The Formation of the First Star in the Universe

Abstract

We describe results from a fully self-consistent three dimensional hydrodynamical simulation of the formation of one of the first stars in the Universe. Dark matter dominated pre-galactic objects form because of gravitational instability from small initidal density perturbations. As they assemble via hierarchical merging, primordial gas cools through ro-vibrational lines of hydrogen molecules and sinks to the center of the dark matter potential well. The high redshift analog of a molecular cloud is formed. When the dense, central parts of the cold gas cloud become self-gravitating, a dense core of approximately 100 solar mass undergoes rapid contraction. At densities n>10^9 cm^-3 a one solar mass proto-stellar core becomes fully molecular due to three-body H_2 formation. Contrary to analytical expectations this process does not lead to renewed fragmentation and only one star is formed. The calculation is stopped when optical depth effects become important, leaving the final mass of the fully formed star somewhat uncertain. At this stage the protostar is acreting material very rapidly (~0.01 solar masses per year). Radiative feedback from the star will not only halt its growth but also inhibit the formation of other stars in the same pre-galactic object (at least until the first star ends its life, presumably as a supernova). We conclude that at most one massive (M >> 1 solar mass) metal free star forms per pre-galactic halo, consistent with recent abundance measurements of metal poor galactic halo stars.

8 pages, 5 figures. Science. Published in Science Express online on 11/15/2001. More information can be found at http://www.TomAbel.com/GB/

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• Simulating the assembly of galaxies at redshifts z = 6 - 12
• The Cosmic Near Infrared Background: Remnant Light from Early Stars
• Dark Stars: A Review
• Fossil remnants of reionization in the halo of the Milky Way
• A Model For Infall Around Virialized Halos
• Pair Instability Supernovae of Very Massive Population III Stars
• The First Generation of Star-Forming Haloes
• The influence of magnetic fields on the thermodynamics of primordial star formation
• The Impact of Box Size on the Properties of Dark Matter Haloes in Cosmological Simulations
• Robust Velocity-induced Acoustic Oscillations at Cosmic Dawn
• Suppression of HD-cooling in protogalactic gas clouds by Lyman-Werner radiation
• Chandra Observations of the Three Most Metal-Deficient Blue Compact Dwarf Galaxies known in the Local Universe, SBS 0335-052, SBS 0335-052W, and I Zw 18
• Revised rate coefficients for H${}_2$ and H${}^{-}$ destruction by realistic stellar spectra
• Dark Matter Capture in the First Stars: a Power Source and Limit on Stellar Mass
• X-ray emission from high-redshift miniquasars: self-regulating the population of massive black holes through global warming
• The First Stars
• The Extended Starformation History of the First Generation of Stars, and the Reionization of Cosmic Hydrogen
• Carbon-Enhanced Metal-Poor Stars, the Cosmic Microwave Background, and the Stellar IMF in the Early Universe
• Making a supermassive star by stellar bombardment
• Cosmological Feedback from High-Redshift Dwarf Galaxies
• Seeding the Second Star: enrichment from population III, dust evolution, and cloud collapse
• Star formation at very low metallicity. II: On the insignificance of metal-line cooling during the early stages of gravitational collapse
• A photometric survey for Lyalpha-HeII dual emitters: Searching for Population III stars in high-redshift galaxies
• Probing the Epoch of Reionization with Milky Way Satellites
• Unique Signatures of Population III Stars in the Global 21-cm Signal
• The mass spectrum of metal-free Stars resulting from photodissociation feedback: A scenario for the formation of low-mass population III stars
• Carbon-Enhanced Hyper-metal-poor Stars and the Stellar IMF at Low Metallicity
• A Standard Ruler at Cosmic Dawn
• Limits on Population III star formation in minihaloes implied by Planck
• The observational signature of the first H II regions
• Pristine IX: CFHT ESPaDOnS Spectroscopic Analysis of 115 Bright Metal-Poor Candidate Stars
• Protostellar Feedback and Final Mass of the Second-Generation Primordial Stars
• First Sources in Infrared Light: Stars, Supernovae and Miniquasars
• Simulating high-z Gamma-ray Burst host galaxies
• Probing the existence of very massive first stars
• New observational Constraints on the Growth of the First Supermassive Black Holes
• Spectral Signature of Cosmological Infall of Gas Around the First Quasars
• Forming massive seed black holes in high-redshift quasar host progenitors
• A Ly-alpha Emitter with an Extremely Large Rest-frame Equivalent Width of ~900A at z=6.5: A Candidate of Population III-dominated Galaxy?
• Gravitational instability in protostellar disks at low metallicities
• Dark Stars: a new look at the First Stars in the Universe
• On the First Generation of Stars
• On the formation of very metal-poor stars: The case of SDSS J1029151+172927
• Heating the IGM by X-rays from Population III Binaries in High Redshift Galaxies
• maxsmooth: Rapid Maximally Smooth Function Fitting With Applications in Global 21-cm Cosmology
• Hypernovae and Other Black-Hole-Forming Supernovae
• Radiative lifetimes and cooling functions for astrophysically important molecules
• Rate Coefficient for H^+ + H_2(X ^1Sigma_g^+, nu=0, J=0) --> H(1s) + H_2^+ Charge Transfer and Some Cosmological Implications
• An old, metal-poor globular cluster in Sextans A and the metallicity floor of globular cluster systems
• Grids of stellar models with rotation: V. Models from 1.7 to 120 Msun at zero metallicity
• Chemical signatures of the first star clusters
• An Introductory Review on Cosmic Reionization
• The formation of massive Pop III stars in the presence of turbulence
• Block Structured Adaptive Mesh and Time Refinement for Hybrid, Hyperbolic + N-body Systems
• Chemistry of the Most Metal-poor Stars in the Bulge and the z > 10 Universe
• The Deaths of Very Massive Stars
• The impact of an evolving stellar initial mass function on early galaxies and reionisation
• First star formation with dark matter annihilation
• Lyman Alpha Driven Outflows Around Star Forming Galaxies
• Supermassive Black Hole Growth and Merger Rates from Cosmological N-body Simulations
• Numerical Simulations of High Redshift Star Formation in Dwarf Galaxies
• Gas depletion in primordial globular clusters due to accretion onto stellar-mass black holes
• Star Formation at Very Low Metallicity. IV. Fragmentation Does Not Depend on Metallicity for Cold Initial Conditions
• Strong magnetic fields and large rotation measures in protogalaxies by supernova seeding
• Ultra-faint dwarf galaxies: unveiling the minimum mass of the first stars
• Large-Scale Structure Formation: from the first non-linear objects to massive galaxy clusters
• Radio Afterglows of Gamma-Ray Bursts and Hypernovae at High Redshift, and their Potential for 21-cm Absorption Studies
• Fitting formulae for evolution tracks of massive stars under extreme metal poor environments for population synthesis calculations and star cluster simulations
• Star Formation at Very Low Metallicity. V. The Greater Importance of Initial Conditions Compared to Metallicity Thresholds
• Finding the First Cosmic Explosions II: Core-Collapse Supernovae
• Constraints on the small-scale power spectrum of density fluctuations from high-redshift gamma-ray bursts
• Fluctuations in the High-Redshift Lyman-Werner and Lyman-alpha Radiation Backgrounds
• The role of HD cooling in primordial star formation
• Finding the First Cosmic Explosions. III. Pulsational Pair-Instability Supernovae
• Influence of primordial magnetic fields on 21 cm emission
• Magnetic Fields in the Formation of the First Stars. I. Theory vs. Simulation
• Discovery of the most metal-poor damped Lyman-alpha system
• The Supernova that Destroyed a Protogalaxy: Prompt Chemical Enrichment and Supermassive Black Hole Growth
• The first galaxies: simulating their feedback-regulated assembly
• Impact of dust cooling on direct collapse black hole formation
• Supermassive Population III Supernovae and the Birth of the First Quasars
• Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
• Supersonic Relative Velocity between Dark Matter and Baryons: A Review
• Resolving Gas Dynamics in the Circumnuclear Region of a Disk Galaxy in a Cosmological Simulation
• Assessing inflow rates in atomic cooling halos: implications for direct collapse black holes
• Binary Formation in Star-Forming Clouds with Various Metallicities
• Chemical enrichment of Damped Lyman Alpha systems as a direct constraint on Population III star formation
• Detecting gravitationally lensed population III galaxies with the Hubble Space Telescope and the James Webb Space Telescope
• A New Statistical Model for Population III Supernova Rates: Discriminating Between $\Lambda$CDM and WDM Cosmologies
• Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7
• Heating of the Intergalactic Medium by Primordial Miniquasars
• Impact of Cosmic Rays on Population III Star Formation
• Implications of WMAP 3 Year Data for the Sources of Reionization
• The Strömgren sphere, the environment and the reionization in the local universe of the highest redshift QSOs
• Supernova dust formation and the grain growth in the early universe: The critical metallicity for low-mass star formation
• The Premature Formation of High Redshift Galaxies
• The formation of massive primordial stars in the presence of moderate UV backgrounds
• The origin of carbon: Low-mass stars and an evolving, initially top-heavy IMF?
• The Opacity of the Intergalactic Medium During Reionization: Resolving Small-Scale Structure
• Trapping of HII regions in Population III star formation
• Primordial Stellar Feedback and the Origin of Hyper Metal-Poor Stars
• Implications of Quasar Black Hole Masses at High Redshifts
• The Chemical Imprint of Silicate Dust on the Most Metal-Poor Stars
• Metallicity and the Universality of the IMF
• The earliest stars and their relics in the Milky Way
• Cosmic Backgrounds from Miniquasars
• The characteristic stellar mass as a function of redshift
• Detectability of the First Cosmic Explosions
• The Number and Observability of Population III Supernovae at High Redshifts
• The sustainable growth of the first black holes
• Probing the stellar initial mass function with high-$z$ supernovae
• Revisiting The First Galaxies: The epoch of Population III stars
• The Formation of Supermassive Black Holes from Population III.1 Seeds. I. Cosmic Formation Histories and Clustering Properties
• Impact of Primordial Ultracompact Minihaloes on the Intergalactic Medium and First Structure Formation
• Following The Cosmic Evolution Of Pristine Gas I: Implications For Milky Way Halo Stars
• Magnetic fields in cosmic particle acceleration sources
• The Ultimately Large Telescope -- what kind of facility do we need to detect Population III stars?
• Star Formation at the Twilight of the Dark Ages: Which Stars Reionized the Universe?
• Pair-Instability Supernova Simulations: Progenitor Evolution, Explosion, and Light Curves
• Population III Gamma-Ray Bursts and Breakout Criteria for Accretion-Powered Jets
• The Biggest Explosions in the Universe
• On the faint-end of the high-$z$ galaxy luminosity function
• Dissipation of Magnetic Flux in Primordial Gas Clouds
• Accretion Phase of Star Formation in Clouds with Different Metallicities
• An Ultra Metal-poor Star Near the Hydrogen-burning Limit
• A tale of two sites -- II: Inferring the properties of minihalo-hosted galaxies with upcoming 21-cm interferometers
• Photoevaporation of Circumstellar Disks Revisited: The Dust-Free Case
• Physical properties of the first quasars
• The Nature of CO Emission From z~6 Quasars
• Testing Reionization with Gamma Ray Burst Absorption Spectra
• Formation of HD molecules in merging dark matter haloes
• The Impact of Lyman alpha Trapping on the Formation of Primordial Objects
• Formation of supermassive black hole seeds in nuclear star clusters via gas accretion and runaway collisions
• Lyman-Werner UV Escape Fractions from Primordial Halos
• Binary Formation with Different Metallicities: Dependence on Initial Conditions
• Supermassive Dark Star candidates seen by JWST?
• Unveiling early black hole growth with multi-frequency gravitational wave observations
• Star Formation in the Most Distant Molecular Cloud in the Extreme Outer Galaxy: A Laboratory of Star Formation in an Early Epoch of the Galaxy's Formation
• Gas in Simulations of High Redshift Galaxies and Minihalos
• The onset of star formation in primordial haloes
• Long Duration X-Ray Flash and X-Ray Rich Gamma Ray Burst from Low Mass Population III Star
• Star Formation in Molecular Clouds
• Detection strategies for the first supernovae with JWST
• Direct Collapse to Supermassive Black Hole Seeds with Radiative Transfer: Isolated Halos
• Supermassive Black Hole Seed Formation at High Redshifts: Long-Term Evolution of the Direct Collapse
• Illuminating the Primeval Universe with Type IIn Supernovae
• Interpreting the Global 21-cm Signal from High Redshifts. I. Model Independent Constraints
• The Biggest Explosions in the Universe. II
• Optimized Multi-Frequency Spectra for Applications in Radiative Feedback and Cosmological Reionization
• Simulations of galaxy formation with radiative transfer: Hydrogen reionization and radiative feedback
• Clues on the presence and segregation of very massive stars in the Sunburst Lyman-continuum cluster at z=2.37
• How AGN and SNe feedback affect mass transport and black hole growth in high redshift galaxies
• Population III Star Formation in a Lambda WDM Universe
• Origin of Cosmic Chemical Abundances
• The role of stellar relaxation in the formation and evolution of the first massive black holes
• Looking for Population III stars with He II line intensity mapping
• Scaling Relations for Galaxies Prior to Reionization
• Galaxy Genesis -- unravelling the epoch of dissipation in the early disk
• The Relative Role of Galaxy Mergers and Cosmic Flows in Feeding Black Holes
• Stellar Winds and Coronae of Low-mass Pop. II/III Stars
• The Pristine survey -- XII: Gemini-GRACES chemo-dynamical study of newly discovered extremely metal-poor stars in the Galaxy
• Stochastic chemical enrichment in metal-poor systems I. Theory
• Intermediate-Mass Black Holes in Early Globular Clusters
• X-ray Twinkles and Pop III Stars
• WIMP DM and first stars: suppression of fragmentation in primordial star formation
• Star-forming accretion flows and the low luminosity nuclei of giant elliptical galaxies
• Radiative and Kinetic Feedback by Low-Mass Primordial Stars
• Supermassive Black Hole Formation at High Redshifts Through a Primordial Magnetic Field
• Population III Star Formation In Large Cosmological Simulations I. Halo Temporal and Physical Environment
• Dissipation of Magnetic Flux in Primordial Star Formation: From Run-away Phase to Mass Accretion Phase
• Dark stars: Implications and constraints from cosmic reionization and extragalactic background radiation
• The Formation of Population III Binaries
• Long-term evolution of supercritical black hole accretion with outflows: a subgrid feedback model for cosmological simulations
• Generation of Seed Magnetic Field around First Stars: the Biermann Battery Effect
• Stationary Population III accretion discs
• The Emergence of the First Star-free Atomic Cooling Haloes in the Universe
• The Lack of Gamma-Ray Bursts from Population III Binaries
• Magnetic fields in the formation of the first stars.--II Results
• An equatorial ultra iron-poor star identified in BOSS
• Dark Matter Halo Environment for Primordial Star Formation
• Following the Cosmic Evolution of Pristine Gas III: The Observational Consequences of the Unknown Properties of Population III Stars
• The Radio to Infrared Emission of Very High Redshift Gamma-Ray Bursts: Probing Early Star Formation through Molecular and Atomic Absorption Lines
• Generation of Seed Magnetic Field around First Stars:Effects of Radiation Force
• The Redshift Distribution of Distant Supernovae and its Use in Probing Reionization
• Disk fragmentation and the formation of population III stars
• Direct Collapse to Supermassive Black Hole Seeds with Radiation Transfer: Cosmological Halos
• The effects of Population III stars and variable IMF on the chemical evolution of the Galaxy
• A cryogenic liquid-mirror telescope on the moon to study the early universe
• The First Stars: formation under X-ray feedback
• First stars and the extragalactic background light: How recent gamma-ray observations constrain the early universe
• Growing Massive Black Holes in a Local Group Environment: the Central Supermassive, Slowly Sinking, and Ejected Populations
• Gravitational wave background from population III binaries
• Circular Polarization of the CMB: A probe of the First stars
• Cosmic rays and the primordial gas
• The Supersonic Project: Shining Light on SIGOs - a New Formation Channel for Globular Clusters
• Did Massive Primordial Stars Preenrich the Lyman Alpha Forest?
• Feedback from the IR Background in the Early Universe
• Low-metallicity star formation: Relative impact of metals and magnetic fields
• Formation of the first stars
• Formation History of Metal-Poor Halo Stars with Hierarchical Model and the Effect of ISM accretion on the Most Metal-Poor Stars
• Non-thermal photons and H2 formation in the early Universe
• Dark matter annihilation from intermediate-mass black holes: Contribution to the extragalactic gamma-ray background
• Primordial Molecular Emission in Population III Galaxies
• Spatially Extended 21 cm Signal from Strongly Clustered UV and X-Ray Sources in the Early Universe
• Fully-Coupled Simulation of Cosmic Reionization. I: Numerical Methods and Tests
• Revisiting the Contributions of Supernova and Hypernova Remnants to the Diffuse High-Energy Backgrounds: Constraints on Very-High-Redshift Injections
• A Study of Primordial Very Massive Star Evolution
• Radiative cooling implementations in simulations of primordial star formation
• The formation of protostellar binaries in primordial minihalos
• Probing Population III Stars in Galaxy IOK-1 at z = 6.96 through He II Emission
• An Observational Pursuit for Population III Stars in a Ly_alpha Emitter at z=6.33 through HeII Emission
• Early structure formation from primordial density fluctuations with a blue-tilted power spectrum
• A gravitational-wave limit on the Chandrasekhar mass of dark matter
• Magnetic fields in primordial accretion disks
• Implications of inhomogeneous metal mixing for stellar archaeology
• Low-metallicity massive single stars with rotation. II. Predicting spectra and spectral classes of chemically-homogeneously evolving stars
• High Energy neutrino signals from the Epoch of Reionization
• A dearth of young and bright massive stars in the Small Magellanic Cloud
• Magneto-Hydrodynamical Effects on Nuclear Deflagration Fronts in Type Ia Supernovae
• The Metallicity of Pre-Galactic Globular Clusters: Observational consequences of the first stars
• SMBH Seeds from Dissipative Dark Matter
• The earliest galaxies seen in 21 cm line absorption
• Angular momentum and clustering properties of early dark matter halos
• Formation, disruption and energy output of Population III X-ray binaries
• 21-cm signature of the first sources in the Universe: Prospects of detection with SKA
• Distribution of the very first PopIII stars and their relation to bright z~6 quasars
• Exploring a primordial solution for early black holes detected with the JWST
• Star Formation Triggered by Supernova Explosions in Young Galaxies
• Gamma-Ray Bursts are Produced Predominately in the Early Universe
• The impact of thermodynamics on gravitational collapse: filament formation and magnetic field amplification
• The surface carbon and nitrogen abundances in models of ultra metal-poor stars
• Unveiling the contribution of Pop III stars in primeval galaxies at redshift $\ge 6$
• Suppression of accretion onto low-mass Population III stars
• Thermal instability and multi-phase interstellar medium in the first galaxies
• Can Non-Gaussian Cosmological Models Explain the WMAP's High Optical Depth for Reionization?
• The Mutual Interaction Between Population III Stars and Self-Annihilating Dark Matter
• Multi-Dimensional Simulations of Pair-Instability Supernovae
• The X-ray Spectrum of the z=6.30 QSO SDSS J1030+0524
• Radiative effects during the assembly of direct collapse black holes
• Low-energy Population III supernovae and the origin of extremely metal-poor stars
• Rapid Star Formation in the Presence of Active Galactic Nuclei
• Formation of massive stars under protostellar radiation feedback: Very metal-poor stars
• Redshift-dependent galaxy formation efficiency at $z=5-13$ in the FirstLight simulations
• Pop. III stars from turbulent fragmentation at redshift ~ 11
• X-ray Background at High Redshifts from Pop III Remnants: Results from Pop III star formation rates in the Renaissance Simulations
• Formation of Massive and Wide First-star Binaries in Radiation Hydrodynamics Simulations
• X-shooting GRBs at high redshift: probing dust production history
• A new approach to determine optically thick H2 cooling and its effect on primordial star formation
• The Radio Signatures of the First Supernovae
• Counts of high-redshift GRBs as probe of primordial non-Gaussianities
• The fingerprint of binary intermediate mass black holes in globular clusters: supra-thermal stars and angular momentum alignment
• Gemini GMOS--IFU spectroscopy of the compact HII galaxies Tol 0104-388 and Tol 2146-391: The dependence on the properties of the interstellar medium
• A particle dark matter footprint on the first generation of stars
• S-process in low-mass extremely metal-poor stars
• Super-Eddington mass growth of intermediate-mass black holes embedded in dusty circumnuclear disks
• Boosting Lya and HeII 1640A Line Fluxes from Pop III Galaxies: Stochastic IMF Sampling and Departures from Case-B
• Primordial star formation: relative impact of H2 three-body rates and initial conditions
• Circular polarization of the CMB: Foregrounds and detection prospects
• Multifrequency radiation hydrodynamics simulations of H2 line emission in primordial, star-forming clouds
• A smoother end to the dark ages
• Cosmic Renaissance: The First Sources of Light
• A bound on the 12C/13C ratio in near-pristine gas with ESPRESSO
• Constraining Dark Matter properties with the first generation of stars
• Supermassive Black Holes in the Early Universe
• Statistical properties of mass, star formation, chemical content and rotational patterns in early z > 9 structures
• Mass-loss predictions for evolved very metal-poor massive stars
• First star formation in ultra-light particle dark matter cosmology
• Blocking metal accretion onto population III stars by stellar wind
• Upper limits on the mass and luminosity of Population III-dominated galaxies
• Dark Stars: Improved Models and First Pulsation Results
• An Observational Limit on the Earliest GRBs
• History of Hydrogen Reionization in the Cold Dark Matter Model
• The clustering of the first galaxy halos
• Chemical evolution of the intra-cluster medium
• Radiative feedback and cosmic molecular gas: the role of different radiative sources
• The Role of Primordial Kicks on Black Hole Merger Rates
• Massive Black Hole Science with eLISA
• Cosmic infrared background from Population III stars and its effect on spectra of high-z gamma-ray bursts
• Atomic and molecular gas from the epoch of reionization down to redshift 2
• Population III Star Clusters in the Reionized Universe
• Ultrafaint Dwarfs - Star Formation and Chemical Evolution in the Smallest Galaxies
• Gamma-ray bursts and Population III stars
• Rapidly rotating Population III stellar models as a source of primary nitrogen
• Constraining Warm Dark Matter and Pop III stars with the Global 21-cm Signal
• Very Massive Star Models: I. Impact of Rotation and Metallicity and Comparisons with Observations
• Magnetohydrodynamic effect on first star formation: prestellar core collapse and protostar formation
• Seeding the second star -- II. CEMP star formation enriched from faint supernovae
• Loss cone: past, present and future
• Gravitational Wave Signal from Assembling the Lightest Supermassive Black Holes
• The implications of dust for high-redshift protogalaxies and the formation of binary disks
• Dark matter powered stars: Constraints from the extragalactic background light
• The role of the H${}_2$ adiabatic index in the formation of the first stars
• Molecular Chemistry for Dark Matter II: Recombination, Molecule Formation, and Halo Mass Function in Atomic Dark Matter
• Radiative feedback and cosmic molecular gas: numerical method
• Formation Criteria and the Mass of Secondary Population III Stars
• Very Massive Stars (VMS) in the Local Universe
• Self-enrichment of Galactic halo globular clusters: stimulated star formation and consequences for the halo metallicity distribution
• Impact of an accurate modeling of primordial chemistry in high resolution studies
• The Polytropic Equation of State of Primordial Gas Clouds
• Amplification of turbulence in contracting prestellar cores in primordial minihalos
• Studying Cosmic Dawn using redshifted HI 21-cm signal: A brief review
• Deep learning approach for identification of HII regions during reionization in 21-cm observations -- II. foreground contamination
• Transition probabilities of Co II, weak lines to the ground and low metastable levels
• Primordial star formation triggered by UV photons from UHECR
• Jet-powered supernovae of $\sim 10^5{M}_{\odot }$ population III stars are observable by $Euclid$, $WFIRST$, $WISH$, and $JWST$
• Impacts of Dark Stars on Reionization and Signatures in the Cosmic Microwave Background
• Hot Cores : Probes of High-Redshift Galaxies
• The 21-cm forest as a simultaneous probe of dark matter and cosmic heating history
• On the spin-temperature evolution during the epoch of reionization
• Fragmentation in Dusty Low-Metallicity Star Forming Halos
• Can the 21 cm signal probe Population III and II star formation?
• Observing the First Stars and Black Holes
• Radiative Feedback in Relic HII Regions at High-Redshift
• Is GRB 050904 at z=6.3 absorbed by dust?
• Probing Population III Initial Mass Functions with He II/H$\alpha$ Intensity Mapping
• Where can we really find the First Stars' Remnants today?
• The Thermodynamics of Molecular Cloud Fragmentation: Star Formation Under Non-Milky Way Conditions
• Multicomponent multiscatter capture of Dark Matter
• Dark-matter halo mergers as a fertile environment for low-mass Population III star formation
• Long gamma-ray burst rate at very high redshift
• The Formation and Evolution of the First Massive Black Holes
• The clustering properties of the first galaxies
• Effects of turbulence and rotation on protostar formation as a precursor to seed black holes
• Formation of Compact Stellar Clusters by High-Redshift Galaxy Outflows I: Nonequillibrium Coolant Formation
• Chemical constraints on the contribution of Population III stars to cosmic reionization
• Stochastic background of gravitational waves generated by pre-galactic black holes
• Globular Cluster Formation in the Virgo Cluster
• Baryon-dark matter scattering and first star formation
• Cold accretion in early galaxy formation and its Lyman-alpha signatures
• High Energy Neutrino Emission from the Earliest Gamma-Ray Bursts
• The early growth of supermassive black holes in cosmological hydrodynamic simulations with constrained Gaussian realizations
• Dark Stars Powered by Self-Interacting Dark Matter
• Detection and Fundamental Applications of Individual First Galaxies
• The imprint of the cosmic supermassive black hole growth history on the 21 cm background radiation
• Black Holes in our Galactic Halo: Compatibility with FGST and PAMELA Data and Constraints on the First Stars
• Do the environmental conditions affect the dust-induced fragmentation in low-metallicity clouds ?: Effect of pre-ionization and far-ultraviolet/cosmic-ray fields
• First supernovae in dwarf protogalaxies
• Distinctive 21 cm structures of the first stars, galaxies, and quasars
• Local Group star formation in warm and self-interacting dark matter cosmologies
• Growth of Massive Disk and Early Disk Fragmentation in the Primordial Star Formation
• The First Galaxies and the Likely Discovery of their Fossils in the Local Group
• Extremely-Metal Poor Stars in the Milky Way: A Second Generation Formed after Reionization
• Timescales for Low-Mass Star Formation in Extragalactic Environments: Implications for the Stellar IMF
• Conditions for HD Cooling in the First Galaxies Revisited: Interplay between Far-Ultraviolet and Cosmic Ray Feedback in Population III Star Formation
• Photometric Properties of the Most Massive High-Redshift Galaxies
• Stellar evolution of massive stars at very low metallicities
• Fates of the oldest intermediate-mass stars - Primordial to Extremely Metal-Poor AGB and Super-AGB Stars: White Dwarf or Supernova progenitors
• Probing the High-Redshift Universe with SPICA: Toward the Epoch of Reionization and Beyond
• The complexity that the first stars brought to the Universe: Fragility of metal enriched gas in a radiation field
• Ionizing photon production of Population III stars: effects of rotation, convection, and initial mass function
• How much radioactive nickel does ASASSN-15lh require?
• Global 21-cm Cosmology from the Farside of the Moon
• Triggering the Formation of Halo Globular Clusters with Galaxy Outflows
• A practical guide to the massive black hole cosmic history
• Cosmological Impact of Population III Binaries
• The nonlinear evolution of baryonic overdensities in the early universe: Initial conditions of numerical simulations
• Modelling Population III stars for semi-numerical simulations
• Non-ideal magnetohydrodynamic simulations of the first star formation: the effect of ambipolar diffusion
• On the operation of the chemothermal instability in primordial star-forming clouds
• Dark Stars: A New Study of the FIrst Stars in the Universe
• Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars
• The First Stars: formation under cosmic ray feedback
• Observing H2 Emission in Forming Galaxies
• A hide-and-seek game: Looking for Population III stars during the Epoch of Reionization through the HeII$\lambda$1640 line
• Possible Evolution of Supermassive Black Holes from FRI quasars
• Implications of primordial black holes on the first stars and the origin of the super--massive black holes
• The stochastic enrichment of Population II stars
• Can Population III stars be major origins of both merging binary black holes and extremely metal poor stars?
• Sources for Metals in the Intergalactic Medium
• Role of primordial black holes in the direct collapse scenario of supermassive black hole formation at high redshifts
• Metal-enriched Galaxies in the First ~1 Billion Years: Evidence of a Smooth Metallicity Evolution at z ~ 5
• A possible bright ultraviolet flash from a galaxy at redshift z ~ 11
• The Reionization History and Early Metal Enrichment inferred from the Gamma-Ray Burst Rate
• High-Entropy Polar Regions Around the First Protostars
• The Supersonic Project: To cool or not to cool Supersonically Induced Gas Objects (SIGOs)?
• Constraining Very High Mass Population III Stars through He II Emission in Galaxy BDF-521 at z = 7.01
• First stars as a possible origin for the helium-rich population in omega Centauri
• Metal Pollution of Low-Mass Population III Stars through Accretion of Interstellar Objects like `Oumuamua
• Gamma-ray bursts as X-ray depth-gauges of the Universe
• Multiscale mass transport in z~6 galactic discs: fueling black holes
• Tomography of the Reionization Epoch with Multifrequency CMB Observations
• Metal enrichment signatures of the first stars on high-z DLAs
• Effect of lithium hydride on the cooling of primordial gas
• The First Billion Years in Seconds: An Effective Model for the 21-cm Signal with Population III Stars
• Star forming filaments in warm dark matter models
• Photoevaporation of Minihalos during Cosmic Reionization: Primordial and Metal-Enriched Halos
• Effect of Population III Multiplicity on Dark Star Formation
• The effect of dark matter resolution on the collapse of baryons in high redshift numerical simulations
• Formation of Compact Stellar Clusters by High-Redshift Galaxy Outflows II: Effect of Turbulence and Metal-Line Cooling
• Simulating a White Dwarf-dominated Galactic Halo
• Evolution and Nucleosynthesis of Very Massive Stars
• Evolution of the First Supernovae in Protogalaxies: Dynamics of Mixing of Heavy Elements
• Vibrational instability of Population III very massive main-sequence stars due to the $\epsilon$-mechanism
• Impact of Rotation on Neutrino Emission and Relic Neutrino Background from Population III Stars
• The Impact of Molecular Hydrogen Cooling on the Galaxy Formation Threshold
• A Pilot Search for Population III Supernova Candidates in the Spitzer/IRAC Dark Field
• Source Mergers and Bubble Growth During Reionization
• Chemical Composition of the Early Universe
• Fragmentation in Population III Galaxies formed through Ionizing Radiation
• Enhanced Detectability of Pre-reionization 21-cm Structure
• Feedback Effects of First Supernovae on the Neighboring Dark Matter Halos
• The Evolution of Accreting Population III Stars at 10${}^{-6}$-10${}^3$ M${}_{\odot }$/yr
• Radiative feedback from ionized gas
• The physical origin of super-competitive accretion during the formation of the first supermassive black holes
• Accretion onto Intermediate-mass Seed Black Holes in Primordial Galaxies
• Supernova explosions in magnetized, primordial dark matter halos
• Computation of Fluid Flows in Non-inertial Contracting, Expanding, and Rotating Reference Frames
• The Evolution of Population III and Extremely Metal-Poor Binary Stars
• The influence of ultra-high-energy cosmic rays on star formation in the early universe
• Supermassive Star Formation in Magnetized Atomic-Cooling Gas Clouds: Enhanced Accretion, Intermittent Fragmentation, and Continuous Mergers
• Stellar mass dependence of the 21-cm signal around the first star and its impact on the global signal
• H_2 Line Emission Associated with the Formation of the First Stars
• Formation of First Galaxies inside Density Peaks and Voids under the Influence of Dark Matter-Baryon Streaming Velocity, I: Initial Condition and Simulation Scheme
• Formation of multiple low mass stars, brown dwarfs and planemos via gravitational collapse
• The high-redshift tail of stellar reionization in LCDM is beyond the reach of the low-$\ell$ CMB
• Neutralino Annihilations and the Gas Temperature in the Dark Ages
• Modeling the survival of Population III stars till present day
• The earliest phases of CNO enrichment in galaxies
• Physics of Superluminous Supernovae
• Hadronic Interactions of Energetic Charged Particles in Protogalactic Outflow Environments and Implications for the Early Evolution of Galaxies
• Cosmic history of integrated galactic stellar initial mass function : a simulation study
• The End of an Era - The Population III to Population II Transition and the Near Infrared Background
• Massive open star clusters using the VVV survey IV. WR 62-2, a new very massive star in the core of the VVV CL041 cluster
• Primordial protostars accreting beyond the $\Omega \Gamma$-limit: radiation effect around the star-disk boundary
• A Search for Metal-poor Stars Pre-enriched by Pair-instability Supernovae I. A Pilot Study for Target Selection from Sloan Digital Sky Survey (SDSS)
• Multiscatter capture of superheavy dark matter by Pop. III stars
• If dark matter is fuzzy, the first stars form in massive pancakes
• Premature Black Hole Death of Population III Stars by Dark Matter
• The extent of intergalactic metal enrichment from galactic winds during the Cosmic Dawn
• The role of 3-body H${}_2$ formation in the fragmentation of primordial gas
• Dark Exoplanets
• The Chemical Evolution of Iron-Peak Elements with Hypernovae
• Signatures of very massive stars: supercollapsars and their cosmological rate
• Effect of interstellar objects on metallicity of low-mass first stars formed in a cosmological model
• Gamma-ray bursts from massive Population III stars: clues from the radio band
• Single-Pass GPU-Raycasting for Structured Adaptive Mesh Refinement Data
• Multi-Resolution Radiative Transfer for Line Emission
• Consequences of cosmic microwave background-regulated star formation
• Shape and Spin of Minihaloes. II: The Effect of Streaming Velocities
• Dark Matter Annihilation in the Circumgalactic Medium at High Redshifts
• Metal-Poor Stars Observed with the Southern African Large Telescope II. An Extended Sample
• Extending Semi-numeric Reionisation Models to the First Stars and Galaxies
• A Study of Primordial Very Massive Star Evolution. II. Stellar Rotation and Gamma-Ray Burst Progenitors
• Direct Collapse to Supermassive Black Hole Seeds: Comparing the AMR and SPH Approaches
• Formation and Radiative Feedback of First Objects and First Galaxies
• Impact of Magnetic Braking on High-mass Close Binary Formation
• The properties of primordially-seeded black holes and their hosts in the first billion years: implications for JWST
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• Magnetic fields during high redshift structure formation
• Can very massive stars avoid Pair-Instability Supernovae?
• Collision-induced mass loss and mass gain on an extremely massive star. An analytical approach and a static proto-globular cluster test-case
• Upper Bound on the First Star Formation History
• Formation of mini-galaxies in defunct cosmological HII regions
• Fragmentation of Primordial Filamentary Clouds under Far-Ultraviolet Radiation
• First Star Formation in the Presence of Primordial Magnetic Fields
• Detectability of Local Group Dwarf Galaxy Analogues at High Redshifts
• Colour gradients in cluster ellipticals at z~1.4: the hidden content of the galaxy central regions
• Nucleosynthetic yields of intermediate-mass primordial to extremely metal-poor stars
• Some First Stars Were Red: Detecting Signatures of Massive Population III Formation Through Long-Term Stochastic Color Variations
• The Science Case for PILOT II: the Distant Universe
• Classifying binary black holes from Population III stars with the Einstein Telescope: A machine-learning approach
• Stability Analysis of Strange-Modes in Hot Massive Stars with Time-Dependent Convection
• On the population of primordial star clusters in the presence of UV background radiation
• Relaxation leptogenesis, isocurvature perturbations, and the cosmic infrared background
• Driving Conditions of Protostellar Outflows in Different Star-Forming Environments
• Extremely Metal-Poor Stars and a Hierarchical Chemical Evolution Model
• Discrimination of heavy elements originating from Pop III stars in z = 3 intergalactic medium
• Do fragmentation and accretion affect the stellar Initial Mass Function?
• The effects of population III stars on the chemical and photometrical evolution of ellipticals
• Isocurvature Fluctuations Induce Early Star Formation
• J1342+0928 Supports the Timeline in the R_h=ct Cosmology
• Formation of Compact Stellar Clusters by High-Redshift Galaxy Outflows III: Observability and Connection to Halo Globular Clusters
• Amplification of Magnetic Fields in a Primordial HII Region and Supernova
• On the effects of rotation in primordial star-forming clouds
• Dark Cosmology: Investigating Dark Matter & Exotic Physics in the Dark Ages using the Redshifted 21-cm Global Spectrum
• Relics of metal-free low mass stars exploding as thermonuclear supernovae
• A Lunar Farside Low Radio Frequency Array for Dark Ages 21-cm Cosmology
• Does the chemothermal instability have any role in the fragmentation of primordial gas
• Let there be Light: the Emergence of Structure out of the Dark Ages in the Early Universe
• Galaxy Formation and Symbiotic Evolution with the Inter-Galactic Medium in the Age of ELT-ANDES
• Astrophysics: Most distant cosmic blast seen
• A new model for the origin of very metal poor stars and their chemical composition
• Aeos: Transport of Metals from Minihalos following Population III Stellar Feedback
• The Luminosity of Population III Star Clusters
• Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos
• Pair-Instability Supernovae of Fast Rotating Stars
• Formation of supermassive stars in the first stellar clusters: Dependence on the gas temperature
• Does the structure of Pop III supernova ejecta affect the elemental abundance of extremely metal-poor stars?
• Coronal Properties of Low-mass Population III Stars and the Radiative Feedback in the Early Universe
• Contribution of the first galaxies to the cosmic far-infrared/sub-millimeter background - I. Mean background level
• Gravitational Wave Sources from Pop III Stars are Preferentially Located within the Cores of their Host Galaxies
• Formation of First Stars Triggered by Collisions and Shockwaves: Prospect for High Star Formation Efficiency and High Ionizing Photon Escape Fraction
• Astrophysics with the Laser Interferometer Space Antenna
• The chemical evolution of self-gravitating primordial disks
• Over-cooled haloes at z > 10: a route to form low-mass first stars
• The Growth of Baryonic Structure in the Presence of Cosmological Magnetic Pressure
• Population III.1 stars: formation, feedback and evolution of the IMF
• Open questions in the study of population III star formation
• Neutrino point source searches for dark matter spikes
• Stochastic microhertz gravitational radiation from stellar convection
• Reionization in the Light of Dark Stars
• Non-grey hydrogen burning evolution of sub-Solar mass Population III stars
• Formation of the First Galaxies: Theory and Simulations
• Effects of a burst of formation of first-generation stars on the evolution of galaxies
• Signatures of Population III supernovae at Cosmic Dawn: the case of GN-z11-flash
• Probing baryonic processes and gastrophysics in the formation of the Milky Way dwarf satellites: I. metallicity distribution properties
• Fast and accurate parameter estimation of high-redshift sources with the Einstein Telescope
• The Chemistry of the Early Universe
• Collapse of Primordial Filamentary Clouds under Far-Ultraviolet Radiation
• The near-infrared radiation background, gravitational wave background and star formation rate of Pop III and Pop II during cosmic reionization
• Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
• Temporal Self-Organization in Galaxy Formation
• First Stars. I. Evolution without mass loss
• Spectral Signatures of Population III and Envelope-stripped Stars in Galaxies at the Epoch of Reionization
• Ionization degree and magnetic diffusivity in star-forming clouds with different metallicities
• Upper Limit on Star Formation and Metal Enrichment in Minihalos
• Globular Cluster formation in a collapsing supershell
• Chemical Evolution of the Juvenile Universe
• An extremely metal-poor Lyman $\alpha$ emitter candidate at $z=6$ revealed through absorption spectroscopy
• Kickstarting Reionization with the First Black Holes: the effects of second-order perturbation theory in pre-reionization volumes
• Growth of Light Seed Black Holes in the Early Universe
• Does slow and steady win the race? Investigating feedback processes in giant molecular clouds
• Radiation Hydrodynamical Instabilities in Cosmological and Galactic Ionization Fronts
• Formation of Compact Clusters from High Resolution Hybrid Cosmological Simulations
• Evolution of Star Cluster Within Galaxy using Self-consistent Hybrid Hydro/N-body Simulation
• Simulating the collapse of rotating primordial gas clouds to study the survival possibility of Pop III protostars
• Condition for low-mass star formation in shock-compressed metal-poor clouds
• Supernovae at the cosmic dawn
• Metal Enrichment of the Intergalactic Medium and Production of Massive Black Holes
• Angular momentum distribution during the collapse of primordial star-forming clouds
• Rydberg States of H${}_3$ and HeH as Potential Coolants for Primordial Star Formation
• Probing the Growth of Massive Black Holes with Black Hole-Host Galaxy Spin Correlations
• First Light: A Brief Review
• The Small Magellanic Cloud through the lens of the James Webb Space Telescope : binaries and mass function within the galaxy outskirts
• The star formation history inferred from long gamma-ray bursts with high pseudo-redshifts
• Revisiting the statistical equilibrium of H${}^{-}$ in stellar atmospheres
• Diversity of the Lyman continuum escape fractions of high-$z$ galaxies and its origins
• Impact of Population III stars on the astrophysical gravitational-wave background
• The Impact of AMR in Numerical Astrophysics and Cosmology
• Searching for Low-mass Population III Stars Disguised as White Dwarfs
• Detectability of Population III stellar remnants as X-ray binaries from tidal captures in the local Universe
• Radiation magnetohydrodynamics simulations of Population III star formation during the Epoch of Reionization
• Luminosity Bias (II): The Cosmic Web of the First Stars
• Aeos: The Impact of Population III Initial Mass Function and Star-by-Star Models in Galaxy Simulations
• Low-temperature primordial gas in merging halos
• Biermann Mechanism in Primordial Supernova Remnant and Seed Fields
• Formation and Evolution of Supermassive Black Holes
• Understanding the IMF
• The Reionization History in the Lognormal Model
• Slow Cooling in Low Metallicity Clouds: An Origin of Globular Cluster Bimodality?
• Population III Supernovae and the Assembly of the First Galaxies
• The mass-function of primordial star clusters
• Supermassive Dark Stars and their remnants as a possible solution to three recent cosmic dawn puzzles
• Helium reionization in the presence of self-annihilating clumpy dark matter
• First Stars. II. Evolution with mass loss
• Black hole merger rates for LISA and LGWA from semi-analytical modelling of light seeds
• The Evolution of the Hubble Sequence: morpho-kinematics of distant galaxies
• The First Stars
• Dark Stars: Dark Matter in the First Stars leads to a New Phase of Stellar Evolution
• Very Massive Close Binaries and the Puzzling Temporal Evolution of 14N in the Solar Neighbourhood
• The first stars
• Generation of strong magnetic fields via the small-scale dynamo during the formation of the first stars
• Neural-Network Chemical Emulator for First-Star Formation: Robust Iterative Predictions over a Wide Density Range
• Impact of Gravitational Slingshot of Dark Matter on Galactic Halo Profiles
• Observing the influence of growing black holes on the pre-reionization IGM
• A test of Ca ii H & K photometry for isolating massive globular clusters below the metallicity floor
• The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES
• The Numerical Simulation of Turbulence
• Quantifying Element Importance for Mass Recovery from Population III Supernova Yield Fits
• Massive star clusters detected by JWST as natural birth places to form intermediate-mass black holes
• A new model of quasar mass evolution
• The Baryon Budget of Galaxies across the First Billion Years
• Nucleosynthesis in the Cosmos: What we think we know and forthcoming questions
• First Light: Switching on Stars at the Dawn of Time
• Powerful explosions at Z=0 ?
• The Impact of a Supernova Explosion in a Very Massive Binary
• Interstellar Chemistry: Radiation, Dust and Metals
• Can UVB variations reconcile simulated quasar absorption lines at high redshift?
• Formation and early evolution of massive black holes
• The star formation process in the Magellanic Clouds
• Discovering Supernovae at Epoch of Reionization with Nancy Grace Roman Space Telescope
• The Effect of Environment on Massive Star Formation
• Scaling Relations Between Low-mass Black Holes and Their Host Galaxies
• It's Always Darkest Before the Cosmic Dawn: Early Results from Novel Tools and Telescopes for 21 cm Cosmology
• The role of gas fragmentation during the formation of supermassive black holes
• Studying The Effect of Radiation Pressure on Evolution of a Population III Stellar Cluster
• Formation of Stellar Clusters and the Importance of Thermodynamics for Fragmentation
• Multidimensional Simulations of Thermonuclear Supernovae from the First Stars
• From Dark Matter Minihalos to Large-Scale Radiative Feedback: A Self-Consistent 3D Simulation of the First Stars and Galaxies using Neural Networks