98 citations · 415 across the 19 of their papers we have counts for
19 papers
Joint Detection and Characterization of the Standing Accretion Shock Instability for Core-Collapse Supernovae with cWB XP
Vicente Sierra, Zidu Lin, Michelle Zanolin +3
The most sensitive to-date multimessenger detection of the standing accretion shock instability in real interferometric data is presented, which quantitatively identifies the prese…
Structure Factors for Hot Neutron Matter from Ab Initio Lattice Simulations with High-Fidelity Chiral Interactions
Yuan-Zhuo Ma, Zidu Lin, Bing-Nan Lu +6
We present the first ab initio lattice calculations of spin and density correlations in hot neutron matter using high-fidelity interactions at next-to-next-to-next-to-leading order…
Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter
Rajesh Kumar, Veronica Dexheimer, Johannes Jahan +57
This review aims at providing an extensive discussion of modern constraints relevant for dense and hot strongly interacting matter. It includes theoretical first-principle results…
Characterizing a supernova's Standing Accretion Shock Instability with neutrinos and gravitational waves
Zidu Lin, Abhinav Rijal, Cecilia Lunardini +2
We perform a novel multi-messenger analysis for the identification and parameter estimation of the Standing Accretion Shock Instability (SASI) in a core collapse supernova with neu…
Uncertainty Quantification for Neutrino Opacities in Core-Collapse Supernovae and Neutron Star Mergers
Zidu Lin, Andrew W. Steiner, Jerome Margueron
We perform an extensive study of the correlations between the neutrino-nucleon inverse mean free paths (IMFPs) and the underlying equation of states (EoSs). Strong interaction unce…
Detectability of neutrino-signal fluctuations induced by the hadron-quark phase transition in failing core-collapse supernovae
Zidu Lin, Shuai Zha, Evan P. O'Connor +1
We introduce a systematic and quantitative methodology for establishing the presence of neutrino oscillatory signals due to the hadron-quark phase transition (PT) in failing core-c…
Memory-triggered supernova neutrino detection
Mainak Mukhopadhyay, Zidu Lin, Cecilia Lunardini
We demonstrate that observations of the gravitational memory from core collapse supernovae at future Deci-Hz interferometers enable time-triggered searches of supernova neutrinos a…
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…
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…
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…
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…
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…
Deep crustal heating by neutrinos from the surface of accreting neutron stars
F. J. Fattoyev, Edward F. Brown, Andrew Cumming +4
We present a new mechanism for deep crustal heating in accreting neutron stars. Charged pions () are produced in nuclear collisions on the neutron star surface during active a…
Disentangling the role of vibration, rotation, and neutron transfer in the fusion of neutron-rich mid-mass nuclei
J. Vadas, Varinderjit Singh, B. B. Wiggins +9
We report the first measurement of the fusion excitation functions for K + Si at near-barrier energies. Evaporation residues resulting from the fusion process were…
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…
Nuclear pasta and supernova neutrinos at late times
C. J. Horowitz, D. K. Berry, M. E. Caplan +5
Nuclear pasta, with nucleons arranged into tubes, sheets, or other complex shapes, is expected in core collapse supernovae (SNe) at just below nuclear density. We calculate the add…
Neutrino-nucleon scattering in supernova matter from the virial expansion
C. J. Horowitz, O. L. Caballero, Zidu Lin +2
We generalize our virial approach to study the neutral current neutrino response of nuclear matter at low densities. In the long-wavelength limit, the virial expansion makes model-…
Effect of topological defects on "nuclear pasta" observables
A. S. Schneider, D. K. Berry, M. E. Caplan +2
[Background] The "pasta" phase of nuclear matter may play an important role in the structure and evolution of neutron stars. Recent works suggest nuclear pasta has a high resistivi…
The full weak charge density distribution of 48Ca from parity violating electron scattering
Z. Lin, C. J. Horowitz
Background: The ground state neutron density of a medium mass nucleus contains fundamental nuclear structure information and is at present relatively poorly known. Purpose: We expl…