The radioactive nuclei 26Al and 60Fe in the Cosmos and in the solar system

Diehl, R.; Lugaro, M.; Heger, A.; Sieverding, A.; Tang, X.; Li, K. A.; Li, E. T.; Doherty, C. L.; Krause, M. H.; Wallner, A.; Prantzos, N.; Brinkman, H. E.; den Hartogh, J. W.; Wehmeyer, B.; Yagüe López, A.; Pleintinger, M. M.; Banerjee, P.; Wang, W.

doi:10.1017/pasa.2021.48

Title: The radioactive nuclei ²⁶Al and ⁶⁰Fe in the Cosmos and in the solar system

Abstract

The cosmic evolution of the chemical elements from the Big Bang to the present time is driven by nuclear fusion reactions inside stars and stellar explosions. A cycle of matter recurrently re-processes metal-enriched stellar ejecta into the next generation of stars. The study of cosmic nucleosynthesis and this matter cycle requires the understanding of the physics of nuclear reactions, of the conditions at which the nuclear reactions are activated inside the stars and stellar explosions, of the stellar ejection mechanisms through winds and explosions, and of the transport of the ejecta towards the next cycle, from hot plasma to cold, star-forming gas. Due to the long timescales of stellar evolution, and because of the infrequent occurrence of stellar explosions, observational studies are challenging, as they have biases in time and space as well as different sensitivities related to the various astronomical methods. Here, we describe in detail the astrophysical and nuclear-physical processes involved in creating two radioactive isotopes useful in such studies, ²⁶Al and ⁶⁰Fe. Due to their radioactive lifetime of the order of a million years, these isotopes are suitable to characterise simultaneously the processes of nuclear fusion reactions and of interstellar transport. We describe and discuss the nuclearmore »« less

Authors:

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^[5]; Li, E. T. ^[6];

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Max Planck Institute for Extraterrestrial Physics, Garching (Germany)
Eotvos Lorand Research Network (ELKH), Budapest (Hungary); Eotvos Lorand Univ., Budapest (Hungary); Monash Univ., Melbourne, VIC (Australia)
Monash Univ., Melbourne, VIC (Australia); Australian Research Council Centre of Excellence for Gravitational Wave Discovery, Clayton (Australia); Center of Excellence for Astrophysics in Three Dimensions (Australia); ; Michigan State Univ., East Lansing, MI (United States)
Univ. of Minnesota, Minneapolis, MN (United States); Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
Chinese Academy of Sciences (CAS), Lanzhou (China)
ShenZhen Univ., Shenzhen (China)
Eotvos Lorand Research Network (ELKH), Budapest (Hungary); Monash Univ., Melbourne, VIC (Australia)
Univ. of Hertfordshire, Hatfield (United Kingdom)
Institute of Ion Beam Physics and Materials Research, Dresden (Germany); Australian National Univ., Canberra, ACT (Australia)
Institut d’Astrophysique, Paris (France)
Eotvos Lorand Research Network (ELKH), Budapest (Hungary); Univ. of Szeged (Hungary)
Eotvos Lorand Research Network (ELKH), Budapest (Hungary)
Eotvos Lorand Research Network (ELKH), Budapest (Hungary); Univ. of Hertfordshire, Hatfield (United Kingdom)
Indian Inst. of Technology (IIT), Palakkad (India)
Wuhan Univ. (China)

Publication Date:: Thu Dec 09 00:00:00 EST 2021

Research Org.:: Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States)

Sponsoring Org.:: USDOE; European Cooperation in Science and Technology; Australian Research Council (ARC); National Science Foundation (NSF)

OSTI Identifier:: 1855649

Grant/Contract Number:: AC05-00OR22725; FG02-87ER40328; 724560; CA16117; PHY-1430152

Resource Type:: Accepted Manuscript

Journal Name:: Publications of the Astronomical Society of Australia

Additional Journal Information:: Journal Volume: 38; Journal Issue: 1; Journal ID: ISSN 1323-3580

Publisher:: CSIRO

Country of Publication:: United States

Language:: English

Subject:: 79 ASTRONOMY AND ASTROPHYSICS; nucleosynthesis; isotope; nucleus; reaction; stars; evolution; interstellar medium

Citation Formats


                    Diehl, R., Lugaro, M., Heger, A., Sieverding, A., Tang, X., Li, K. A., Li, E. T., Doherty, C. L., Krause, M. H., Wallner, A., Prantzos, N., Brinkman, H. E., den Hartogh, J. W., Wehmeyer, B., Yagüe López, A., Pleintinger, M. M., Banerjee, P., and Wang, W. The radioactive nuclei 26Al and 60Fe in the Cosmos and in the solar system.  United States: N. p., 2021. 
Web.  doi:10.1017/pasa.2021.48.

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                    Diehl, R., Lugaro, M., Heger, A., Sieverding, A., Tang, X., Li, K. A., Li, E. T., Doherty, C. L., Krause, M. H., Wallner, A., Prantzos, N., Brinkman, H. E., den Hartogh, J. W., Wehmeyer, B., Yagüe López, A., Pleintinger, M. M., Banerjee, P., & Wang, W. The radioactive nuclei 26Al and 60Fe in the Cosmos and in the solar system.  United States.  https://doi.org/10.1017/pasa.2021.48

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                    Diehl, R., Lugaro, M., Heger, A., Sieverding, A., Tang, X., Li, K. A., Li, E. T., Doherty, C. L., Krause, M. H., Wallner, A., Prantzos, N., Brinkman, H. E., den Hartogh, J. W., Wehmeyer, B., Yagüe López, A., Pleintinger, M. M., Banerjee, P., and Wang, W. Thu .  
"The radioactive nuclei 26Al and 60Fe in the Cosmos and in the solar system".  United States.  https://doi.org/10.1017/pasa.2021.48.  https://www.osti.gov/servlets/purl/1855649.

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@article{osti_1855649,

  title        = {The radioactive nuclei 26Al and 60Fe in the Cosmos and in the solar system},

  author       = {Diehl, R. and Lugaro, M. and Heger, A. and Sieverding, A. and Tang, X. and Li, K. A. and Li, E. T. and Doherty, C. L. and Krause, M. H. and Wallner, A. and Prantzos, N. and Brinkman, H. E. and den Hartogh, J. W. and Wehmeyer, B. and Yagüe López, A. and Pleintinger, M. M. and Banerjee, P. and Wang, W.},

  abstractNote = {The cosmic evolution of the chemical elements from the Big Bang to the present time is driven by nuclear fusion reactions inside stars and stellar explosions. A cycle of matter recurrently re-processes metal-enriched stellar ejecta into the next generation of stars. The study of cosmic nucleosynthesis and this matter cycle requires the understanding of the physics of nuclear reactions, of the conditions at which the nuclear reactions are activated inside the stars and stellar explosions, of the stellar ejection mechanisms through winds and explosions, and of the transport of the ejecta towards the next cycle, from hot plasma to cold, star-forming gas. Due to the long timescales of stellar evolution, and because of the infrequent occurrence of stellar explosions, observational studies are challenging, as they have biases in time and space as well as different sensitivities related to the various astronomical methods. Here, we describe in detail the astrophysical and nuclear-physical processes involved in creating two radioactive isotopes useful in such studies, 26Al and 60Fe. Due to their radioactive lifetime of the order of a million years, these isotopes are suitable to characterise simultaneously the processes of nuclear fusion reactions and of interstellar transport. We describe and discuss the nuclear reactions involved in the production and destruction of 26Al and 60Fe, the key characteristics of the stellar sites of their nucleosynthesis and their interstellar journey after ejection from the nucleosynthesis sites. This allows us to connect the theoretical astrophysical aspects to the variety of astronomical messengers presented here, from stardust and cosmic-ray composition measurements, through observation of γ rays produced by radioactivity, to material deposited in deep-sea ocean crusts and to the inferred composition of the first solids that have formed in the Solar System. We show that considering measurements of the isotopic ratio of 26Al to 60Fe eliminate some of the unknowns when interpreting astronomical results, and discuss the lessons learned from these two isotopes on cosmic chemical evolution. This review paper has emerged from an ISSI-BJ Team project in 2017–2019, bringing together nuclear physicists, astronomers, and astrophysicists in this inter-disciplinary discussion.},

  doi          = {10.1017/pasa.2021.48},

  journal      = {Publications of the Astronomical Society of Australia},

  number       = 1,

  volume       = 38,

  place        = {United States},

  year         = {Thu Dec 09 00:00:00 EST 2021},

  month        = {Thu Dec 09 00:00:00 EST 2021}

}

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Title: The radioactive nuclei 26Al and 60Fe in the Cosmos and in the solar system

Abstract

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New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s): Improved astrophysical parameters for the Geneva-Copenhagen Survey⋆ journal, May 2011

Astromers: Nuclear Isomers in Astrophysics journal, December 2020

Constraints on the Time Delay between Nucleosynthesis and Cosmic-Ray Acceleration from Observations of [TSUP]59[/TSUP]N[CLC]i[/CLC] and [TSUP]59[/TSUP]C[CLC]o[/CLC] journal, September 1999

The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars journal, January 2014

Status on $$^{\mathbf {12}}\mathbf {C}+{}^{\mathbf {12}}{\mathbf {C}}$$ fusion at deep subbarrier energies: impact of resonances on astrophysical $$S^{*}$$ factors journal, March 2020

CARBON-RICH PRESOLAR GRAINS FROM MASSIVE STARS: SUBSOLAR 12 C/ 13 C AND 14 N/ 15 N RATIOS AND THE MYSTERY OF 15 N journal, July 2015

Triggering Collapse of the Presolar Dense Cloud core and Injecting Short-Lived Radioisotopes with a Shock Wave. iii. Rotating Three-Dimensional Cloud Cores journal, May 2014

Capture of particles by isospin-symmetric nuclei journal, August 2000

Astrophysical Reaction Rates From Statistical Model Calculations journal, May 2000

Reaction rate uncertainties and the operation of the NeNa and MgAl chains during HBB in intermediate-mass AGB stars journal, February 2007

Nuclear astrophysics lessons from INTEGRAL journal, February 2013

Solar r-process-constrained actinide production in neutrino-driven winds of supernovae journal, April 2016

L'enfant consultant journal, January 2001

Impact of transport modeling on the Fe 60 abundance inside Galactic cosmic ray sources journal, April 2020

The effects of short-lived radionuclides and porosity on the early thermo-mechanical evolution of planetesimals journal, August 2016

Comparing simulated 26 Al maps to gamma-ray measurements journal, December 2019

Measurement of the Secondary Radionuclides 10 Be, 26 Al, 36 Cl, 54 Mn, and 14 C and Implications for the Galactic Cosmic‐Ray Age journal, December 2001

F 60 e Anomaly in a Deep-Sea Manganese Crust and Implications for a Nearby Supernova Source journal, October 2004

Chemical enrichment of the pre-solar cloud by supernova dust grains journal, July 2016

A RUNAWAY WOLF-RAYET STAR AS THE ORIGIN OF 26 Al IN THE EARLY SOLAR SYSTEM journal, April 2010

The s process in rotating low-mass AGB stars: Nucleosynthesis calculations in models matching asteroseismic constraints journal, September 2019

The abundance of 26 Al-rich planetary systems in the Galaxy journal, September 2015

Galacti chemical evolution: Hygrogen through zinc journal, May 1995

Mass loss of stars on the asymptotic giant branch: Mechanisms, models and measurements journal, January 2018

Title: The radioactive nuclei ²⁶Al and ⁶⁰Fe in the Cosmos and in the solar system

Kinematics of massive star ejecta in the Milky Way as traced by ²⁶ Al
journal, November 2013

New Measurement of the ${}^{60}{Fe}$ Half-Life
journal, August 2009

Spin-isospin strength distributions in f - p shell nuclei: A study of the ${}^{51}V$ ( n , p ) and ${}^{59}{Co}$ ( n , p ) reactions at 198 MeV
journal, December 1993

Production of ²⁶ Al by super-AGB stars
journal, July 2008

²⁶ Al kinematics: superbubbles following the spiral arms? : Constraints from the statistics of star clusters and HI supershells
journal, June 2015

Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes
journal, April 2020

A deep insight into the Mg-Al-Si nucleosynthesis in massive asymptotic giant branch and super-asymptotic giant branch stars: Mg-Al-Si nucleosynthesis in massive AGB stars
journal, June 2011

Short-lived radioactivity in the early solar system: The Super-AGB star hypothesis: SLR and the super-AGB star hypothesis
journal, September 2012

26Al–26Mg and 207Pb–206Pb systematics of Allende CAIs: Canonical solar initial 26Al/27Al ratio reinstated
journal, July 2008

Cosmogenic-nuclide production rates: Reaction cross section update
journal, January 2013

Intermediate-mass Asymptotic Giant Branch Stars and Sources of ²⁶ Al, ⁶⁰ Fe, ¹⁰⁷ Pd, and ¹⁸² Hf in the Solar System
journal, February 2017

Evolution of massive AGB stars: III. the thermally pulsing super-AGB phase
journal, March 2010

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

Stellar Winds
journal, September 1979

Thermonuclear (Type I) X‐Ray Bursts Observed by the Rossi X‐Ray Timing Explorer
journal, December 2008

Progenitor-Explosion Connection and Remnant Birth Masses for Neutrino-Driven Supernovae of Iron-Core Progenitors
journal, September 2012

Probing the evolving massive star population in Orion with kinematic and radioactive tracers
journal, September 2010

Interaction of Supernova Ejecta with Nearby Protoplanetary Disks
journal, June 2007

Supernova enrichment of planetary systems in low-mass star clusters
journal, October 2016

Mass spectrometric searches for superheavy elements in terrestrial matter
journal, December 2015

Supernova theory and supernova 1987A
journal, August 1987

New estimates of the contribution of Wolf-Rayet stellar winds to the Galactic $\mathsf{^{26}}$Al
journal, December 2004

ABUNDANCE OF ²⁶ Al AND ⁶⁰ Fe IN EVOLVING GIANT MOLECULAR CLOUDS
journal, May 2013

LOW ⁶⁰ FE ABUNDANCE IN SEMARKONA AND SAHARA 99555
journal, March 2015

ELECTRON-CAPTURE SUPERNOVAE AS SOURCES OF ⁶⁰ Fe
journal, August 2013

Volatile Delivery to Planets from Water-Rich Planetesimals Around Low-Mass Stars
journal, April 2015

Origin of the Local Bubble
journal, September 2008

The Nucleosynthesis of ²⁶ Al and ⁶⁰ Fe in Solar Metallicity Stars Extending in Mass from 11 to 120 M _⊙ : The Hydrostatic and Explosive Contributions
journal, August 2006

Surface wave photonic quasicrystal
journal, April 2020

Endomorphisms of words in a quiver
journal, November 1993

Stochastic Chemical Evolution of Radioactive Isotopes with a Monte Carlo Approach
journal, December 2019

Galactic Chemical Evolution of Radioactive Isotopes
journal, June 2019

An increase in the 12C + 12C fusion rate from resonances at astrophysical energies
journal, May 2018

Progenitors of Core-Collapse Supernovae
journal, September 2009

Effective stellar $β$ -decay rates of nuclei with long-lived isomers: ${}^{26}{Al}$ and ${}^{34}{Cl}$
journal, June 2018

Supernova remnants: the X-ray perspective
journal, December 2011

The Non-carbonaceous–Carbonaceous Meteorite Dichotomy
journal, May 2020

Slowing the spins of stellar cores
journal, February 2019

New Constraints on the Abundance of ⁶⁰ Fe in the Early Solar System
journal, April 2018

The nu-process
journal, June 1990

Neutron‐rich Nucleosynthesis in Carbon Deflagration Supernovae
journal, February 1997

The theory of stellar winds
journal, February 2011

Radioactive ²⁶ Al from the Scorpius-Centaurus association
journal, November 2010

Injection of Short‐Lived Radionuclides into the Early Solar System from a Faint Supernova with Mixing Fallback
journal, December 2008

Nucleosynthesis in Supernovae
journal, March 2018

The supernova trigger for formation of the solar system
journal, March 1977

EVOLUTION, NUCLEOSYNTHESIS, AND YIELDS OF AGB STARS AT DIFFERENT METALLICITIES. III. INTERMEDIATE-MASS MODELS, REVISED LOW-MASS MODELS, AND THE pH-FRUITY INTERFACE
journal, August 2015

Aluminum-26 in the early solar system - Fossil or fuel
journal, January 1977

A complete catalogue of dusty supernova remnants in the Galactic plane
journal, February 2020

Supernova-Produced ${}^{53}{Mn}$ on Earth
journal, July 2020

Constraints on models for chemical evolution in the solar neighborhood
journal, September 1974

26Al in the interstellar medium
journal, January 1987

On the variation of the initial mass function
journal, April 2001

New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s): Improved astrophysical parameters for the Geneva-Copenhagen Survey⋆
journal, May 2011

Astromers: Nuclear Isomers in Astrophysics
journal, December 2020

Constraints on the Time Delay between Nucleosynthesis and Cosmic-Ray Acceleration from Observations of [TSUP]59[/TSUP]N[CLC]i[/CLC] and [TSUP]59[/TSUP]C[CLC]o[/CLC]
journal, September 1999

The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars
journal, January 2014

Status on $$^{\mathbf {12}}\mathbf {C}+{}^{\mathbf {12}}{\mathbf {C}}$$ fusion at deep subbarrier energies: impact of resonances on astrophysical $$S^{*}$$ factors
journal, March 2020

CARBON-RICH PRESOLAR GRAINS FROM MASSIVE STARS: SUBSOLAR ¹² C/ ¹³ C AND ¹⁴ N/ ¹⁵ N RATIOS AND THE MYSTERY OF ¹⁵ N
journal, July 2015

Triggering Collapse of the Presolar Dense Cloud core and Injecting Short-Lived Radioisotopes with a Shock Wave. iii. Rotating Three-Dimensional Cloud Cores
journal, May 2014

Capture of particles by isospin-symmetric nuclei
journal, August 2000

Astrophysical Reaction Rates From Statistical Model Calculations
journal, May 2000

Reaction rate uncertainties and the operation of the NeNa and MgAl chains during HBB in intermediate-mass AGB stars
journal, February 2007

Nuclear astrophysics lessons from INTEGRAL
journal, February 2013

Solar r-process-constrained actinide production in neutrino-driven winds of supernovae
journal, April 2016

L'enfant consultant
journal, January 2001

Impact of transport modeling on the ${}^{60}{Fe}$ abundance inside Galactic cosmic ray sources
journal, April 2020

The effects of short-lived radionuclides and porosity on the early thermo-mechanical evolution of planetesimals
journal, August 2016

Comparing simulated ²⁶ Al maps to gamma-ray measurements
journal, December 2019

Measurement of the Secondary Radionuclides ¹⁰ Be, ²⁶ Al, ³⁶ Cl, ⁵⁴ Mn, and ¹⁴ C and Implications for the Galactic Cosmic‐Ray Age
journal, December 2001

${}^{60}F e$ Anomaly in a Deep-Sea Manganese Crust and Implications for a Nearby Supernova Source
journal, October 2004

Chemical enrichment of the pre-solar cloud by supernova dust grains
journal, July 2016

A RUNAWAY WOLF-RAYET STAR AS THE ORIGIN OF ²⁶ Al IN THE EARLY SOLAR SYSTEM
journal, April 2010

The s process in rotating low-mass AGB stars: Nucleosynthesis calculations in models matching asteroseismic constraints
journal, September 2019

The abundance of ²⁶ Al-rich planetary systems in the Galaxy
journal, September 2015

Galacti chemical evolution: Hygrogen through zinc
journal, May 1995

Mass loss of stars on the asymptotic giant branch: Mechanisms, models and measurements
journal, January 2018

Angular Momentum Transport in Stellar Interiors
journal, August 2019

Inheritance of solar short- and long-lived radionuclides from molecular clouds and the unexceptional nature of the solar system
journal, April 2014