tipa -- 3/15/2012

A New Monte Carlo Method for Time-Dependent Neutrino Radiation Transport

Linking Type Ia Supernova Progenitors and their Resulting Explosions

Direct Numerical Simulation of Radiation Pressure-Driven Turbulence and Winds in Star Clusters and Galactic Disks

Evidence of nuclear disks in starburst galaxies from their radial distribution of supernovae

Reconnection Studies Under Different Types of Turbulence Driving

Turbulence and Radio Mini-halos in the Sloshing Cores of Galaxy Clusters

Investigating stellar-mass black hole kicks

Turbulent Magnetic Field Amplification from Spiral SASI Modes: Implications for Core-Collapse Supernovae and Proto-Neutron Star Magnetization

Electroweak Baryogenesis and Higgs Signatures

Excluding Electroweak Baryogenesis in the MSSM

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