy Astrophysical Phenomena · Physics 2015-11-25 R. Blandford , W. East , K. Nalewajko , Y. Yuan , J. Zrake

Relativistic black-hole jet sources are leading candidates for high energy (>> TeV) neutrino production. The relations defining (a) efficient photopion losses of cosmic-ray protons on target photons and (b) gamma-gamma opacity of gamma rays…

Astrophysics · Physics 2009-11-13 C. Dermer , E. Ramirez-Ruiz , T. Le

The source of extragalactic neutrinos in the TeV-PeV range is a matter of very active research, with blazar jets having been postulated to be the origin of at least some of the detections. The blazar PKS 0735+178 is a prominent example;…

High Energy Astrophysical Phenomena · Physics 2025-08-06 G. F. Paraschos , E. Traianou , L. C. Debbrecht , I. Liodakis , E. Ros

We explored the expected properties of the neutrino emission from accreting neutron stars in X-ray binaries using numerical simulations. The simulations are based on a model in which neutrinos are produced by the decay of charged pions and…

High Energy Astrophysical Phenomena · Physics 2025-08-15 L. Ducci , E. Perinati , P. Romano , S. Vercellone , M. Nikołajuk , A. Santangelo , M. Sasaki
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