output
20022026
most citedThe density-matrix renormalization group in the age of matrix product states

4.2k citations

Showing 2017 · astro-ph.HEShow all

7 papers · 2 filters

astro-ph.HE2017556 cited

GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations

David Radice, Albino Perego, Francesco Zappa +1

Gravitational waves detected from the binary neutron star (NS) merger GW170817 constrained the NS equation of state by placing an upper bound on certain parameters describing the b…

astro-ph.HE2017256 cited

AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817

Albino Perego, David Radice, Sebastiano Bernuzzi

The detection of a kilo/macronova electromagnetic counterpart (AT2017gfo) of the first gravitational wave signal compatible with the merger of two neutron stars (GW170817) has conf…

astro-ph.HE2017477 cited

Modeling GW170817 based on numerical relativity and its implications

Masaru Shibata, Sho Fujibayashi, Kenta Hotokezaka +4

Gravitational-wave observation together with a large number of electromagnetic observations shows that the source of the latest gravitational-wave event, GW170817, detected primari…

astro-ph.HE201735 cited

Probing motion of fast radio burst sources by timing strongly lensed repeaters

Liang Dai, Wenbin Lu

Given the possible repetitive nature of fast radio bursts (FRBs), their cosmological origin, and their high occurrence, detection of strongly lensed sources due to intervening gala…

astro-ph.HE2017151 cited

General-Relativistic Large-Eddy Simulations of Binary Neutron Star Mergers

David Radice

The flow inside remnants of binary neutron star (NS) mergers is expected to be turbulent, because of magnetohydrodynamics instability activated at scales too small to be resolved i…

astro-ph.HE201717 cited

Radial Transport and Meridional Circulation in Accretion Disks

Alexander A. Philippov, Roman R. Rafikov

Radial transport of particles, elements and fluid driven by internal stresses in three-dimensional (3D) astrophysical accretion disks is an important phenomenon, potentially releva…