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20022026
most citedQuantum ESPRESSO: a modular and open-source software project for quantum simulations of materials

29.3k citations

Showing 2021Show all

229 papers · 1 filter

hep-ex20211 cited

Search for the decay

Belle Collaboration, B. Bhuyan, K. J. Nath +184

We report results from a search for the decay using 121.4 fb of data collected at the resonance with the Belle detector at the KEKB asymmetric-e…

cond-mat.str-el20214 cited

Quantum Monte Carlo simulations of highly frustrated magnets in a cluster basis: The two-dimensional Shastry-Sutherland model

Andreas Honecker, Lukas Weber, Philippe Corboz +2

Quantum Monte Carlo (QMC) simulations constitute nowadays one of the most powerful methods to study strongly correlated quantum systems, provided that no "sign problem" arises. How…

astro-ph.IM202110 cited

New Periodograms Separating Orbital Radial Velocities and Spectral Shape Variation

Avraham Binnenfeld, Sahar Shahaf, Richard I. Anderson +1

We present new periodograms that are effective in distinguishing Doppler shift from spectral shape variability in astronomical spectra. These periodograms, building upon the concep…

quant-ph2021

Neural-Network Quantum States for Periodic Systems in Continuous Space

Gabriel Pescia, Jiequn Han, Alessandro Lovato +2

We introduce a family of neural quantum states for the simulation of strongly interacting systems in the presence of spatial periodicity. Our variational state is parameterized in…

astro-ph.GA202122 cited

The Pristine survey -- XV. A CFHT ESPaDOnS view on the Milky Way halo and disc populations

R. Lucchesi, C. Lardo, P. Jablonka +14

We present a one-dimensional, local thermodynamic equilibrium (1D-LTE) homogeneous analysis of 132 stars observed at high-resolution with ESPaDOnS. This represents the largest samp…

astro-ph.GA202112 cited

On the dynamical evolution of Cepheids in star clusters

František Dinnbier, Richard I. Anderson, Pavel Kroupa

We investigate the occurrence of classical (type-I) Cepheid variable stars (henceforth: Cepheids) in dynamically evolving star clusters from birth to an age of approximately 300 My…