activity
19962007
most citedIn which shell-type SNRs should we look for gamma-rays and neutrinos from p-p collisions?

98 citations · 208 across the 8 of their papers we have counts for

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Showing 2002 · astro-phShow all

6 papers · 2 filters

astro-ph2002

Stability of an Ultra-Relativistic Blast Wave in an External Medium with a Steep Power-Law Density Profile

Xiaohu Wang, Abraham Loeb, Eli Waxman

We examine the stability of self-similar solutions for an accelerating relativistic blast wave which is generated by a point explosion in an external medium with a steep radial den…

astro-ph2002

High Energy Neutrinos from Gamma-Ray Bursts with Precursor Supernovae

Soebur Razzaque, Peter Meszaros, Eli Waxman

The high energy neutrino signature from proton-proton and photo-meson interactions in a supernova remnant shell ejected prior to a gamma-ray burst provides a test for the precursor…

astro-ph2002

Astrophysical sources of high energy neutrinos

E. Waxman

Several high energy, >100 GeV, neutrino telescopes are currently operating or under construction. Their main motivation is the extension of the horizon of neutrino astronomy to cos…

astro-ph2002

GeV Emission from TeV Blazars and Intergalactic Magnetic Fields

Z. G. Dai, B. Zhang, L. J. Gou +2

Several high-frequency peaked BL Lac objects such as Mrk 501 are strong TeV emitters. However, a significant fraction of the TeV gamma rays emitted are likely to be absorbed in int…

astro-ph20022 cited

TeV Neutrinos from Galactic Microquasar Jets

D. Guetta, C. Distefano, A. Levinson +1

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…

astro-ph20022 cited

Galactic Constraints on the Sources of Ultra-High Energy Cosmic Rays

Abraham Loeb, Eli Waxman

We show that if the sources of ultra-high energy cosmic rays (UHECRs) with energies E>10^{19}eV are associated with galaxies, then the production of UHECRs must occur in transient…