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Title: Effects of axions on Population III stars

Abstract

Following the renewed interest in axions as a dark matter component, we revisit the effects of energy loss by axion emission on the evolution of the first generation of stars. These stars with zero metallicity are assumed to be massive, more compact, and hotter than subsequent generations. It is hence important to extend previous studies, which were restricted to solar metallicity stars. Here, our analysis first compares the evolution of solar metallicity 8, 10, and 12 M stars to previous work. We then calculate the evolution of 8 zero-metallicity stars with and without axion losses and with masses ranging from 20 to 150 M. For the solar metallicity models, we confirm the disappearance of the blue-loop phase for a value of the axion-photon coupling of g = 10-10 GeV-1. We show that for g = 10-10 GeV-1, the evolution of Population III stars is not much affected by axion losses, except within the range of masses 80–130 M. Such stars show significant differences in both their tracks within the Tc–ρc diagram and their central composition (in particular 20Ne and 24Mg). We discuss the origin of these modifications from the stellar physics point of view, and also their potential observational signatures.

Authors:
 [1];  [2];  [1];  [3];  [4];  [5]
  1. Univ. of Geneva, Sauverny (Switzerland). Geneva Observatory
  2. Univ. Paris-Saclay, Orsay (France). Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM)
  3. Univ. of Minnesota, Minneapolis, MN (United States). School of Physics and Astronomy, William I. Fine Theoretical Physics Inst.
  4. Univ. Pierre et Marie Curie, Paris (France). Inst. d'Astrophysique de Paris; Sorbonne Univ., Paris (France). Inst. Lagrange de Paris
  5. Univ. Pierre et Marie Curie, Paris (France). Inst. d'Astrophysique de Paris; Sorbonne Univ., Paris (France). Inst. Lagrange de Paris
Publication Date:
Research Org.:
Univ. of Minnesota, Minneapolis, MN (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1535275
Grant/Contract Number:  
SC0011842
Resource Type:
Accepted Manuscript
Journal Name:
Astronomy and Astrophysics
Additional Journal Information:
Journal Volume: 605; Journal ID: ISSN 0004-6361
Publisher:
EDP Sciences
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; astronomy & astrophysics; elementary particles; star evolution; Population III; massive stars

Citation Formats

Choplin, Arthur, Coc, Alain, Meynet, Georges, Olive, Keith A., Uzan, Jean-Philippe, and Vangioni, Elisabeth. Effects of axions on Population III stars. United States: N. p., 2017. Web. doi:10.1051/0004-6361/201731040.
Choplin, Arthur, Coc, Alain, Meynet, Georges, Olive, Keith A., Uzan, Jean-Philippe, & Vangioni, Elisabeth. Effects of axions on Population III stars. United States. https://doi.org/10.1051/0004-6361/201731040
Choplin, Arthur, Coc, Alain, Meynet, Georges, Olive, Keith A., Uzan, Jean-Philippe, and Vangioni, Elisabeth. Mon . "Effects of axions on Population III stars". United States. https://doi.org/10.1051/0004-6361/201731040. https://www.osti.gov/servlets/purl/1535275.
@article{osti_1535275,
title = {Effects of axions on Population III stars},
author = {Choplin, Arthur and Coc, Alain and Meynet, Georges and Olive, Keith A. and Uzan, Jean-Philippe and Vangioni, Elisabeth},
abstractNote = {Following the renewed interest in axions as a dark matter component, we revisit the effects of energy loss by axion emission on the evolution of the first generation of stars. These stars with zero metallicity are assumed to be massive, more compact, and hotter than subsequent generations. It is hence important to extend previous studies, which were restricted to solar metallicity stars. Here, our analysis first compares the evolution of solar metallicity 8, 10, and 12 M⊙ stars to previous work. We then calculate the evolution of 8 zero-metallicity stars with and without axion losses and with masses ranging from 20 to 150 M⊙. For the solar metallicity models, we confirm the disappearance of the blue-loop phase for a value of the axion-photon coupling of gaγ = 10-10 GeV-1. We show that for gaγ = 10-10 GeV-1, the evolution of Population III stars is not much affected by axion losses, except within the range of masses 80–130 M⊙. Such stars show significant differences in both their tracks within the Tc–ρc diagram and their central composition (in particular 20Ne and 24Mg). We discuss the origin of these modifications from the stellar physics point of view, and also their potential observational signatures.},
doi = {10.1051/0004-6361/201731040},
journal = {Astronomy and Astrophysics},
number = ,
volume = 605,
place = {United States},
year = {Mon Sep 18 00:00:00 EDT 2017},
month = {Mon Sep 18 00:00:00 EDT 2017}
}

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Works referenced in this record:

Effects of axions on nucleosynthesis in massive stars
journal, September 2015


Pulsational Pair-instability Supernovae
journal, February 2017


The not-so-harmless axion
journal, January 1983


Constraints on axions from SN 1987A
journal, March 1988


Supersymmetric relics from the big bang
journal, June 1984


Cosmology of the invisible axion
journal, January 1983


Grids of stellar models with rotation: I. Models from 0.8 to 120 
journal, January 2012


Can confinement ensure natural CP invariance of strong interactions?
journal, April 1980


Constraint on the Photino Mass from Cosmology
journal, May 1983


Problem of Strong P and T Invariance in the Presence of Instantons
journal, January 1978


A simple solution to the strong CP problem with a harmless axion
journal, August 1981


Early Supernovae Light Curves Following the Shock Breakout
journal, November 2010


Stellar evolution with rotation. VII.: Low metallicity models and the blue to red supergiant ratio in the SMC
journal, July 2001


Revisiting the Bound on Axion-Photon Coupling from Globular Clusters
journal, November 2014


Neon Abundances in B Stars of the Orion Association: Solving the Solar Model Problem?
journal, August 2006

  • Cunha, Katia; Hubeny, Ivan; Lanz, Thierry
  • The Astrophysical Journal, Vol. 647, Issue 2
  • DOI: 10.1086/507301

Constraints imposed by CP conservation in the presence of pseudoparticles
journal, September 1977


Supersymmetric dark matter after LHC run 1
journal, October 2015


Multiple-scattering suppression of the bremsstrahlung emission of neutrinos and axions in supernovae
journal, November 1991


A Two-Parameter Criterion for Classifying the Explodability of Massive Stars by the Neutrino-Driven Mechanism
journal, February 2016


Zero-metallicity stars: II. Evolution of very massive objects with mass loss
journal, February 2003


CP Conservation in the Presence of Pseudoparticles
journal, June 1977


Bounds on hadronic axions from stellar evolution
journal, October 1987


Neutrino energy loss in stellar interiors. III - Pair, photo-, plasma, and bremsstrahlung processes
journal, April 1989

  • Itoh, Naoki; Adachi, Tomoo; Nakagawa, Masayuki
  • The Astrophysical Journal, Vol. 339
  • DOI: 10.1086/167301

Mass-loss predictions for O and B stars as a function of metallicity
journal, April 2001

  • Vink, Jorick S.; de Koter, A.; Lamers, H. J. G. L. M.
  • Astronomy & Astrophysics, Vol. 369, Issue 2
  • DOI: 10.1051/0004-6361:20010127

Fresh look at axions and SN 1987A
journal, August 1997

  • Keil, Wolfgang; Janka, Hans-Thomas; Schramm, David N.
  • Physical Review D, Vol. 56, Issue 4
  • DOI: 10.1103/PhysRevD.56.2419

Red giant bound on the axion-electron coupling reexamined
journal, February 1995


Updated constraints on axions from SN1987A
journal, March 1989


Astrophysical constraints on the couplings of axions, majorons, and familons
journal, January 1986

  • Dearborn, David S. P.; Schramm, David N.; Steigman, Gary
  • Physical Review Letters, Vol. 56, Issue 1
  • DOI: 10.1103/PhysRevLett.56.26

The Nucleosynthetic Signature of Population III
journal, March 2002

  • Heger, A.; Woosley, S. E.
  • The Astrophysical Journal, Vol. 567, Issue 1
  • DOI: 10.1086/338487

Astrophysical axion bounds diminished by screening effects
journal, February 1986


Astrophysical methods to constrain axions and other novel particle phenomena
journal, December 1990


Type II-Plateau supernova radiation: dependences on progenitor and explosion properties
journal, June 2013

  • Dessart, Luc; Hillier, D. John; Waldman, Roni
  • Monthly Notices of the Royal Astronomical Society, Vol. 433, Issue 2
  • DOI: 10.1093/mnras/stt861

THE TYPE IIb SUPERNOVA 2011dh FROM A SUPERGIANT PROGENITOR
journal, August 2012

  • Bersten, Melina C.; Benvenuto, Omar G.; Nomoto, Ken'ichi
  • The Astrophysical Journal, Vol. 757, Issue 1
  • DOI: 10.1088/0004-637X/757/1/31

Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-Powered Explosions
journal, April 2016


A cosmological bound on the invisible axion
journal, January 1983


Bounds on exotic-particle interactions from SN1987A
journal, May 1988


Axions and SN 1987A: Axion trapping
journal, November 1990


Solar System Abundances and Condensation Temperatures of the Elements
journal, July 2003

  • Lodders, Katharina
  • The Astrophysical Journal, Vol. 591, Issue 2
  • DOI: 10.1086/375492

Neutrino Energy Loss in Stellar Interiors. VII. Pair, Photo-, Plasma, Bremsstrahlung, and Recombination Neutrino Processes
journal, January 1996

  • Itoh, Naoki; Hayashi, Hiroshi; Nishikawa, Akinori
  • The Astrophysical Journal Supplement Series, Vol. 102
  • DOI: 10.1086/192264

Constraints on light particles from supernova SN 1987A
journal, July 1987


Numerical Modeling of the Early Light Curves of type iip Supernovae
journal, September 2016


Axion cosmology
journal, July 2016


Constraining the Axion-Photon Coupling with Massive Stars
journal, February 2013


On the blue loops of intermediate-mass stars
journal, January 2015

  • Walmswell, J. J.; Tout, C. A.; Eldridge, J. J.
  • Monthly Notices of the Royal Astronomical Society, Vol. 447, Issue 3
  • DOI: 10.1093/mnras/stu2666

Axions: Theory and Cosmological Role
journal, October 2013


A New Light Boson?
journal, January 1978


Formation of the first stars
journal, October 2013


Effects of rotation on the evolution of primordial stars
journal, July 2008


Works referencing / citing this record:

Accretion-induced Collapse of Dark Matter Admixed White Dwarfs. II. Rotation and Gravitational-wave Signals
journal, September 2019

  • Zha, Shuai; Chu, Ming-Chung; Leung, Shing-Chi
  • The Astrophysical Journal, Vol. 883, Issue 1
  • DOI: 10.3847/1538-4357/ab3640