86 citations · 128 across the 9 of their papers we have counts for
9 papers
Beyond Constant Error: Heteroscedastic Bayesian Model Combination for Modeling Unmeasured Nuclei
B. Knight, S. Lalit, P. Giuliani +4
Experimentally inaccessible regions of the nuclear chart remain a challenge for global models of atomic nuclei to predict. This includes exotic nuclei near particle drip lines, sup…
Finite-range pairing in nuclear density functional theory
Sudhanva Lalit, Paul-Gerhard Reinhard, Kyle Godbey +1
Pairing correlations are ubiquitous in low-energy states of atomic nuclei. To incorporate them within nuclear density functional theory, often used for global computations of nucle…
The mass of Sn and Bayesian extrapolations to the proton drip line
Christian M. Ireland, Georg Bollen, Scott E. Campbell +23
The favorable energy configurations of nuclei at magic numbers of neutrons and protons are fundamental for understanding the evolution of nuclear structure. The ${Z=50}…
The nucleardatapy toolkit for simple access to experimental nuclear data, astrophysical observations, and theoretical predictions
Jérôme Margueron, Christian Drischler, Mariana Dutra +10
Systematic comparisons across theoretical predictions for the properties of dense matter, nuclear physics data, and astrophysical observations (also called meta-analyses) are perfo…
Star Log-extended eMulation: a method for efficient computation of the Tolman-Oppenheimer-Volkoff equations
Sudhanva Lalit, Alexandra C. Semposki, Joshua M. Maldonado
We emulate the Tolman-Oppenheimer-Volkoff (TOV) equations, including tidal deformability, for neutron stars using a new method based upon the Dynamic Mode Decomposition (DMD). This…
Crust Cooling Models are Insensitive to the Crust-Core Transition Pressure for Realistic Equations of State
Sudhanva Lalit, Zach Meisel, Edward F. Brown
Neutron stars cooling after sustained accretion outbursts provide unique information about the neutron star crust and underlying dense matter. Comparisons between astronomical obse…
Treating quarks within neutron stars
Sophia Han, M. A. A. Mamun, S. Lalit +2
Neutron star interiors provide the opportunity to probe properties of cold dense matter in the QCD phase diagram. Utilizing models of dense matter in accord with nuclear systematic…
Dense matter equation of state for neutron star mergers
S. Lalit, M. A. A. Mamun, C. Constantinou +1
In simulations of binary neutron star mergers, the dense matter equation of state (EOS) is required over wide ranges of density and temperature as well as under conditions in which…
Thermal Effects in Dense Matter Beyond Mean Field Theory
Constantinos Constantinou, Sudhanva Lalit, Madappa Prakash
The formalism of next-to-leading order Fermi Liquid Theory is employed to calculate the thermal properties of symmetric nuclear and pure neutron matter in a relativistic many-body…