Compact Object Modeling with the StarTrack Population Synthesis Code

Abstract

We present a comprehensive description of the population synthesis code StarTrack. The original code has been significantly modified and updated. Special emphasis is placed here on processes leading to the formation and further evolution of compact objects (white dwarfs, neutron stars, and black holes). Both single and binary star populations are considered. The code now incorporates detailed calculations of all mass-transfer phases, a full implementation of orbital evolution due to tides, as well as the most recent estimates of magnetic braking. This updated version of StarTrack can be used for a wide variety of problems, with relevance to many current and planned observatories, e.g., studies of X-ray binaries (Chandra, XMM-Newton), gravitational radiation sources (LIGO, LISA), and gamma-ray burst progenitors (HETE-II, Swift). The code has already been used in studies of Galactic and extra-galactic X-ray binary populations, black holes in young star clusters, Type Ia supernova progenitors, and double compact object populations. Here we describe in detail the input physics, we present the code calibration and tests, and we outline our current studies in the context of X-ray binary populations.

40 pages, 14 figures, accepted to ApJS (major extensions/revisions)

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• The High Time Resolution Universe Pulsar Survey -- XVII. PSR J1325-6253, a low eccentricity double neutron star system from an ultra-stripped supernova
• Exploring compact binary populations with the Einstein Telescope
• Binary Black Hole Mergers within the LIGO Horizon: Statistical Properties and prospects for detecting Electromagnetic Counterparts
• Impact of natal kicks on merger rates and spin-orbit misalignments of black hole -- neutron star mergers
• Close Encounters of Stars with Stellar-mass Black Hole Binaries
• dart_board: Binary Population Synthesis with Markov Chain Monte Carlo
• R Coronae Borealis Stars are Viable Factories of Pre-solar Grains
• Effects of Irradiation on the Evolution of Ultra-compact X-ray Binaries
• Mining for Candidates of Galactic Stellar-mass Black Hole Binaries with LAMOST
• Population synthesis on high-mass X-ray binaries: prospects and constraints from the universal X-ray luminosity function
• MOCCA: Dynamics and evolution of binary stars of multiple stellar populations in tidally filling and underfilling globular star clusters
• Progenitors of low-mass binary black-hole mergers in the isolated binary evolution scenario
• Orbital period dependent spatial scatter of Galactic Black Hole Transients
• Observational constraints on the origin of the elements. V. Non-LTE abundance ratios of [Ni/Fe] in Galactic stars and enrichment by sub-Chandrasekhar mass SNe
• Monte Carlo population synthesis on massive star binaries: Astrophysical implications for gravitational wave sources
• Supernovae Producing Unbound Binaries and Triples
• On the Mass Ratio Distribution of Black Hole Mergers in Triple Systems
• Formation and Evolution of Galactic Intermediate/Low-Mass X-ray Binaries
• The role of stellar expansion on the formation of gravitational wave sources
• The Blue Stragglers of the Old Open Cluster NGC 188
• Scenario Machine: fast radio bursts, short gamma-ray burst, dark energy and Laser Interferometer Gravitational-wave Observatory silence
• Unmodelled Clustering Methods for Gravitational Wave Populations of Compact Binary Mergers
• Core radii and common-envelope evolution
• Young Accreting Compact Objects in M31: The Combined Power of NuSTAR, Chandra, and Hubble
• X-ray luminosity function of high-mass X-ray binaries: Studying the signatures of different physical processes using detailed binary evolution calculations
• Revisiting Common Envelope Evolution -- A New Semi-Analytic Model for N-body and Population Synthesis Codes
• Exploring the borderline between stable mass transfer and mergers in close binary evolution
• GW170817: implications for the local kilonova rate and for surveys from ground-based facilities
• Binary black holes mergers from hierarchical triples in open clusters
• Remnant masses from 1D+ core-collapse supernovae simulations: bimodal neutron star mass distribution and black holes in the low-mass gap
• Neutron Star Physics in the Square Kilometer Array Era : An Indian Perspective
• The spin, expansion and contraction of open star clusters
• The dawn of a new era for dustless HdC stars with GAIA eDR3
• LISA sources from young massive and open stellar clusters
• Comparing compact binary parameter distributions I: Methods
• Tidal Dissipation Impact on the Eccentric Onset of Common Envelope Phases in Massive Binary Star Systems
• The Location and Environments of Neutron Star Mergers in an Evolving Universe
• Probing the X-Ray Binary Populations of the Ring Galaxy NGC 1291
• The black hole retention fraction in star clusters
• Effect of orbital eccentricity on the dynamics of precessing compact binaries
• Reverse Algols and hydrogen-rich Wolf-Rayet stars from very massive binaries
• Population synthesis of accreting white dwarfs: Rates and evolutionary pathways of H and He novae
• Comparing Chandra and Hubble in the Northern Disk of M31
• X-ray Binaries and Star Clusters in the Antennae: Optical Cluster Counterparts
• The role of binding energies of neutron stars on the accretion driven evolution
• A systematic study of super-Eddington layers in the envelopes of massive stars
• The Stellar Age Dependence of X-ray Emission from Normal Star-Forming Galaxies in the GOODS Fields
• Detailed equilibrium and dynamical tides: impact on circularization and synchronization in open clusters
• Predicting the self-lensing population in optical surveys
• Simulations of the tidal interaction and mass transfer of a star in an eccentric orbit around an intermediate-mass black hole: the case of HLX-1
• The Galactic Millisecond Pulsar Population
• Common origin for black holes in both high mass X-ray binaries and gravitational-wave sources
• Dynamical formation of Black Hole Low-Mass X-Ray Binaries in the field - an alternative to common envelope
• Rapid population synthesis of black-hole high-mass X-ray binaries: implications for binary stellar evolution
• Exploring binary black hole mergers and host galaxies with Shark and COMPAS
• Population Synthesis of Millisecond X-ray Pulsars
• Revisiting the Galactic Double Neutron Star merger and LIGO detection rates
• Black Holes In Young Stellar Clusters
• The Impact of Initial-Final Mass Relations on Black Hole Microlensing
• The Galactic Underworld: The spatial distribution of compact remnants
• Wind-powered ultraluminous X-ray sources
• Forward Modelling the O3(a+b) GW transient mass distributions with BPASS by varying compact remnant mass and SNe kick prescriptions
• The impact of metallicity on nova populations
• Backward Population Synthesis: Mapping the Evolutionary History of Gravitational-Wave Progenitors
• Collective Properties of X-ray Binary Populations of Galaxies. I. Luminosity and Orbital Period Distributions of High-Mass X-ray Binaries
• Detectability of continuous gravitational waves from isolated neutron stars in the Milky Way: the population synthesis approach
• Mergers of neutron stars and black holes with cores of giant stars: a population synthesis study
• Rapid formation of a very massive star >50000 $M_{\odot }$ and subsequently an IMBH from runaway collisions. Direct N-body and Monte Carlo simulations of dense star clusters
• Ultra wide black-hole - neutron star binaries as a possible source for gravitational waves and short gamma ray bursts
• Average bolometric corrections and optical to X-ray flux measurements as a function of accretion rate for X-ray binaries
• On the Simultaneous Modelling of Dust and Stellar Populations for Interpretation of Galaxy Properties
• Lower-mass-gap Black Holes in Dense Star Clusters
• End-to-end study of the home and genealogy of the first binary neutron star merger
• Searching for Millisecond Pulsars: Surveys, Techniques and Prospects
• Expected number of supergiant fast X-ray transients in the Milky Way
• Understanding the progenitor formation galaxies of merging binary black holes
• Theoretical Delay Time Distributions
• Footprints of population III stars in the gravitational-wave background
• Populations of evolved massive binary stars in the Small Magellanic Cloud I: Predictions from detailed evolution models
• Accretion disks in Algols: progenitors and evolution
• The Binary Black Hole Merger Rate from Ultraluminous X-ray Source Progenitors
• Repeated mergers of black hole binaries: implications for GW190521
• Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries
• Modelling stellar evolution in mass-transferring binaries and gravitational-wave progenitors with METISSE
• High proper motion X-ray binaries from the Yale Southern Proper Motion Survey
• An Alternative Channel For High-Mass Binary Black Holes-----Dark Matter Accretion Onto Black Hole
• Whispering in the dark: Faint X-ray emission from black holes with OB star companions
• Merger rate density of stellar-mass binary black holes from young massive clusters, open clusters, and isolated binaries: comparisons with LIGO-Virgo-KAGRA results
• Simulations of the progenitors of black hole-neutron star gravitational wave sources
• The long and the short of it: modelling double neutron star and collapsar Galactic dynamics
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• On the Rarity of X-Ray Binaries with Naked Helium Donors
• The Demographics of Binary Companions to Stripped-Envelope Supernovae: Confronting Observations with Population Synthesis
• New insights on binary black hole formation channels after GWTC-2: young star clusters versus isolated binaries
• What Determines the Maximum Mass of AGN-assisted Black Hole Mergers?
• New constraints on the Bray conservation-of-momentum natal kick model from multiple distinct observations
• Synthetic population of binary Cepheids. I. The effect of metallicity and initial parameter distribution on characteristics of Cepheids' companions
• Effects of the core-collapse supernova ejecta impact on a rapidly rotating massive companion star
• The Population of Helium-Merger Progenitors: Observational Predictions
• The rate of iPTF 14gqr like ultra-stripped supernovae and binary evolution leading to double neutron star formation
• Supernova and prompt gravitational-wave precursors to LIGO gravitational-wave sources and short-GRBs
• Growth of Massive Black Hole Seeds by Migration of Stellar and Primordial Black Holes: Gravitational Waves and Stochastic Background
• Active Learning for Computationally Efficient Distribution of Binary Evolution Simulations
• Surrogate forward models for population inference on compact binary mergers
• Testing the robustness of simulation-based gravitational-wave population inference
• Infrared outbursts as potential tracers of common envelope events in high-mass X-ray binary formation
• Development of convective envelopes in massive stars: Implications for gravitational wave sources
• Chandra Observations of the Collisional Ring Galaxy NGC 922
• Searching for ejected supernova companions in the era of precise proper motion and radial velocity measurements
• Gravitational Radiation from Close Binaries with Time-Varying Masses
• A Nuclear Equation of State Inferred from Stellar r-process Abundances
• Single Millisecond Pulsars from Dynamical Interaction Processes in Dense Star Clusters
• Common Envelope Mechanisms: Constraints from the X-ray Luminosity Function of High Mass X-ray Binaries
• Donors of Persistent Neutron-star Low-mass X-ray Binaries
• Common Proper Motion Wide White Dwarf Binaries Selected From The Sloan Digital Sky Survey
• Effects of Rotationally-Induced Mixing in Compact Binary Systems with Low-Mass Secondaries and in Single Solar-Type Stars
• X-ray Binaries in External Galaxies
• A Search for Unbound Stellar Companions to Pulsar J1124-5916
• The impact of precession on the observed population of ULXs
• Applications of Stellar Population Synthesis in the Distant Universe
• Nucleosynthetic Yields from Neutron Stars Accreting in Binary Common Envelopes
• Long gamma ray burst rate in the binary merger progenitor model
• The Contribution Of Outer HI Disks To The Merging Binary Black Hole Population
• Binary Evolution: Roche Lobe Overflow and Blue Stragglers
• Reconstructing parametric gravitational-wave population fits from non-parametric results without refitting the data
• Young and eccentric: the quadruple system HD 86588
• Prospects of direct detection of ${}^{48}$V gamma-rays from thermonuclear supernovae
• The contribution of X-ray binaries to the evolution of late-type galaxies: Evolutionary population synthesis simulations
• Astrometric mass measurement of compact companions in binary systems with Gaia
• Reconstructing post-common envelope white dwarf+main sequence binary histories through inverse population synthesis techniques
• Rethinking mass transfer: a unified semi-analytical framework for circular and eccentric binaries. I. Orbital evolution due to conservative mass transfer
• Can the Subsonic Accretion Model Explain the Spin Period Distribution of Wind-fed X-ray Pulsars?
• Evidence for low kick velocities among high-mass X-ray binaries in the Small Magellanic Cloud from the spatial correlation function
• Stacking Star Clusters in M51: Searching for Faint X-Ray Binaries
• Population Synthesis of Black Hole Binaries with Compact Star Companions
• Using chemical evolution models of the Milky Way disk to constrain Type Ia supernova progenitors
• Synthetic Population of Binary Cepheids. II. The effect of companion light on the extragalactic distance scale
• Astrophysics with the Laser Interferometer Space Antenna
• Gravitational Waves from Stellar Black Hole Binaries and the Impact on Nearby Sun-like Stars
• Faint X-ray Binaries and Their Optical Counterparts in M31
• Modelling multiwavelength emission of Ultra-luminous X-ray Sources accreting above the Eddington limit
• Compact object populations over cosmic time II. Compact object merger rates and masses over redshift from varying initial conditions
• Hubble without the Hubble: cosmology using advanced gravitational-wave detectors alone
• X-ray emission from helium star+black hole binaries as probes of tidally induced spin-up of second-born black holes
• Merger of a Neutron Star with a Black Hole: one-family vs. two-families scenario
• Hα imaging for BeXRBs in the Small Magellanic Cloud
• On the rapid orbital expansion in the compact low-mass X-ray binary 2A 1822$-$371
• The properties of long gamma-ray bursts in massive compact binaries
• Polar kicks and the spin period - eccentricity relation in double neutron stars
• VLT/MUSE and ATCA observations of the host galaxy of the short GRB 080905A at z=0.122
• The cosmological distribution of compact object mergers from dynamical interactions with SMBH binaries
• Heavy element contributions of rotating massive stars to Interstellar Medium
• Rethinking mass transfer: a unified semianalytical framework for circular and eccentric binaries. II. Orbital evolution due to nonconservative mass transfer
• The Black Hole Candidate Swift J1728.9$-$3613 and the Supernova Remnant G351.9$-$0.9
• MOCCA-Survey Database: Extra Galactic Globular Clusters. III. The population of black holes in Milky Way and Andromeda-like galaxies
• LB-1 is inconsistent with the X-ray source population and pulsar-black hole binary searches in the Milky Way
• Formation of millisecond pulsar-helium star binaries
• LAMOST medium-resolution spectroscopic survey of binarity and exotic star (LAMOST-MRS-B): Observation strategy and target selection
• Strong Variability in AzV 493, an Extreme Oe-Type Star in the SMC
• Weighing the Darkness II: Astrometric Measurement of Partial Orbits with Gaia
• Local merger rates of double neutron stars
• Implications of binary black hole detections on the merger rates of double neutron stars and neutron star-black holes
• Magnetic Interaction in Ultra-compact Binary Systems
• Accretion, Ablation and Propeller Evolution in Close Millisecond Pulsar Binary Systems
• The effects of Galactic model uncertainties on LISA observations of double neutron stars
• Wolf-Rayet -- compact object binaries as progenitors of binary compact objects
• Chirp mass-distance distributions of the sources of gravitational waves
• Emulators for stellar profiles in binary population modeling
• Evaluating the gravitational wave detectability of globular clusters and the Magellanic Clouds for LISA
• Reconstructing the star formation rate for compact binary populations with the Einstein telescope
• Impact of Population III stars on the astrophysical gravitational-wave background
• Event Rate of Fast Radio Burst from Binary Neutron-star Mergers
• Planetary Systems in a Star Cluster II: intermediate-mass black holes and planetary systems
• On the Astrophysical Origin of Binary Black Hole Subpopulations: A Tale of Three Channels?
• Searches for Gravitational Waves from Binary Neutron Stars: A Review
• Close encounters with the Death Star: Interactions between collapsed bodies and the Solar System
• Dark Star Clusters or Ultra-Faint Dwarf galaxies? Revisiting UMa3/U1
• Effect of tides on the orbital evolution of the redback system PSR 1723-2837
• Ultraluminous X-ray sources in Globular Clusters
• Fundamental parameters of the massive eclipsing binary HM1 8
• Uncovering the identities of compact objects in high-mass X-ray binaries and gamma-ray binaries by astrometric measurements
• Collective Properties of X-ray Binary Populations of Galaxies II. Pre-Low-mass X-ray Binary Properties, Formation Rates, and Constraints
• Compact object populations over cosmic time I. BOSSA: a Binary Object environment-Sensitive Sampling Algorithm
• Population Synthesis of Gravitational Wave Sources
• Calibration of Binary Population Synthesis Models Using White Dwarf Binaries from APOGEE, GALEX and Gaia
• Comparing population synthesis models of compact double white dwarfs to electromagnetic observations
• Spatial mixing of stellar populations in globular clusters via binary-single star scattering
• Helium emission from Balmer-dominated shocks in Type Ia supernova remnants provides constraints to their progenitor systems
• Origin of High Dark Remnant Fractions in Milky Way Globular Clusters: The Crucial Role of Initial Black Hole Retention
• Evolutionary tracks of binary neutron star progenitors across cosmic times
• Determination method of binary fractions by the integrated spectrum
• Testing the presence of a dormant black hole inside HR 6819
• Kilonova rates from spherical and axisymmetrical models
• Models of Individual Blue Stragglers
• Single-event likelihood of star cluster properties with LIGO-Virgo-Kagra binary black hole observations
• True Unicorns and False Positives: Simulated Probabilities of Dark Massive Companions to Bright Stars
• Interpreting Galaxy Properties with Improved Modelling
• Inferences about the distribution, merger rate, and evolutionary processes of compact binaries from gravitational wave observations
• Magnetic fileds of coalescing neutron stars and the luminosity function of short gamma-ray burst
• The X-ray binaries in M83: will any of them form gravitational wave sources for LIGO/VIRGO/KAGRA?
• Constraints on Weak Supernova Kicks from Observed Pulsar Velocities
• A Fundamental Plane in X-ray Binary Activity of External Galaxies
• Could the high-mass black holes from gravitational-wave observations be explained by lensing?
• Mock Catalogs of Strongly Lensed Gravitational Waves via A Halo Model Approach with Ground-based Detectors
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations II: Double Compact Object Rates and Properties
• Identifying Host Galaxies of Binary Black Hole Mergers with Next-Generation Gravitational Wave Detector Networks
• Merging massive black holes: the right place and the right time
• Modern tidal interaction models for rapid binary population synthesis: I. Methods
• SN1991bg-like supernovae are a compelling source of most Galactic antimatter
• SMC3 as a test to the binary evolution
• The Progenitor of the S147 Supernova Remnant
• Diagnosing the Properties and Evolutionary Fates of Black Hole and Wolf-Rayet X-ray Binaries as Potential Gravitational Wave Sources for the LIGO-Virgo-KAGRA Network
• Simulation-calibrated Bayesian inference for progenitor properties of the microquasar SS 433
• Self-lensing binaries as probes of Supernova physics
• Detailed properties of gravitational-wave mergers from flyby perturbations of wide binary black holes in the field
• Constraining Black Hole Natal Kicks with Astrometric Microlensing
• Revisiting black hole hyperaccretion in the center of gamma-ray bursts for the lower mass gap
• A database of spectral energy distributions of progenitors of core-collapse supernovae
• Modelling the formation of the first two neutron star-black hole mergers, GW200105 and GW200115: metallicity, chirp masses and merger remnant spins
• Impact of tides on non-coplanar orbits of progenitors of high-mass X-ray binaries
• Dynamical double black holes and their host cluster properties
• On the apparent lack of be x-ray binaries with black holes in the galaxy and in the Magellanic clouds
• A Synthetic Population of Ultra-Luminous X-ray Sources: Optical-X-ray Correlation
• Resolving white dwarf binaries within globular clusters with LISA