Relevant bibliographies by topics / Stellar nucleosynthesi

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
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Academic literature on the topic 'Stellar nucleosynthesi'

Author: Grafiati
Published: 9 March 2023
Last updated: 31 July 2025

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Journal articles on the topic "Stellar nucleosynthesi"

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Ryan, Sean G. "Big Bang Nucleosynthesis, Population III, and Stellar Genetics in the Galactic Halo." Publications of the Astronomical Society of Australia 19, no. 2 (2002): 238–45. http://dx.doi.org/10.1071/as01067.

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AbstractThe diverse isotopic and elemental signatures produced in different nucleosynthetic sites are passed on to successive generations of stars. By tracing these chemical signatures back through the stellar populations of the Galaxy, it is possible to unravel its nucleosynthetic history and even to study stars which are now extinct. This review considers recent applications of ‘stellar genetics’ to examine the earliest episodes of nucleosynthesis in the universe, in Population iii stars and the Big Bang.
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Doherty, Carolyn, John Lattanzio, George Angelou та ін. "Monash Chemical Yields Project (Monχey) Element production in low- and intermediate-mass stars". Proceedings of the International Astronomical Union 11, A29B (2015): 164–65. http://dx.doi.org/10.1017/s1743921316004725.

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AbstractThe Monχey project will provide a large and homogeneous set of stellar yields for the low- and intermediate- mass stars and has applications particularly to galactic chemical evolution modelling. We describe our detailed grid of stellar evolutionary models and corresponding nucleosynthetic yields for stars of initial mass 0.8 M⊙ up to the limit for core collapse supernova (CC-SN) ≈ 10 M⊙. Our study covers a broad range of metallicities, ranging from the first, primordial stars (Z = 0) to those of super-solar metallicity (Z = 0.04). The models are evolved from the zero-age main-sequence
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Salpeter, Edwin E. "Stellar nucleosynthesis." Reviews of Modern Physics 71, no. 2 (1999): S220—S222. http://dx.doi.org/10.1103/revmodphys.71.s220.

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Weiss, A. "Stellar nucleosynthesis." Physica Scripta T133 (January 1, 2008): 014025. http://dx.doi.org/10.1088/0031-8949/2008/t133/014025.

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Vescovi, Diego. "Mixing and Magnetic Fields in Asymptotic Giant Branch Stars in the Framework of FRUITY Models." Universe 8, no. 1 (2021): 16. http://dx.doi.org/10.3390/universe8010016.

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In the last few years, the modeling of asymptotic giant branch (AGB) stars has been much investigated, both focusing on nucleosynthesis and stellar evolution aspects. Recent advances in the input physics required for stellar computations made it possible to construct more accurate evolutionary models, which are an essential tool to interpret the wealth of available observational and nucleosynthetic data. Motivated by such improvements, the FUNS stellar evolutionary code has been updated. Nonetheless, mixing processes occurring in AGB stars’ interiors are currently not well-understood. This is
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Gil-Pons, P., C. L. Doherty, J. Gutiérrez, S. W. Campbell, L. Siess, and J. C. Lattanzio. "Nucleosynthetic yields of Z = 10−5 intermediate-mass stars." Astronomy & Astrophysics 645 (December 21, 2020): A10. http://dx.doi.org/10.1051/0004-6361/201937264.

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Context. Observed abundances of extremely metal-poor stars in the Galactic halo hold clues for understanding the ancient universe. Interpreting these clues requires theoretical stellar models in a wide range of masses in the low-metallicity regime. The existing literature is relatively rich with extremely metal-poor massive and low-mass stellar models. However, relatively little information is available on the evolution of intermediate-mass stars of Z ≲ 10−5, and the impact of the uncertain input physics on the evolution and nucleosynthesis has not yet been systematically analysed. Aims. We ai
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Tolasa, Diriba. "Stellar Evolution and Nucleosynthesis: Investigating the Life Cycles of Massive Stars and Their Role in Galactic Chemical Enrichment." Engineering Physics 8, no. 1 (2025): 24–40. https://doi.org/10.11648/j.ep.20250801.13.

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Stellar evolution and nucleosynthesis are fundamental processes that govern the life cycles of massive stars, significantly influencing the chemical enrichment of galaxies. This study aims to elucidate the intricate mechanisms underlying the evolution of massive stars, from their formation in molecular clouds to their explosive demise as supernovae. Massive stars, defined as those with initial masses exceeding approximately eight solar masses, undergo a series of complex nuclear fusion reactions that synthesize heavier elements, thereby contributing to the cosmic abundance of elements beyond h
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Monpribat, E., A. Choplin, S. Martinet, et al. "A new 12C+12C reaction rate: Impact on stellar evolution." EPJ Web of Conferences 279 (2023): 11016. http://dx.doi.org/10.1051/epjconf/202327911016.

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Among the reactions driving stellar evolution during carbon burning, 12C + 12C fusion provides the key ingredients. This system reveals many resonances, but also regions with suppressed fusion cross-sections. The reaction was recently measured by the STELLA collaboration utilizing the gammaparticle coincidence technique for precise cross-section measurements reaching down to the Gamow window of massive stars. From the experimental data, reaction rates were determined by approximating a hindrance parametrization and by adding on top a resonance at the lowest measured energy. The impact of these
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Karinkuzhi, D., S. Van Eck, A. Jorissen, et al. "When binaries keep track of recent nucleosynthesis." Proceedings of the International Astronomical Union 14, S343 (2018): 438–40. http://dx.doi.org/10.1017/s1743921318006567.

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AbstractWe determine Zr and Nb elemental abundances in barium stars to probe the operation temperature of the s-process that occurred in the companion asymptotic giant branch (AGB) stars. Along with Zr and Nb, we derive the abundances of a large number of heavy elements. They provide constraints on the s-process operation temperature and therefore on the s-process neutron source. The results are then compared with stellar evolution and nucleosynthesis models. We compare the nucleosynthetic profile of the present sample stars with those of CEMP-s, CEMP-rs and CEMP-r stars. One barium star of ou
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AOKI, Wako, and Nobuyuki IWAMOTO. "Stellar Evolution and Nucleosynthesis." Journal of Plasma and Fusion Research 79, no. 9 (2003): 871–77. http://dx.doi.org/10.1585/jspf.79.871.

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Dissertations / Theses on the topic "Stellar nucleosynthesi"

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MASHA, ELIANA. "ASTROPHYSICAL NUCLEAR REACTIONS ON NEON ISOTOPES AT LUNA." Doctoral thesis, Università degli Studi di Milano, 2022. http://hdl.handle.net/2434/899089.

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This thesis reports the direct measurements of the 22Ne(α,γ)26Mg and 20Ne(p,γ)21Na reactions at astrophysical energies of interest. The 22Ne(α,γ)26Mg reaction competes with the 22Ne(α,n)25Mg reaction which is the main source of neutrons for the s-process in low-mass Asymptotic Giant Branch and massive stars. At temperatures T < 300 MK where the (α,γ) channel becomes dominant, the rate of the 22Ne(α,γ)26Mg reaction is influenced by several resonances studied only indirectly. The first part of this thesis concerns the direct measurement of one of these resonances, Er = 334 keV, which so f
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Joseph, Craig L. "Q-nucleosynthesis : implications for stellar evolution /." The Ohio State University, 1985. http://rave.ohiolink.edu/etdc/view?acc_num=osu1487260531956577.

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Scholz, Philipp [Verfasser]. "Exploring statistical properties of nuclei for explosive stellar nucleosynthesis / Philipp Scholz." München : Verlag Dr. Hut, 2018. http://d-nb.info/1170473377/34.

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Margerin, Vincent. "Transfer reaction measurements and the stellar nucleosynthesis of 26A1 and 44Ti." Thesis, University of Edinburgh, 2016. http://hdl.handle.net/1842/25428.

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Progress in the description of stellar evolution is driven by the collaborative effort of nuclear physics, astrophysics and astronomy. Using those developments, the theory of the origin of elements in the Universe is challenged. This thesis addresses the problem behind the abundance of 44Ti and the origin of 26Al. The mismatch between the predicted abundance of 44Ti as produced by the only sites known to be able to create 44Ti, core collapse supernovae (CCSNe), and the observations, highlight the current uncertainty that exists in the physics of these stars. Several satellite based γ-ray obser
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Mountford, David James. "Investigations of nuclear reactions relevant to stellar γ-ray emission". Thesis, University of Edinburgh, 2013. http://hdl.handle.net/1842/8238.

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The detection of γ-rays from explosive astrophysical scenarios such as novae provides an excellent opportunity for the study of on-going nucleosynthesis in the Universe. Within this context, this work has addressed an uncertainty in the destruction rate of the 18F nucleus, thought to be the primary source of 511 keV γ-rays from novae. A direct measurement of the 18F(p,α )15O cross section has provided the opportunity to extract resonance parameters through the R-Matrix formalism. The inferred parameters of populated states in 19Ne include the observation of a broad 1/2+ state, consistent with
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Arzhanov, Alexander. "Gogny-Hartree-Fock-Bogolyubov Nuclear Mass Models with Application to r-Process Stellar Nucleosynthesis." Thesis, KTH, Kärnfysik, 2013. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-139303.

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Lombardo, Linda. "Explorer l'histoire de la Galaxie grâce à la spectroscopie stellaire." Electronic Thesis or Diss., Université Paris sciences et lettres, 2022. http://www.theses.fr/2022UPSLO011.

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Ce travail de thèse présente plusieurs études qui utilisent la spectroscopie à haute résolution pour déterminer les propriétés chimiques des différentes populations stellaires de la Voie Lactée. Le document est structuré comme suit : Le premier chapitre de la thèse, divisée en 3 sections, est une introduction générale à la structure de la Voie lactée et à ses populations stellaires, suivie d'une partie décrivant les différentes méthodes utilisées pour mesurer les abondances chimiques des étoiles. La première section décrit les différents scénarios concernant la structure et la formation de la
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Meakin, Casey Adam. "Hydrodynamic Modeling of Massive Star Interiors." Diss., The University of Arizona, 2006. http://hdl.handle.net/10150/194035.

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In this thesis, the hydrodynamics of massive star interiors are explored. Our primary theoretical tool is multi-dimensional hydrodynamic simulation using realistic initial conditions calculated with the one-dimensional stellar evolution code, TYCHO. The convective shells accompanying oxygen and carbon burning are examined, including models with single as well as multiple, simultaneously burning shells. A convective core during hydrogen burning is also studied in order to test the generality of the flow characteristics. Two and three dimensional models are calculated. We analyze the properties
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KIOUS, MALEK. "Determination de taux de reactions nucleaires conduisant a la nucleosynthese stellaire du fluor." Paris 11, 1990. http://www.theses.fr/1990PA112371.

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La nucleosynthese stellaire du fluor reste a ce jour inexpliquee. Si l'on en croit les taux de reaction admis actuellement, le fluor synthetise au cours de la combustion de l'hydrogene ou de l'helium est immediatement detruit. Nous avons entrepris l'etude spectroscopique des niveaux du neon vingt (participant a la combustion du fluor) situes pres du seuil proton. Nous avons en particulier mis en evidence l'importance d'un niveau proche du seuil proton, qui par des effets d'interferences qu'il induit avec les autres niveaux de meme spin-parite, modifie de facon importante le taux de destruction
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Wagner, Louis. "Precise nuclear data of the 14N(p,gamma)15O reaction for solar neutrino predictions." Helmholtz-Zentrum Dresden-Rossendorf, 2018. https://tud.qucosa.de/id/qucosa%3A31122.

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The 14N(p,gamma)15O reaction is the slowest stage of the carbon-nitrogen-oxygen cycle of hydrogen burning and thus determines its reaction rate. Precise knowledge of its rate is required to improve the model of hydrogen burning in our sun. The reaction rate is a necessary ingredient for a possible solution of the solar abundance problem that led to discrepancies between predictions of the solar standard model and helioseismology. The solar 13N and 15O neutrino fluxes are used as independent observables that probe the carbon and nitrogen abundances in the solar core. This could settle the disag
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Books on the topic "Stellar nucleosynthesi"

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J, Norton Andrew, ed. Stellar evolution and nucleosynthesis. Cambridge University Press, 2010.

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Charbonnel, C., and J. P. Zahn. Stellar nucleosyntheis 50 years after B²FH: Summer school on stellar physics XVI, Aussois, France, December 4-8, 2006. EDP Sciences, 2008.

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N, Schramm David, Truran James W, Fermi National Accelerator Laboratory, and United States. National Aeronautics and Space Administration., eds. On relative supernova rates and nucleosynthesis roles. Fermi National Accelerator Laboratory, 1988.

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G, Barnes Thomas, Bash Frank N, and Lambert David L, eds. Cosmic abundances as records of stellar evolution and nucleosynthesis in honor of David L. Lambert: Proceedings of a symposium held in Austin, Texas, USA, 17-19 June 2004. Astronomical Society of the Pacific, 2005.

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Green, James A. Galactic Evolution and Stellar Nucleosynthesis. Greenwood Research, 1999.

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Stellar Explosions: Nucleosynthesis and Cosmochemistry. Taylor & Francis Group, 2015.

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Jose, Jordi. Stellar Explosions: Hydrodynamics and Nucleosynthesis. Taylor & Francis Group, 2016.

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Jose, Jordi. Stellar Explosions: Hydrodynamics and Nucleosynthesis. Taylor & Francis Group, 2016.

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Close, Frank. 5. Making and breaking nuclei. Oxford University Press, 2015. http://dx.doi.org/10.1093/actrade/9780198718635.003.0005.

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‘Making and breaking nuclei’ describes the process by which the atomic elements came to be in the early universe. The heat energy in the big bang, some 13.7 billion years ago, converted into counterbalanced particles of matter and antimatter. The seeds of atomic nuclei were initially the simplest constituents: quarks. During the last 5 billion years, the majority of elements found on earth were formed inside a long-dead star, where they were all cooked from protons, which were synthesised within the first second of the universe. The processes of stellar nucleosynthesis, the CNO cycle, supernov
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Chiosi, C., and Alvio Renzini. Stellar Nucleosynthesis: Proceedings of the Third Workshop of the Advanced School of Astronomy of the Ettore Majorana Centre for Scientific Culture, Erice, Italy, May 11-21 1983. Springer, 2012.

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Book chapters on the topic "Stellar nucleosynthesi"

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Prantzos, Nikos, and Sylvia Ekström. "Stellar Nucleosynthesis." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2011. http://dx.doi.org/10.1007/978-3-642-11274-4_1084.

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Prantzos, Nikos, and Sylvia Ekström. "Nucleosynthesis, Stellar." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-44185-5_1084.

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Prantzos, Nikos, and Sylvia Ekström. "Nucleosynthesis, Stellar." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2023. http://dx.doi.org/10.1007/978-3-662-65093-6_1084.

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Salpeter, Edwin E. "Stellar Nucleosynthesis." In More Things in Heaven and Earth. Springer New York, 1999. http://dx.doi.org/10.1007/978-1-4612-1512-7_23.

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Prantzos, Nikos, and Sylvia Ekström. "Nucleosynthesis, Stellar." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-27833-4_1084-3.

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Thielemann, F. K., D. Argast, F. Brachwitz, et al. "Nucleosynthesis and Stellar Evolution." In The Evolution of Galaxies. Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-017-3311-3_3.

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Matteucci, Francesca. "Stellar Evolution and Nucleosynthesis." In The Chemical Evolution of the Galaxy. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0967-6_2.

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Maeda, Keiichi. "Stellar Evolution, SN Explosion, and Nucleosynthesis." In Handbook of X-ray and Gamma-ray Astrophysics. Springer Nature Singapore, 2024. http://dx.doi.org/10.1007/978-981-19-6960-7_85.

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Maeda, Keiichi. "Stellar Evolution, SN Explosion, and Nucleosynthesis." In Handbook of X-ray and Gamma-ray Astrophysics. Springer Nature Singapore, 2022. http://dx.doi.org/10.1007/978-981-16-4544-0_85-1.

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Smith, Verne V. "Nucleosynthesis in the MS and S Stars." In Late Stages of Stellar Evolution. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3813-7_36.

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Conference papers on the topic "Stellar nucleosynthesi"

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Thielemann, F. K. "Stellar nucleosynthesis and galactic abundances." In SOLAR AND GALACTIC COMPOSITION: A Joint SOHO/ACE Workshop. AIP, 2001. http://dx.doi.org/10.1063/1.1434005.

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Hirschi, Raphael, Jacqueline den Hartogh, Andrea Cristini, Cyril Georgy, and Marco Pignatari. "Stellar structure, evolution and nucleosynthesis." In XIII Nuclei in the Cosmos. Sissa Medialab, 2015. http://dx.doi.org/10.22323/1.204.0001.

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Sharina, M., M. Maricheva, I. Acharova, and V. Shimansky. "Stellar populations of extragalactic globular clusters." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.088.

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Globular clusters (GCs) are the oldest (ages up to 13.6 Gyr), but not the most metal-poor ( -2.9<[Fe/H]<0 dex) objects in the Universe. Studying properties of their stellar populations and comparing them with the properties of structural components of galaxies and stellar streams is necessary to understand the processes of nucleosynthesis and galaxy formation. We analyse integrated-light (IL) spectra of extragalactic GCs in order to determine the properties of their horizontal branch stars, ages and chemical composition. For this purpose, we compare the observed and synthetic spectra of
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Chieffi, Alessandro. "Element production - stellar evolution - explosive nucleosynthesis." In 11th Symposium on Nuclei in the Cosmos. Sissa Medialab, 2011. http://dx.doi.org/10.22323/1.100.0296.

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El Eid, Mounib, Claudi Spitaleri, Claus Rolfs, and Rosario G. Pizzone. "Stellar Nucleosynthesis: s-Process in Massive Stars." In FIFTH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS. AIP, 2010. http://dx.doi.org/10.1063/1.3362611.

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Mengoni, A. "Neutron capture reaction rates for stellar nucleosynthesis." In CAPTURE GAMMA-RAY SPECTROSCOPY AND RELATED TOPICS: 12th International Symposium. AIP, 2006. http://dx.doi.org/10.1063/1.2187868.

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Chiosi, Cesare, Claudi Spitaleri, Claus Rolfs, and Rosario G. Pizzone. "Primordial and Stellar Nucleosynthesis Chemical Evolution of Galaxies." In FIFTH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS. AIP, 2010. http://dx.doi.org/10.1063/1.3362605.

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Zinner, Ernst. "What presolar grains tell us about stellar nucleosynthesis." In 11th Symposium on Nuclei in the Cosmos. Sissa Medialab, 2011. http://dx.doi.org/10.22323/1.100.0306.

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Masseron, Thomas. "Stellar Nucleosynthesis in the Galactic History: the Carbon Stars." In FIRST STARS III: First Stars II Conference. American Institute of Physics, 2008. http://dx.doi.org/10.1063/1.2905535.

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Suzuki, Toshio, Michio Honma, Noritaka Shimizu, et al. "Electron-capture Rates Of Nuclei At Stellar Environments And Nucleosynthesis." In The 26th International Nuclear Physics Conference. Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.281.0155.

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Reports on the topic "Stellar nucleosynthesi"

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Hart, M. Boson Fermion Nuclei Stellar Nucleosynthesis: Monograph #7. Office of Scientific and Technical Information (OSTI), 2021. http://dx.doi.org/10.2172/1773253.

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Isselhardt, B. Deciphering Fingerprints of Stellar Nucleosynthesis Through Nuclear Reaction Rate Measurements and Isotopic Analyses of Stardust. Office of Scientific and Technical Information (OSTI), 2023. http://dx.doi.org/10.2172/1999459.

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Isselhardt, B. Deciphering Fingerprints of Stellar Nucleosynthesis Through Nuclear Reaction Rate Measurements and Isotopic Analyses of Stardust. Office of Scientific and Technical Information (OSTI), 2023. http://dx.doi.org/10.2172/1999460.

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