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9 papers · 2 filters
3D deflagration simulations leaving bound remnants: a model for 2002cx-like Type Ia supernovae
M. Kromer, M. Fink, V. Stanishev +10
2002cx-like supernovae are a sub-class of sub-luminous Type Ia supernovae. Their light curves and spectra are characterized by distinct features that indicate strong mixing of the…
A Search for Point Sources of EeV Neutrons
The Pierre Auger Collaboration
A thorough search of the sky exposed at the Pierre Auger Cosmic Ray Observatory reveals no statistically significant excess of events in any small solid angle that would be indicat…
The impact of kinetic effects on the properties of relativistic electron-positron shocks
A. Stockem, F. Fiuza, R. A. Fonseca +1
We assess the impact of non-thermally shock-accelerated particles on the magnetohydrodynamic (MHD) jump conditions of relativistic shocks. The adiabatic constant is calculated dire…
An Alternative Numerical Method for the Stationary Pulsar Magnetosphere
Yohsuke Takamori, Hirotada Okawa, Makoto Takamoto +1
Stationary pulsar magnetospheres in the force-free system are governed by the pulsar equation. In 1999, Contopoulos, Kazanas, and Fendt (hereafter CKF) numerically solved the pulsa…
Acceleration in perpendicular relativistic shocks for plasmas consisting of leptons and hadrons
A. Stockem, F. Fiuza, R. A. Fonseca +1
We investigate the acceleration of light particles in perpendicular shocks for plasmas consisting of a mixture of leptonic and hadronic particles. Starting from the full set of con…
Effects of post-Newtonian Spin Alignment on the Distribution of Black-Hole Recoils
Emanuele Berti, Michael Kesden, Ulrich Sperhake
Recent numerical relativity simulations have shown that the final black hole produced in a binary merger can recoil with a velocity as large as 5,000 km/s. Because of enhanced grav…