activity
20162020
most citedNeutrino scattering in supernovae and spin correlations of a unitary gas

14 citations · 23 across the 3 of their papers we have counts for

collaborators

7 papers

nucl-th2020

Fast neutrino cooling of nuclear pasta in neutron stars: molecular dynamics simulations

Zidu Lin, Matthew E. Caplan, Charles J. Horowitz +1

The direct URCA process of rapid neutrino emission can occur in nonuniform nuclear pasta phases that are expected in the inner crust of neutron stars. Here, the periodic potential…

nucl-ex2020

Investigating the dependence of collective dynamics on n/p asymmetry for light nuclei

R. T. deSouza, Varinderjit Singh, S. Hudan +2

The dynamics present in the fusion of neutron-rich nuclei is explored through the comparison of experimental cross-sections at above-barrier energies with measurements of the inter…

astro-ph.HE2019

Detectability of SASI activity in supernova neutrino signals

Zidu Lin, Cecilia Lunardini, Michele Zanolin +2

We introduce a novel methodology for establishing the presence of Standing Accretion Shock Instabilities (SASI) in the dynamics of a core collapse supernova from the observed neutr…

astro-ph.HE2019

Observing cosmological binary mergers with next generation neutrino and gravitational wave detectors

Zidu Lin, Cecilia Lunardini

We discuss the potential of detecting thermal neutrinos from matter-rich binary mergers, via a decades-long multi-messenger campaign involving a Mt-scale water Cherenkov neutrino d…

astro-ph.HE20179 cited

Core-Collapse Supernova Simulations including Neutrino Interactions from the Virial EOS

Evan O'Connor, C. J. Horowitz, Zidu Lin +1

Core-collapse supernova explosions are driven by a central engine that converts a small fraction of the gravitational binding energy released during core collapse to outgoing kinet…

astro-ph.HE201714 cited

Neutrino scattering in supernovae and spin correlations of a unitary gas

Zidu Lin, C. J. Horowitz

Core collapse supernova simulations can be sensitive to neutrino interactions near the neutrinosphere. This is the surface of last scattering. We model the neutrinosphere region as…