Relevant bibliographies by topics / Globular Clusters Core Dynamics

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers

Academic literature on the topic 'Globular Clusters Core Dynamics'

Author: Grafiati
Published: 4 June 2021
Last updated: 5 February 2022

Create a spot-on reference in APA, MLA, Chicago, Harvard, and other styles

Select a source type:

Consult the lists of relevant articles, books, theses, conference reports, and other scholarly sources on the topic 'Globular Clusters Core Dynamics.'

Next to every source in the list of references, there is an 'Add to bibliography' button. Press on it, and we will generate automatically the bibliographic reference to the chosen work in the citation style you need: APA, MLA, Harvard, Chicago, Vancouver, etc.

You can also download the full text of the academic publication as pdf and read online its abstract whenever available in the metadata.

Journal articles on the topic "Globular Clusters Core Dynamics"

1

Cohn, Haldan. "After Core Collapse. What?" Symposium - International Astronomical Union 126 (1988): 379–92. http://dx.doi.org/10.1017/s0074180900042613.

Full text
Abstract:
As our understanding of core collapse in globular clusters has improved through detailed computer simulations, attention has naturally turned to dynamical evolution of globular clusters after core collapse. The results of recent simulations of post-collapse cluster evolution are reviewed. An assessment is given of progress towards the goal of developing astrophysically realistic models that cover all phases of globular cluster evolution. A focus of this review is the stability of the post-collapse expansion phase to the large amplitude core oscillations first observed in the simulations of Sug
APA, Harvard, Vancouver, ISO, and other styles
2

Ivanova, Natalia, and Frederic A. Rasio. "Compact Binaries in Globular Clusters." International Astronomical Union Colloquium 194 (2004): 67–70. http://dx.doi.org/10.1017/s0252921100151942.

Full text
Abstract:
AbstractIn dense stellar systems the frequent dynamical interactions between stars play a crucial role in the formation and evolution of compact binaries. We study these processes using a novel approach combining a state-of-the- art binary population synthesis code with a simple treatment of dynamical interactions in dense star cluster cores. Here we focus on the dynamical and evolutionary processes leading to the formation of compact binaries containing white dwarfs in dense globular clusters. We demonstrate that dynamics can increase by factors ~ 2 – 100 the production rates of interesting b
APA, Harvard, Vancouver, ISO, and other styles
3

King, Ivan R. "Dynamical Implications of Deep HST Imaging of Globular Clusters." Symposium - International Astronomical Union 174 (1996): 29–38. http://dx.doi.org/10.1017/s0074180900001352.

Full text
Abstract:
HST observations contribute in many ways to a better understanding of the dynamical nature of globular clusters. Unprecedentedly faint photometry gives new determinations of the numbers of low-mass stars. Cluster-to-cluster differences at the faint ends of the mass functions suggest differences in dynamical evolution. Mass segregation is clearly observed, from the envelope inward to the dense cluster center. The distribution of stars in the hitherto unresolved cores gives new data with which to test theories of core collapse, and these core profiles are also sensitive to the number of unseen r
APA, Harvard, Vancouver, ISO, and other styles
4

Piatti, Andrés E., Jeremy J. Webb, and Raymond G. Carlberg. "Characteristic radii of the Milky Way globular clusters." Monthly Notices of the Royal Astronomical Society 489, no. 3 (2019): 4367–77. http://dx.doi.org/10.1093/mnras/stz2499.

Full text
Abstract:
ABSTRACT We report on the extent of the effects of the Milky Way gravitational field in shaping the structural parameters and internal dynamics of its globular cluster population. We make use of a homogeneous, up-to-date data set with kinematics, structural properties, current and initial masses of 156 globular clusters. In general, cluster radii increase as the Milky Way potential weakens; with the core and Jacobi radii being those which increase at the slowest and fastest rate, respectively. We interpret this result as the innermost regions of globular clusters being less sensitive to change
APA, Harvard, Vancouver, ISO, and other styles
5

Orkney, M. D. A., J. I. Read, J. A. Petts, and M. Gieles. "Globular clusters as probes of dark matter cusp-core transformations." Monthly Notices of the Royal Astronomical Society 488, no. 3 (2019): 2977–88. http://dx.doi.org/10.1093/mnras/stz1625.

Full text
Abstract:
Abstract Bursty star formation in dwarf galaxies can slowly transform a steep dark matter cusp into a constant density core. We explore the possibility that globular clusters (GCs) retain a dynamical memory of this transformation. To test this, we use the nbody6df code to simulate the dynamical evolution of GCs, including stellar evolution, orbiting in static and time-varying potentials for a Hubble time. We find that GCs orbiting within a cored dark matter halo, or within a halo that has undergone a cusp-core transformation, grow to a size that is substantially larger (Reff > 10 pc) th
APA, Harvard, Vancouver, ISO, and other styles
6

Sugimoto, Daiichiro. "A Comparative Study of Globular Clusters." Symposium - International Astronomical Union 174 (1996): 1–7. http://dx.doi.org/10.1017/s0074180900001327.

Full text
Abstract:
This paper is intended for an introduction to the Symposium. In 47 Tuc many milli-second pulsars are found while none has been reported in ω Cen. One might think that in 47 Tuc they have been formed in the collapsed core through tidal capture of a main sequence star by a neutron star. If we use the standard model of gravothermal collapse of globular clusters to integrate the squared stellar density over the core and over its time history, we find, however, the accumulated probability of tidal capture is lower in 47 Tuc than ω Cen. Such contradiction suggests that it will be important to take a
APA, Harvard, Vancouver, ISO, and other styles
7

Noyola, Eva, Karl Gebhardt та Marcel Bergmann. "Central Dynamics of Globular Clusters: the Case for a Black Hole in ω Centauri". Proceedings of the International Astronomical Union 3, S246 (2007): 341–45. http://dx.doi.org/10.1017/s1743921308015895.

Full text
Abstract:
AbstractThe globular cluster ω Centauri is one of the largest and most massive members of the Galactic system. Its classification as a globular cluster has been challenged making it a candidate for being the stripped core of an accreted dwarf galaxy; this and the fact that it has one of the largest velocity dispersions for star clusters in our galaxy makes it an interesting candidate for harboring an intermediate mass black hole. We measure the surface brightness profile from integrated light on an HST/ACS image, and find a central power-law cusp of logarithmic slope -0.08. We also analyze Gem
APA, Harvard, Vancouver, ISO, and other styles
8

Meylan, G., P. Dubath, and M. Mayor. "Dynamical study of the LMC globular cluster NGC 1978 from core velocity dispersion." Symposium - International Astronomical Union 148 (1991): 211–12. http://dx.doi.org/10.1017/s0074180900200405.

Full text
Abstract:
The projected velocity dispersion in the core of the Large Magellanic Cloud (LMC) intermediate-age globular cluster NGC 1978 is deduced from integrated light spectra. A numerical cross-correlation technique gives a projected velocity dispersion σp(core) = 5.8±1.2 km s−1. Multimass anisotropic King-Michie dynamical models are applied to the observational constraints given by the surface brightness profile and the above central projected velocity dispersion. Depending on the model, the values obtained for the total mass of the cluster range from 0.36 to 1.44 106M⊙, corresponding to mass-to-light
APA, Harvard, Vancouver, ISO, and other styles
9

Kremer, Kyle, Claire S. Ye, Sourav Chatterjee, Carl L. Rodriguez, and Frederic A. Rasio. "The Role of “black hole burning” in the evolution of dense star clusters." Proceedings of the International Astronomical Union 14, S351 (2019): 357–66. http://dx.doi.org/10.1017/s1743921319007269.

Full text
Abstract:
AbstractAs self-gravitating systems, dense star clusters exhibit a natural diffusion of energy from their innermost to outermost regions, leading to a slow and steady contraction of the core until it ultimately collapses under gravity. However, in spite of the natural tendency toward “core collapse,” the globular clusters (GCs) in the Milky Way exhibit a well-observed bimodal distribution in core radii separating the core-collapsed and non-core-collapsed clusters. This suggests an internal energy source is at work, delaying the onset of core collapse in many clusters. Over the past decade, a l
APA, Harvard, Vancouver, ISO, and other styles
10

Belloni, Diogo, Mirek Giersz, Liliana E. Rivera Sandoval, Abbas Askar, and Pawel Ciecielag. "Are most Cataclysmic Variables in Globular Clusters dynamically formed?" Proceedings of the International Astronomical Union 14, S351 (2019): 404–7. http://dx.doi.org/10.1017/s174392131900718x.

Full text
Abstract:
AbstractWe have been investigating populations of cataclysmic variables (CVs) in a set of more than 300 globular cluster (GC) models evolved with themoccacode.[-120pt] One of the main questions we have intended to answer is whether most CVs in GCs are dynamically formed or not. Contrary to what has been argued for a long time, we found that dynamical destruction of primordial CV progenitors is much stronger in GCs than dynamical formation of CVs. In particular, we found that, on average, the detectable CV population is predominantly composed of CVs formed via a typical common envelope phase (≳
APA, Harvard, Vancouver, ISO, and other styles
More sources

Dissertations / Theses on the topic "Globular Clusters Core Dynamics"

1

Sieni, Marco. "La cinematica nel core dell'ammasso globulare NGC 6441 da osservazioni SINFONI." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2016. http://amslaurea.unibo.it/9876/.

Full text
Abstract:
In questo elaborato viene presentata l'analisi cinematica delle regioni centrali di NGC 6441, uno degli ammassi globulari più massivi (M ~10^6 Msol) della nostra Galassia. L'ammasso è stato selezionato, insieme ad altri 18, all'interno dell'ESO Large Program “Unveiling the kinematics in the core of high-density globular clusters with SINFONI" (PI: Ferraro) per cercare evidenze di buchi neri di massa intermedia (IMBH), la cui esistenza è ancora controversa. Poichè la misura della dispersione di velocità da spettri integrati può essere affetta dalla contaminazione di poche stelle brillanti, in q
APA, Harvard, Vancouver, ISO, and other styles
2

Weldrake, David Thomas Frederick. "Giant planets and variable stars in globular clusters /." View thesis entry in Australian Digital Theses Program, 2005. http://thesis.anu.edu.au/public/adt-ANU20050616.191315/index.html.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Bradnick, Benjamin Thomas George. "On the dynamics in planetary systems, globular clusters and galactic nuclei." Thesis, University of Birmingham, 2017. http://etheses.bham.ac.uk//id/eprint/7826/.

Full text
Abstract:
N-body simulations are used to investigate the dynamics of planetary systems based on the observed period-radius distribution by Kepler. The stability of the distri- bution is tested using integrations of 2,000 systems and with the addition of a Jupiter-like perturber in an aligned and inclined configuration sufficient for Lidov- Kozai (LK) oscillations. ∼ 67% of planetary systems are found stable, falling to ∼ 62% and ∼ 48% with an aligned or inclined giant perturber. Planet ejections are rare. Instability timescales of systems are predicted by spacing and multiplicity of planets, but excepti
APA, Harvard, Vancouver, ISO, and other styles
4

Souza, Juliana Crestani Ribeiro de. "Spatial distribution of galactic globular clusters : distance uncertainties and dynamical effects." reponame:Biblioteca Digital de Teses e Dissertações da UFRGS, 2017. http://hdl.handle.net/10183/156776.

Full text
Abstract:
Fornecemos uma amostra de 170 Aglomerados Globulares Galácticos (GCs) e analisamos as propriedades de sua distribuição espacial. Utilizando um vasto catálogo de nuvens escuras identificadas, listamos os GCs que estão atrás de uma ou mais delas e que podem estar submetidos a uma extinção mais complexa do que a considerada por mapas de extinção. Valores de incerteza em distância são obtidos da literatura recente e comparados com valores derivados de uma fórmula de propagação de erro. GCs são agrupados de acordo com características inusitadas, tais como idades relativamente jovens ou possível con
APA, Harvard, Vancouver, ISO, and other styles
5

Pooley, David Aaron 1976. "Very old and very young compact objects : X-ray studies of galactic globular clusters and recent core-collapse supernovae." Thesis, Massachusetts Institute of Technology, 2003. http://hdl.handle.net/1721.1/29309.

Full text
Abstract:
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2003.<br>Includes bibliographical references.<br>This thesis comprises the results of two distinct areas of research, namely, X-ray studies of Galactic globular clusters and X-ray studies of recent core collapse supernovae. My analyses of the Chandra X-ray Observatory observations of the globular clusters NGC 6752 and NGC 6440 revealed as many low-luminosity X-ray sources as was in the entire census of globular cluster sources with the previous best X-ray imaging instrument, Rontgensatellit. In the observation of NGC 675
APA, Harvard, Vancouver, ISO, and other styles
6

Kamann, Sebastian. "Crowded field spectroscopy and the search for intermediate-mass black holes in globular clusters." Phd thesis, Universität Potsdam, 2013. http://opus.kobv.de/ubp/volltexte/2013/6776/.

Full text
Abstract:
Globular clusters are dense and massive star clusters that are an integral part of any major galaxy. Careful studies of their stars, a single cluster may contain several millions of them, have revealed that the ages of many globular clusters are comparable to the age of the Universe. These remarkable ages make them valuable probes for the exploration of structure formation in the early universe or the assembly of our own galaxy, the Milky Way. A topic of current research relates to the question whether globular clusters harbour massive black holes in their centres. These black holes would brid
APA, Harvard, Vancouver, ISO, and other styles
7

Dias, Bruno Moreira de Souza. "Formation and evolution of globular clusters in the Galaxy and Magellanic Clouds." Universidade de São Paulo, 2014. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-26082014-090039/.

Full text
Abstract:
Globular clusters are tracers of the formation and evolution of their host galaxies. Kinematics, chemical abundances, age and position of the clusters allows tracing interactions between Milky Way and surrounding galaxies and outlines their chemical enrichment history. In this thesis we analyse mid-resolution spectra of about 800 red giant stars in 51 Galactic globular clusters. It is the first time that [Fe/H] and [Mg/Fe] derived in a consistent way are published for such a huge sample of globular clusters, almost 1/3 of the total number of catalogued clusters. Our metallicities are showed to
APA, Harvard, Vancouver, ISO, and other styles
8

Bellini, Andrea, Mattia Libralato, Luigi R. Bedin та ін. "The HST Large Programme on ω Centauri. II. Internal Kinematics". IOP PUBLISHING LTD, 2018. http://hdl.handle.net/10150/627043.

Full text
Abstract:
In this second installment of the series, we look at the internal kinematics of the multiple stellar populations of the globular cluster omega Centauri in one of the parallel Hubble Space Telescope (HST) fields, located at about 3.5 hal-flight radii from the center of the cluster. Thanks to the over 15 yr long baseline and the exquisite astrometric precision of the HST cameras, well-measured stars in our proper-motion catalog have errors as low as similar to 10 mu as yr(-1), and the catalog itself extends to near the hydrogen-burning limit of the cluster. We show that second-generation (2G) st
APA, Harvard, Vancouver, ISO, and other styles
9

Libralato, Mattia, Andrea Bellini, Luigi R. Bedin та ін. "The HST Large Programme on ω Centauri. III. Absolute Proper Motion". IOP PUBLISHING LTD, 2018. http://hdl.handle.net/10150/627099.

Full text
Abstract:
In this paper, we report a new estimate of the absolute proper motion (PM) of the globular cluster NGC 5139 (omega Cen) as part of the HST large program GO-14118+ 14662. We analyzed a field 17 arcmin southwest of the center of omega Cen and computed PMs with epoch spans of similar to 15.1 years. We employed 45 background galaxies to link our relative PMs to an absolute reference-frame system. The absolute PM of the cluster in our field is (mu(alpha) cos delta, mu(delta))=(-3.341. 0.028, -6.557 +/- 0.043) mas yr(-1). Upon correction for the effects of viewing perspective and the known cluster r
APA, Harvard, Vancouver, ISO, and other styles
10

Frank, Matthias Johannes [Verfasser], and E. K. [Akademischer Betreuer] Grebel. "Observational Dynamics of Low-Mass Stellar Systems - The Mass Content of Ultra-Compact Dwarf Galaxies and Diffuse Globular Clusters / Matthias Johannes Frank ; Betreuer: E. K. Grebel." Heidelberg : Universitätsbibliothek Heidelberg, 2012. http://d-nb.info/1177808978/34.

Full text
APA, Harvard, Vancouver, ISO, and other styles

Books on the topic "Globular Clusters Core Dynamics"

1

Lupton, Robert Hugh. The dynamics and stellar content of globular star clusters. University Microfilms International, 1986.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
2

Stefan, Deiters, ed. Dynamics of star clusters and the Milky Way: Proceedings of the international spring Meeting of Astronomische Gesellschaft to celebrate the 300th anniversary of the "Calendar Edict" foundation document of Astronomisches Rechen-Institut held in Heidelberg, Germany, 20-24 March 2000. Astronomical Society of the Pacific, 2001.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
3

1956-, Goodman Jeremy, and Hut Piet 1952-, eds. Dynamics of star clusters: Proceedings of the 113th Symposium of the International Astronomical Union, held in Princeton, New Jersey, U.S.A., 29 May-1 June, 1984. D. Reidel Pub. Co., 1985.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
4

Merritt, David Roy. Dynamics of dense stellar systems: Proceedings of a workshop held at the University of Toronto, May 27-28, 1988. Cambridge University Press, 1989.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
5

Symposium, International Astronomical Union. Dynamical evolution of star clusters: Confrontation of theory and observations : proceedings of the 174th Symposium of the International Astronomical Union, held in Tokyo, Japan, August 22-25, 1995. Kluwer Academic Publishers, 1996.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
6

Symposium, International Astronomical Union. Dynamical evolution of star clusters: Confrontation of theory and observations : proceedings of the 174th Symposium of the International Astronomical Union, held in Tokyo, Japan, 22 August-25 August, 1995. Kluwer Academic Publishers, 1996.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
7

Structure and dynamics of globular clusters. Astronomical Society of the Pacific, 1993.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
8

David, Merritt, ed. Dynamics of dense stellar systems. Cambridge University Press, 1989.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
9

(Editor), Piet Hut, and Junichiro Makino (Editor), eds. Dynamical Evolution of Star Clusters - Confrontation of Theory and Observations (International Astronomical Union Symposia). Springer, 1996.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
10

Heggie, Douglas, and Piet Hut. The Gravitational MillionBody Problem: A Multidisciplinary Approach to Star Cluster Dynamics. Cambridge University Press, 2003.

Find full text
APA, Harvard, Vancouver, ISO, and other styles

Book chapters on the topic "Globular Clusters Core Dynamics"

1

Heggie, Douglas C. "Dynamical Evolution of Globular Clusters After Core Collapse." In Dynamics of Star Clusters. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5335-2_19.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Aurière, M., J. P. Cordoni, O. Le Fèvre, and A. Terzan. "A High Spatial Resolution Investigation of the Core of Some Dynamically Evolved Globular Clusters." In Dynamics of Star Clusters. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5335-2_5.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Lugger, Phyllis M., Haldan Cohn, and Jonathan E. Grindlay. "Where’s the CUSP? (Or CCD Photometry of Globular Cluster Cores)." In Dynamics of Star Clusters. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5335-2_12.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Spitzer, Lyman. "Precollapse Evolution of Globular Clusters." In Dynamics of Star Clusters. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5335-2_18.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Freeman, K. C. "Chemical Gradients in Globular Clusters." In Dynamics of Star Clusters. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5335-2_3.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Seitzer, P. "Tidal Effects on Globular Clusters." In Dynamics of Star Clusters. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5335-2_42.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Larson, R. B. "Are Our Globular Clusters Coeval?" In Dynamics and Interactions of Galaxies. Springer Berlin Heidelberg, 1990. http://dx.doi.org/10.1007/978-3-642-75273-5_7.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Fall, S. Michael, and Carlos S. Frenk. "Rotation and Flattening of Globular Clusters." In Dynamics of Star Clusters. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5335-2_29.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Lupton, Robert. "3-Integral Models for Globular Clusters." In Dynamics of Star Clusters. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5335-2_38.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Larson, Richard B. "Black-Hole Remnants in Globular Clusters." In Dynamics of Star Clusters. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5335-2_48.

Full text
APA, Harvard, Vancouver, ISO, and other styles

Conference papers on the topic "Globular Clusters Core Dynamics"

1

Merafina, Marco. "Does the core collapse in globular clusters onset before than commonly believed?" In XII Multifrequency Behaviour of High Energy Cosmic Sources Workshop. Sissa Medialab, 2018. http://dx.doi.org/10.22323/1.306.0004.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Zhang, Jiapei, Wei Li, Zhangcan Yang, and Yingzhao He. "Molecular Dynamics Simulation of Diffusion and Aggregation Behavior of Helium in Tungsten Bulk Materials." In ASME 2019 6th International Conference on Micro/Nanoscale Heat and Mass Transfer. American Society of Mechanical Engineers, 2019. http://dx.doi.org/10.1115/mnhmt2019-3947.

Full text
Abstract:
Abstract Controlled thermonuclear fusion is a promising project. If it can be realized, it will certainly replace fossil fuels and solve the problem of energy exhaustion facing humanity. The fusion reaction fuel is a light core, which can be extracted from sea water. The source is very rich, and the fusion reaction of hydrogen and its isotopes is not radioactive, so the fusion energy can be efficient, cheap and clean. At present, the realization of this technology still faces many difficult problems that have not been overcome. The Tokamak device is the most promising device for realizing the
APA, Harvard, Vancouver, ISO, and other styles
3

Mintu, Shafiul A., and David Molyneux. "Application of GPGPU to Accelerate CFD Simulation." In ASME 2018 37th International Conference on Ocean, Offshore and Arctic Engineering. American Society of Mechanical Engineers, 2018. http://dx.doi.org/10.1115/omae2018-77649.

Full text
Abstract:
Computational Fluid Dynamics (CFD) is widely used in industry and academic research to investigate complex fluid flow. The bottleneck of a realistic CFD simulation is its long simulation time. The simulation time is generally reduced by massively parallel Central Processing Unit (CPU) clusters, which are very expensive. In this paper, it is shown that the CFD simulation can be accelerated significantly by a novel hardware called General Purpose Computing on Graphical Processing Units (GPGPU). GPGPU is a cost-effective computing cluster, which uses the Compute Unified Device Architecture (CUDA)
APA, Harvard, Vancouver, ISO, and other styles
4

Abu-Shams, Mohammad, and Ishraq Shabib. "Irradiation Induced Damage of Fe-10%Cr Under Uniaxial Pressure." In ASME 2015 International Mechanical Engineering Congress and Exposition. American Society of Mechanical Engineers, 2015. http://dx.doi.org/10.1115/imece2015-51686.

Full text
Abstract:
Structural materials of next generation nuclear reactors are expected to experience severe operating conditions including intense heat, high irradiation doses, thermal and mechanical stresses, and corrosive environments, which would potentially degrade material properties and impose severe threat to structural integrity. For example, high irradiation doses cause the evolution of displacement cascades, consisting of point defects, which lead to void swelling, irradiation creep, irradiation assisted stress corrosion cracking, and embrittlement. Over the last several decades, extensive computatio
APA, Harvard, Vancouver, ISO, and other styles
You might also be interested in the extended bibliographies on the topic 'Globular Clusters Core Dynamics' for particular source types:
Journal articles
We offer discounts on all premium plans for authors whose works are included in thematic literature selections. Contact us to get a unique promo code!

To the bibliography