activity
19942026
most citedThe Man Behind the Curtain: X-rays Drive the UV through NIR Variability in the 2013 AGN Outburst in NGC 2617

1.9k citations · 21.8k across the 225 of their papers we have counts for

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Showing 2004Show all

6 papers · 1 filter

astro-ph2004★ 10 cited

APS Neutrino Study: Report of the Neutrino Astrophysics and Cosmology Working Group

Steve W. Barwick, John F. Beacom, Vince Cianciolo +11

In 2002, Ray Davis and Masatoshi Koshiba were awarded the Nobel Prize in Physics ``for pioneering contributions to astrophysics, in particular for the detection of cosmic neutrinos…

physics.acc-ph2004★ 3 cited

The Neutrino Factory and Beta Beam Experiments and Development

C. Albright, V. Barger, J. Beacom +13

The long-term prospects for fully exploring three-flavor mixing in the neutrino sector depend upon an ongoing and increased investment in the appropriate accelerator R&D. Two new c…

astro-ph2004★ 204 cited

Gamma-Ray Constraint on Galactic Positron Production by MeV Dark Matter

John F. Beacom, Nicole F. Bell, Gianfranco Bertone

The Galactic positrons, as observed by their annihilation gamma-ray line at 0.511 MeV, are difficult to account for with astrophysical sources. It has been proposed that they are p…

hep-ph2004★ 57 cited

Shower Power: Isolating the Prompt Atmospheric Neutrino Flux Using Electron Neutrinos

John F. Beacom, Julián Candia

At high energies, the very steep decrease of the conventional atmospheric component of the neutrino spectrum should allow the emergence of even small and isotropic components of th…

astro-ph2004★ 155 cited

Neutrinoless Universe

John F. Beacom, Nicole F. Bell, Scott Dodelson

We consider the consequences for the relic neutrino abundance if extra neutrino interactions are allowed, e.g., the coupling of neutrinos to a light (compared to ) boson. For…

astro-ph2004★ 35 cited

Angular Correlations of the MeV Cosmic Gamma Ray Background

Pengjie Zhang, John F. Beacom

The measured cosmic gamma ray background (CGB) spectrum at MeV energies is in reasonable agreement with the predicted contribution from type Ia supernovae (SNIa). But the character…