activity
19942026
most citedNeutrino oscillation physics with a neutrino factory

294 citations · 1.4k across the 44 of their papers we have counts for

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18 papers · 1 filter

astro-ph2008★ 30 cited

The diverse broad-band light-curves of Swift GRBs reproduced with the cannonball model

Shlomo Dado, Arnon Dar, A. De Rujula

Two radiation mechanisms, inverse Compton scattering (ICS) and synchrotron radiation (SR), suffice within the cannonball (CB) model of long gamma ray bursts (LGRBs) and X-ray flash…

astro-ph2008★ 27 cited

Short Hard Gamma Ray Bursts And Their Afterglows

Shlomo Dado, Arnon Dar

Long duration gamma ray bursts (GRBs) and X-ray flashes (XRFs) are produced by highly- relativistic jets ejected in core-collapse supernova explosions. The origin of short hard gam…

astro-ph2007★ 26 cited

On the origin of the correlations between Gamma-Ray Burst observables

Shlomo Dado, Arnon Dar, A. De Rujula

Several pairs of observable properties of Gamma Ray Bursts (GRBs) are known to be correlated. Many such correlations are straightforward predictions of the 'cannonball' model of GR…

astro-ph2006★ 8 cited

Long gamma-ray bursts without visible supernovae: a case study of redshift estimators and alleged novel objects

Shlomo Dado, Arnon Dar, A. De Rujula +1

It has been argued that the observational limits on a supernova (SN) associated with GRB060614 convincingly exclude a SN akin to SN1998bw as its originator, and provide evidence fo…

astro-ph2005★ 17 cited

On the "canonical behaviour" of the X-ray afterglows of the Gamma Ray Bursts observed with Swift's XRT

Shlomo Dado, Arnon Dar, A. De Rujula

The "canonical behaviour" of the early X-ray afterglows of long-duration Gamma-Ray Bursts (GRBs) --observed by the X-Ray Telescope of the SWIFT satellite-- is precisely the one pre…

astro-ph2004★ 4 cited

A Unified Model of High-Energy Astrophysical phenomena

A. De Rujula

I outline a unified model of high-energy astrophysics, in which the gamma background radiation, cluster "cooling flows", gamma-ray bursts, X-ray flashes and cosmic-ray electrons an…

astro-ph2002★ 17 cited

The supernova associated with GRB 020405

Shlomo Dado, Arnon Dar, Alvaro De Rujula

We use the very simple and successful Cannonball (CB) model of gamma ray bursts (GRBs) and their afterglows (AGs) to analyze the observations of the mildly extinct optical AG of th…

astro-ph2002★ 8 cited

On the X-ray lines in the afterglows of GRBs

Shlomo Dado, Arnon Dar, Alvaro De Rujula

The observation of X-ray lines in the afterglow of GRB 011211 has been reported, and challenged. The lines were interpreted as blue-shifted X-rays characteristic of a set of photoi…

astro-ph2002★ 34 cited

On the radio afterglow of gamma ray bursts

Shlomo Dado, Arnon Dar, A. De Rujula

We use the cannonball (CB) model of gamma ray bursts (GRBs) to predict the spectral and temporal behaviour of their radio afterglows (AGs). A single simple expression describes the…

astro-ph2002★ 26 cited

Is there a 1998bw-like supernova in the afterglow of gamma ray burst 011121?

Shlomo Dado, Arnon Dar, Alvaro De Rujula

We use the very simple and successful Cannonball Model (CB) of gamma ray bursts (GRBs) and their afterglows (AGs) to analyze the observations of the strongly extinct optical AG of…

astro-ph2002

Optical and X-ray Afterglows in the Cannonball Model of GRBs

A. De Rujula

The Cannonball Model is based on the hypothesis that GRBs and their afterglows are made in supernova explosions by relativistic ejecta similar to the ones observed in quasars and m…

astro-ph2001★ 100 cited

On the optical and X-ray afterglows of gamma ray bursts

Shlomo Dado, Arnon Dar, A. De Rujula

We severely criticize the consuetudinary analysis of the afterglows of gamma-ray bursts (GRBs) in the conical-ejection fireball scenarios. We argue that, instead, recent observatio…

astro-ph2000★ 5 cited

The Cannonball Model of Gamma Ray Bursts: Spectral and Temporal Properties of the Gamma Rays

Arnon Dar, Alvaro De Rújula

Recent observations suggest that gamma ray bursts (GRBs) and their afterglows are produced by highly relativistic jets emitted in supernova explosions. We have proposed that the re…

astro-ph2000★ 21 cited

What is the Cosmic-Ray luminosity of our Galaxy?

A. Dar, A. De Rújula

The total cosmic-ray luminosity of the Galaxy is an important constraint on models of cosmic-ray generation. The diffuse high energy -ray and radio-synchrotron emissions of the…

astro-ph2000★ 26 cited

Is the diffuse gamma background radiation generated by galactic cosmic rays?

Arnon Dar, A. De Rújula

We explore the possibility that the diffuse gamma-ray background radiation (GBR) at high galactic latitudes could be dominated by inverse Compton scattering of cosmic ray (CR) elec…

astro-ph1997★ 246 cited

A Matter-Antimatter Universe?

A. G. Cohen, A. De Rujula, S. L. Glashow

We ask whether the universe can be a patchwork consisting of distinct regions of matter and antimatter. We demonstrate that, after recombination, it is impossible to avoid annihila…

astro-ph1997★ 2 cited

Avatars of a Matter-Antimatter Universe

Alvaro De Rujula

An elegantly symmetric Universe, consisting of large islands of matter and antimatter, is by no means obviously out of the question. I review the observations that lead to the usua…

astro-ph1994★ 12 cited

Whither do the microlensing Brown Dwarfs rove?

A. de Rujula, G. Giudice, S. Mollerach +1

The EROS and MACHO collaborations have reported observations of light curves of stars in the Large Magellanic Cloud that are compatible with gravitational microlensing by interveni…