2.7k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Oak Ridge National LaboratoryUS200 papers
- Los Alamos National LaboratoryUS198 papers
- Duke UniversityUS187 papers
- Triangle Universities Nuclear LaboratoryUS171 papers
- University of Tennessee at KnoxvilleUS134 papers
- University of WashingtonUS134 papers
- University of North Carolina at Chapel HillUS130 papers
- Lawrence Berkeley National LaboratoryUS119 papers
- University of California, BerkeleyUS103 papers
- Centre National de la Recherche ScientifiqueFR98 papers
- Indiana University BloomingtonUS94 papers
- Massachusetts Institute of TechnologyUS93 papers
12 papers · 2 filters
Exploring Properties of Dark and Visible Mass Distribution on Different Scales in the Universe
Yuriy Mishchenko, Chung-Ryong Ji
In this short note we discuss recent observation of linear correlation on log-log scale between distribution of dark and visible mass in gravitationally bound systems. The coeffici…
Neutrino Scattering, Absorption and Annihilation above the accretion disks of Gamma Ray Bursts
J. P. Kneller, G. C. McLaughlin, R. Surman
The central engine that drives gamma ray burst (GRB) explosions may derive from the ability of electrons/positrons and nucleons to tap into the momentum and energy from the large n…
INTEGRAL/SPI Limits on Electron-Positron Annihilation Radiation from the Galactic Plane
B. J. Teegarden, K. Watanabe, P. Jean +24
The center of our Galaxy is a known strong source of electron-positron 511-keV annihilation radiation. Thus far, however, there have been no reliable detections of annihilation rad…
Neutrino Emission from Ungapped Quark Matter
Thomas Schafer, Kai Schwenzer
We study neutrino emission from a normal, ungapped, quark phase in the core of a compact star. Neutrino emission from non-interacting quark matter leads to an emissivity that scale…
A Million-Second Chandra View of Cassiopeia A
Una Hwang, J. Martin Laming, Carles Badenes +20
We introduce a million-second observation of the supernova remnant Cassiopeia A with the Chandra X-ray Observatory. The bipolar structure of the Si-rich ejecta (NE jet and SW count…
Nonlinear Particle Acceleration at Reverse Shocks in Supernova Remnants
Donald C. Ellison, Anne Decourchelle, Jean Ballet
Without amplification, magnetic fields in expanding ejecta of young supernova remnants (SNRs) will be orders of magnitude below those required to shock accelerate thermal electrons…
Diffusive Shock Acceleration in Unmodified Relativistic, Oblique Shocks
Donald C. Ellison, Glen P. Double
We present results from a fully relativistic Monte Carlo simulation of diffusive shock acceleration (DSA) in unmodified shocks. The computer code uses a single algorithmic sequence…
Prospects for obtaining an r-process from Gamma Ray Burst Disk Winds
G. C. McLaughlin, R. Surman
We discuss the possibility that r-process nucleosynthesis may occur in the winds from gamma ray burst accretion disks. This can happen if the temperature of the disk is sufficientl…
Neutrino Interactions in the Outflow from Gamma-Ray Burst Accretion Disks
R. Surman, G. C. McLaughlin
We examine the composition of matter as it flows away from gamma ray burst accretion disks, in order to determine what sort of nucleosynthesis may occur. Since there is a large flu…
BBN For Pedestrians
James P. Kneller, Gary Steigman
The simplest, `standard' model of Big Bang Nucleosynthesis (SBBN) assumes three light neutrinos (N_nu = 3) and no significant electron neutrino asymmetry, leaving only one adjustab…
Magnetic Rayleigh-Taylor instability for Pulsar Wind Nebulae in expanding Supernova Remnants
N. Bucciantini, E. Amato, R. Bandiera +2
We present a numerical investigation of the development of Rayleigh-Taylor instability at the interface between an expanding Pulsar Wind Nebula and its surrounding Supernova Remnan…
The effects of spin-down on the structure and evolution of pulsar wind nebulae
N. Bucciantini, R. Bandiera, J. M. Blondin +2
We present high resolution spherically symmetric relativistic magnetohydrodynamical simulations of the evolution of a pulsar wind nebula inside the free expanding ejecta of the sup…