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23 papers · 1 filter
Formation of Galactic Bulges
Nickolay Y. Gnedin, Michael L. Norman, Jeremiah P. Ostriker
We use cosmological hydrodynamic simulations to investigate formation of galactic bulges within the framework of hierarchical clustering in a representative CDM cosmological model.…
Numerical Models of Binary Neutron Star System Mergers. I.: Numerical Methods and Equilibrium Data for Newtonian Models
F. Douglas Swesty, Edward Y. M. Wang, Alan C. Calder
The numerical modeling of binary neutron star mergers has become a subject of much interest in recent years. While a full and accurate model of this phenomenon would require the ev…
R-Mode Oscillations in Rotating Magnetic Neutron Stars
Luciano Rezzolla, Frederick K. Lamb, Stuart L. Shapiro
We show that r-mode oscillations distort the magnetic fields of neutron stars and that their occurrence is likely to be limited by this interaction. If the field is gtrsim 10^{16}…
The Debye-Waller Factor in solid 3He and 4He
E. W. Draeger, D. M. Ceperley
The Debye-Waller factor and the mean-squared displacement from lattice sites for solid 3He and 4He were calculated with Path Integral Monte Carlo at temperatures between 5 K and 35…
Characterization of the State of Hydrogen
Burkhard Militzer, William Magro, David Ceperley
Fermionic path integral Monte Carlo simulations have been applied to study the equilibrium properties of the hydrogen and deuterium in the density and temperature range of 1.6 < rs…
Path Integral Monte Carlo Simulations for Fermion Systems: Pairing in the Electron-Hole Plasma
J. Shumway, D. M. Ceperley
We review the path integral method wherein quantum systems are mapped with Feynman's path integrals onto a classical system of "ring-polymers" and then simulated with the Monte Car…