Zidu Lin
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View article: Voltage faults diagnosis for lithium-ion batteries in electric vehicles using optimized graphical neural network
Voltage faults diagnosis for lithium-ion batteries in electric vehicles using optimized graphical neural network Open
Diagnosing voltage faults of lithium-ion batteries is a critical function in the battery management system. Accurate diagnosis of voltage faults is crucial for ensuring the safety and reliability of energy storage applications and electric…
View article: Recurring region for neutron-star observables
Recurring region for neutron-star observables Open
In this letter, we report a new phenomena of recurring regions when relating observables for hybrid neutron stars and hybrid neutron-star mergers. To describe dense matter within hybrid stars, we introduce a percolation to vary the size an…
View article: Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis
Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Open
The potential hadron-to-quark phase transition in neutron stars has not been fully understood as the property of cold, dense, and strongly interacting matter cannot be theoretically described by the first-principle perturbative calculation…
View article: Indication of Sharp and Strong Phase Transitions from NICER Observations
Indication of Sharp and Strong Phase Transitions from NICER Observations Open
In this Letter, we present a new, weakly model-dependent test for “standard” equation-of-state (EoS) models that disfavor sharp and strong phase transitions by using NS mass and radius observations. We show the radii of two NSs observed by…
View article: Theoretical and experimental constraints for the equation of state of dense and hot matter
Theoretical and experimental constraints for the equation of state of dense and hot matter Open
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 from lattice and perturbative QCD, as well as chiral effect…
View article: Structure Factors for Hot Neutron Matter from <i>Ab Initio</i> Lattice Simulations with High-Fidelity Chiral Interactions
Structure Factors for Hot Neutron Matter from <i>Ab Initio</i> Lattice Simulations with High-Fidelity Chiral Interactions Open
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 in chiral effective field theory. These correlations have …
View article: Detectability of neutrino-signal fluctuations induced by the hadron-quark phase transition in failing core-collapse supernovae
Detectability of neutrino-signal fluctuations induced by the hadron-quark phase transition in failing core-collapse supernovae Open
Here 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-collapse supernovae from the observed neutrino event ra…
View article: Indication of Sharp and Strong Phase-Transitions from NICER Observations
Indication of Sharp and Strong Phase-Transitions from NICER Observations Open
In this letter, we present a new, weakly model-dependent, test for ``standard" equations of state (EoS) models that disfavor sharp and strong phase-transitions, by using neutron star mass and radius observations. We show the radii of two n…
View article: Structure Factors for Hot Neutron Matter from Ab Initio Lattice Simulations with High-Fidelity Chiral Interactions
Structure Factors for Hot Neutron Matter from Ab Initio Lattice Simulations with High-Fidelity Chiral Interactions Open
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 (N3LO) in chiral effective field theory. These correlation…
View article: Characterizing a supernova’s standing accretion shock instability with neutrinos and gravitational waves
Characterizing a supernova’s standing accretion shock instability with neutrinos and gravitational waves Open
Here, 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 neutrino and gravitational wave (GW) signals. In the neu…
View article: Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter
Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter Open
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 from lattice and perturbative QCD, as well as chiral effect…
View article: Uncertainty quantification for neutrino opacities in core-collapse supernovae and neutron star mergers
Uncertainty quantification for neutrino opacities in core-collapse supernovae and neutron star mergers Open
We perform an extensive study of the correlations between the\nneutrino-nucleon inverse mean free paths (IMFPs) and the underlying equation of\nstates (EoSs). Strong interaction uncertainties in the neutrino mean free path\nare investigate…
View article: Characterizing a supernova's Standing Accretion Shock Instability with neutrinos and gravitational waves
Characterizing a supernova's Standing Accretion Shock Instability with neutrinos and gravitational waves Open
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 neutrino and gravitational wave (GW) signals. In the neutrino …
View article: Memory-triggered supernova neutrino detection
Memory-triggered supernova neutrino detection Open
When a burst of neutrinos from a core-collapse supernova (CCSN) passes by the Earth, it causes a permanent change in the local space-time metric, called the gravitational wave (GW) memory. Long considered unobservable, this effect will be …
View article: Detectability of neutrino-signal fluctuations induced by the hadron-quark phase transition in failing core-collapse supernovae
Detectability of neutrino-signal fluctuations induced by the hadron-quark phase transition in failing core-collapse supernovae Open
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-collapse supernovae from the observed neutrino event rate in…
View article: Fast neutrino cooling of nuclear pasta in neutron stars: Molecular dynamics simulations
Fast neutrino cooling of nuclear pasta in neutron stars: Molecular dynamics simulations Open
The direct Urca process of rapid neutrino emission can occur in nonuniform nuclear pasta phases that are expected in the inner crusts of neutron stars. Here, the periodic potential for a nucleon in nuclear pasta allows momentum conservatio…
View article: Extracting dynamics in the fusion of neutron-rich light nuclei
Extracting dynamics in the fusion of neutron-rich light nuclei Open
The dependence of fusion dynamics on neutron excess for light nuclei is extracted. This is accomplished by comparing the average fusion cross-section at energies just above the fusion barrier for $^{12-15}$C + $^{12}$C with measurements of…
View article: Detectability of standing accretion shock instabilities activity in supernova neutrino signals
Detectability of standing accretion shock instabilities activity in supernova neutrino signals Open
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 neutrino event rate at water- or ice- based neutrino detectors. …
View article: Enhanced dynamics in fusion of neutron-rich oxygen nuclei at above-barrier energies
Enhanced dynamics in fusion of neutron-rich oxygen nuclei at above-barrier energies Open
Above-barrier fusion cross-sections for an isotopic chain of oxygen isotopes with A=16-19 incident on a 12C target are presented. Experimental data are compared with both static and dynamical microscopic calculations. These calculations ar…
View article: Investigating the dependence of collective dynamics on n/p asymmetry for light nuclei
Investigating the dependence of collective dynamics on n/p asymmetry for light nuclei Open
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 interaction cross-section at relativistic energies. The increase…
View article: Observing cosmological binary mergers with next generation neutrino and gravitational wave detectors
Observing cosmological binary mergers with next generation neutrino and gravitational wave detectors Open
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 detector and one or more next generation gravitational wave …
View article: Deep crustal heating by neutrinos from the surface of accreting neutron stars
Deep crustal heating by neutrinos from the surface of accreting neutron stars Open
Here, we present a new mechanism for deep crustal heating in accreting neutron stars. Charged pions (π+) are produced in nuclear collisions on the neutron star surface during active accretion and upon decay they provide a flux of neutrinos…
View article: Probing the fusion of neutron-rich nuclei with re-accelerated radioactive beams
Probing the fusion of neutron-rich nuclei with re-accelerated radioactive beams Open
Here, we report the first measurement of the fusion excitation functions for 39,47K + 28Si at near-barrier energies. Evaporation residues resulting from the fusion process were identified by direct measurement of their energy and time-of-f…
View article: Neutrino scattering in supernovae and the universal spin correlations of a unitary gas
Neutrino scattering in supernovae and the universal spin correlations of a unitary gas Open
Core collapse supernova simulations can be sensitive to neutrino interactions\nnear the neutrinosphere. This is the surface of last scattering. We model the\nneutrinosphere region as a warm unitary gas of neutrons. A unitary gas is a low\n…
View article: Neutrino scattering in supernovae and spin correlations of a unitary gas
Neutrino scattering in supernovae and spin correlations of a unitary gas Open
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 a warm unitary gas of neutrons. A unitary gas is a low den…
View article: Core-Collapse Supernova Simulations including Neutrino Interactions from the Virial EOS
Core-Collapse Supernova Simulations including Neutrino Interactions from the Virial EOS Open
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 kinetic energy. The suspected mode for this energy conversion is…
View article: Neutrino-nucleon scattering in supernova matter from the virial expansion
Neutrino-nucleon scattering in supernova matter from the virial expansion Open
We generalize our virial approach to study the neutral current neutrino\nresponse of nuclear matter at low densities. In the long-wavelength limit, the\nvirial expansion makes model-independent predictions for neutrino-nucleon\nscattering …
View article: Fusion of neutron-rich oxygen nuclei
Fusion of neutron-rich oxygen nuclei Open
\nMeasurement of the fusion excitation function for 18O + 12C and 19O + 12C is described. The fusion cross-section is extracted through the direct measurement of evaporation residues resulting from the fusion process. At near barrier energ…
View article: Fusion enhancement at near and sub-barrier energies in 19O + 12C
Fusion enhancement at near and sub-barrier energies in 19O + 12C Open
Measuring the fusion excitation function for an isotopic chain of projectile nuclei provides a stringent test of a microscopic description of fusion. We report the first measurement of the fusion excitation function at near-barrier energie…