Accurate knowledge of the properties of hydrogen at high compression is crucial for astrophysics (eg, planetary and stellar interiors, brown dwarfs, atmosphere of compact stars) …
We present quasi-exact ab initio path integral Monte Carlo (PIMC) results for the partial static density responses and local field factors of hydrogen in the warm dense matter regime, from …
The finite temperature version of the Vashishta-Singwi (VS) dielectric scheme for the paramagnetic warm dense uniform electron fluid is revisited correcting for an earlier …
We present extensive new ab initio path integral Monte Carlo (PIMC) results for a variety of structural properties of warm dense hydrogen and beryllium. To deal with the fermion sign …
The study of matter at extreme densities and temperatures has emerged as a highly active frontier at the interface of plasma physics, material science and quantum chemistry with …
We carry out highly accurate\emph {ab initio} path integral Monte Carlo (PIMC) simulations to directly estimate the free energy of various warm dense matter systems including the …
Accurate knowledge of the properties of hydrogen at high compression is crucial for astrophysics (eg planetary and stellar interiors, brown dwarfs, atmosphere of compact stars) …
We compute the energy per particle of normal liquid ${}^ 3$ He in the temperature range $0.15-2$ K using Path Integral Monte Carlo simulations, leveraging a recently proposed …
Y Xiong, S Liu, H Xiong - Physical Review E, 2024 - APS
Recently, fictitious identical particles have provided a promising way to overcome the fermion sign problem and have been used in path integral Monte Carlo to accurately …