Cococubed.com Neutron Star & Black Hole Mass Function
Home Astronomy Research    2025 Neutrinos From De-excitation    Radiative Opacity    2024 Neutrino Emission from Stars    2023 White Dwarfs & 12C(α,γ)16O    2023 MESA VI    2022 Earendel, A Highly Magnified Star    2022 Black Hole Mass Spectrum    2021 Skye Equation of State    2021 White Dwarf Pulsations & 22Ne    Software Instruments      Stellar equation of states      EOS with ionization      EOS for supernovae      Chemical potentials      Stellar atmospheres      Voigt Function      Jeans escape      Polytropic stars      Cold white dwarfs      Adiabatic white dwarfs      Cold neutron stars      Stellar opacities      Neutrino energy loss rates      Ephemeris routines      Fermi-Dirac functions      Polyhedra volume      Plane - cube intersection      Coating an ellipsoid      Nuclear reaction networks      Nuclear statistical equilibrium      Laminar deflagrations      CJ detonations      ZND detonations      Fitting to conic sections      Unusual linear algebra      Derivatives on uneven grids      Pentadiagonal solver      Quadratics, Cubics, Quartics      Supernova light curves      Exact Riemann solutions      1D PPM hydrodynamics      Hydrodynamic test cases      Galactic chemical evolution      Universal two-body problem      Circular and elliptical 3 body      The pendulum      Phyllotaxis      MESA      MESA-Web      FLASH      Zingale's software      Brown's dStar      GR1D code      Iliadis' STARLIB database      Herwig's NuGRID      Meyer's NetNuc 2026 AAS Journals    AAS YouTube    Listing of 500+ Author Videos    AAS Peer Review Workshops Outreach Material Education Material Other Stuff:    Bicycle Adventures    Illustrations    Presentations Contact: F.X.Timmes my one page vitae, full vitae, research statement, and teaching statement.	You can download the chemical evolution code that generated these foregoing abundance histories. Here is a journal paper that describes this prediction of the initial mass function for neutron stars and black holes. Core and Remnant Masses Zero metallicity Solar Metallicity Finer mass grid   Remnant Distribution Functions Iron core only Iron + Silicon shell Post Explosion Explosion energy dependence   Birth Functions Pure Type II Supernovae Half Type II + Half Type Ib Pure Type Ib Supernovae Sensitivity to slope   Observations Only Measured neutron star masses High-mass x-ray binary masses