A Systematic Survey of the Effects of Wind Mass Loss Algorithms on the Evolution of Single Massive Stars

Abstract

Mass loss is a key uncertainty in the evolution of massive stars. Stellar evolution calculations must employ parametric algorithms for mass loss, and usually only include stellar winds. We carry out a parameter study of the effects of wind mass loss on massive star evolution using the open-source stellar evolution code MESA. We provide a systematic comparison of wind mass loss algorithms for solar-metallicity, nonrotating, single stars in the initial mass range of $15-35M_{\odot }$. We consider combinations drawn from two hot phase algorithms, three cool phase algorithms, and two Wolf-Rayet algorithms. We consider linear wind efficiency scale factors of $1$, $0.33$, and $0.1$ to account for reductions in mass loss rates due to wind inhomogeneities. We find that the initial to final mass mapping for each zero-age main-sequence (ZAMS) mass has a $\sim 50\%$ uncertainty if all algorithm combinations and wind efficiencies are considered. The ad-hoc efficiency scale factor dominates this uncertainty. While the final total mass and internal structure of our models vary tremendously with mass loss treatment, final observable parameters are much less sensitive for ZAMS mass $\lesssim 30M_{\odot }$. This indicates that uncertainty in wind mass loss does not negatively affect estimates of the ZAMS mass of most single-star supernova progenitors from pre-explosion observations. Furthermore, we show that the internal structure of presupernova stars is sensitive to variations in both main sequence and post main-sequence mass loss. We find that the compactness parameter $\xi \propto M/R(M)$ varies by as much as $30\%$ for a given ZAMS mass evolved with different wind efficiencies and mass loss algorithm combinations. [abridged]

arXiv commentAccepted for publication on A&A, 22 pages + 2 appendixes, 12 figures, online input parameters available at https://stellarcollapse.org/renzo2017 and data at https://zenodo.org/record/292924#.WK0q2tWi6Wg

References in corpus (79)

• Modules for Experiments in Stellar Astrophysics (MESA)
• Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
• Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions
• Binary interaction dominates the evolution of massive stars
• Mass-loss predictions for O and B stars as a function of metallicity
• Progenitors of core-collapse supernovae
• Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
• Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars
• Compact Remnant Mass Function: Dependence on the Explosion Mechanism and Metallicity
• Physical Properties of Wolf-Rayet Stars
• Pre-Supernova Evolution of Massive Single and Binary Stars
• Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields
• Astrophysical Implications of the Binary Black-Hole Merger GW150914
• The death of massive stars - I. Observational constraints on the progenitors of type II-P supernovae
• Black Hole Formation in Failing Core-Collapse Supernovae
• Pulsational Pair-Instability Supernovae
• Nucleosynthesis and Remnants in Massive Stars of Solar Metallicity
• Mass loss from hot massive stars
• On The Maximum Mass of Stellar Black Holes
• The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 Msun stellar mass limit
• The High Angular Resolution Multiplicity of Massive Stars
• Observed Fractions of Core-Collapse Supernova Types and Initial Masses of their Single and Binary Progenitor Stars
• Progenitor-Explosion Connection and Remnant Birth Masses for Neutrino-Driven Supernovae of Iron-Core Progenitors
• Stellar evolution with rotation X: Wolf-Rayet star populations at solar metallicity
• The nucleosynthesis of Al26 and Fe60 in solar metallicity stars extending in mass from 11 to 120 Msun: the hydrostatic and explosive contributions
• Type Ib/c supernovae in binary systems I. Evolution and properties of the progenitor stars
• An empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich Asymptotic Giant Branch stars
• On the role of continuum-driven eruptions in the evolution of very massive stars and Population III stars
• A two-parameter criterion for classifying the explodability of massive stars by the neutrino-driven mechanism
• The Discordance of Mass-Loss Estimates for Galactic O-Type Stars
• Wave-Driven Mass Loss in the Last Year of Stellar Evolution: Setting the Stage for the Most Luminous Core-Collapse Supernovae
• A spectroscopic survey on the multiplicity of high-mass stars
• The Progenitors of Core-Collapse Supernovae
• The Compactness of Presupernova Stellar Cores
• Toward Complete Statistics of Massive Binary Stars: Penultimate Results from the Cygnus OB2 Radial Velocity Survey
• Low mass loss rates in O-type stars: Spectral signatures of dense clumps in the wind of two Galactic O4 stars
• Preparing for an Explosion: Hydrodynamic Instabilities and Turbulence in Presupernovae
• Very Low Energy Supernovae from Neutrino Mass Loss
• Flash Spectroscopy: Emission Lines from the Ionized Circumstellar Material around $<10$-Day-Old Type II Supernovae
• $s$-process production in rotating massive stars at solar and low metallicities
• Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit
• The evolution of runaway stellar collision products
• The mass-loss rates of red supergiants and the de Jager prescription
• Setting the Stage for Circumstellar Interaction in Core-Collapse Supernovae II: Wave-Driven Mass Loss in Supernova Progenitors
• The Role of Turbulence in Neutrino-Driven Core-Collapse Supernova Explosions
• Type II-Plateau supernova radiation: dependencies on progenitor and explosion properties
• Revised Stellar Temperatures for Magellanic Cloud O Supergiants from FUSE and VLT-UVES Spectroscopy
• Ejection of the massive Hydrogen-rich envelope timed with the collapse of the stripped SN2014C
• Luminous Blue Variables are Antisocial: Their Isolation Implies that they are Kicked Mass Gainers in Binary Evolution
• Neutron star kicks by the gravitational tug-boat mechanism in asymmetric supernova explosions: progenitor and explosion dependence
• Sub-Inertial Gravity Modes in the B8V Star KIC 7760680 Reveal Moderate Core Overshooting and Low Vertical Diffusive Mixing
• Natal Kicks of Stellar-Mass Black Holes by Asymmetric Mass Ejection in Fallback Supernovae
• The evolution of massive stars and their spectra I. A non-rotating 60 Msun star from the zero-age main sequence to the pre-supernova stage
• The Progenitor Dependence of the Preexplosion Neutrino Emission in Core-Collapse Supernovae
• An Updated Look at Binary Characteristics of Massive Stars in the Cygnus OB2 Association
• The Tarantula Massive Binary Monitoring: I. Observational campaign and OB-type spectroscopic binaries
• Yellow supergiants as supernova progenitors: an indication of strong mass loss for red supergiants?
• Implications of the metallicity dependence of Wolf-Rayet winds
• The impact of mass-loss on the evolution and pre-supernova properties of red supergiants
• On Variations Of Pre-Supernova Model Properties
• Silicon Burning I: Neutronization and the Physics of Quasi-Equilibrium
• Massive star evolution: Luminous Blue Variables as unexpected Supernova progenitors
• Super-Eddington Stellar Winds Driven by Near-Surface Energy Deposition
• Beyond Mixing-length Theory: a step toward 321D
• Magnetic massive stars as progenitors of "heavy" stellar-mass black holes
• The VLT-FLAMES Tarantula Survey III: A very massive star in apparent isolation from the massive cluster R136
• Quantitative studies of the Far-UV, UV and optical spectra of late O and early B-type supergiants in the Magellanic Clouds
• 2D Simulations of the Line-Driven Instability in Hot-Star Winds: II. Approximations for the 2D Radiation Force
• A new prescription for the mass-loss rates of WC and WO stars
• Luminous and Variable Stars in M31 and M33. III. The Yellow and Red Supergiants and Post-Red Supergiant Evolution
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• Convective Properties of Rotating Two-Dimensional Core-Collapse Supernova Progenitors
• Probing Final Stages of Stellar Evolution with X-Ray Observations of SN 2013ej
• On the observability of bow shocks of Galactic runaway OB stars
• Key Issues Review: Numerical studies of turbulence in stars
• Population I Wolf-Rayet Runaway Stars: the Case of WR124 and its Expanding Nebula M1-67
• Physics of mass loss in massive stars
• Can very massive stars avoid Pair-instability Supernovae?
• The advanced stages of stellar evolution: impact of mass loss, rotation, and link with B[e] stars

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