activity
19982023
most citedMeasuring Flavor Ratios of High-Energy Astrophysical Neutrinos

231 citations · 5.3k across the 87 of their papers we have counts for

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9 papers · 1 filter

astro-ph2008★ 40 cited

Gamma-ray Constraints on Dark Matter Annihilation into Charged Particles

Nicole F. Bell, Thomas D. Jacques

Dark matter annihilation into charged particles is necessarily accompanied by gamma rays, produced via radiative corrections. Internal bremsstrahlung from the final state particles…

astro-ph2008★ 83 cited

Conservative Constraints on Dark Matter Annihilation into Gamma Rays

Gregory D. Mack, Thomas D. Jacques, John F. Beacom +2

Using gamma-ray data from observations of the Milky Way, Andromeda (M31), and the cosmic background, we calculate conservative upper limits on the dark matter self-annihilation cro…

astro-ph2006★ 151 cited

Upper Bound on the Dark Matter Total Annihilation Cross Section

John F. Beacom, Nicole F. Bell, Gregory D. Mack

We consider dark matter annihilation into Standard Model particles and show that the least detectable final states, namely neutrinos, define an upper bound on the total cross secti…

astro-ph2005★ 118 cited

Cosmological Signatures of Interacting Neutrinos

Nicole F. Bell, Elena Pierpaoli, Kris Sigurdson

We investigate signatures of neutrino scattering in the Cosmic Microwave Background (CMB) and matter power spectra, and the extent to which present cosmological data can distinguis…

astro-ph2004★ 82 cited

Cosmological Lepton Asymmetry, Primordial Nucleosynthesis, and Sterile Neutrinos

Kevork Abazajian, Nicole F. Bell, George M. Fuller +1

We study post weak decoupling coherent active-sterile and active-active matter-enhanced neutrino flavor transformation in the early universe. We show that flavor conversion efficie…

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…