Bibliographies thématiques / Cosmology Mathematical models

Sommaire

  1. Articles de revues
  2. Thèses
  3. Livres
  4. Chapitres de livres
  5. Actes de conférences

Littérature scientifique sur le sujet « Cosmology Mathematical models »

Auteur : Grafiati
Publié le 4 juin 2021
Mis à jour le 28 janvier 2023

Créez une référence correcte selon les styles APA, MLA, Chicago, Harvard et plusieurs autres

Choisissez une source :

Consultez les listes thématiques d’articles de revues, de livres, de thèses, de rapports de conférences et d’autres sources académiques sur le sujet « Cosmology Mathematical models ».

À côté de chaque source dans la liste de références il y a un bouton « Ajouter à la bibliographie ». Cliquez sur ce bouton, et nous générerons automatiquement la référence bibliographique pour la source choisie selon votre style de citation préféré : APA, MLA, Harvard, Vancouver, Chicago, etc.

Vous pouvez aussi télécharger le texte intégral de la publication scolaire au format pdf et consulter son résumé en ligne lorsque ces informations sont inclues dans les métadonnées.

Articles de revues sur le sujet "Cosmology Mathematical models"

1

Christianto, Victor, et Yunita Umniyati. « Remark on ‘The future of mathematical Cosmology” and “100 years of mathematical cosmology : Models, theories and problems, Part B” by S. Cotsakis and A.P. Yefremov ». Journal of Cosmology, Filaments and Astrobiology 2, no 1 (2022) : 38–41. http://dx.doi.org/10.54216/jcfa.020105.

Texte intégral
Résumé :
In this review article, allow us to offer a few remark on “the future of mathematical cosmology” “100 years of mathematical cosmology: Models, theories and problems, Part B” by Cotsakis and Yefremov, which seems to us very interesting piece of review on progress on the last 3 or 4 decades in theoretical cosmology development. In particular, we would emphasize on testability of cosmology models, which seem to us this criterion can only be achieved via correspondence between condensed mattersuperfluiditylow temperature physics and cosmology (cf. for instance, Kibble Pickett, 2008).
Styles APA, Harvard, Vancouver, ISO, etc.
2

Tzvi Langermann, Y. « Arabic Cosmology ». Early Science and Medicine 2, no 2 (1997) : 185–213. http://dx.doi.org/10.1163/157338297x00113.

Texte intégral
Résumé :
AbstractRepresentations of the heavens in various levels of detail can be found in a number of branches of Arabic literature. One particular genre, the hay'a texts, has as its purpose a full though non-mathematical discussion of the arrangement of the celestial orbs; hay'a writers are particularly sensitive to the philosophical requirements which all systems must meet. The pivotal work in this genre, On the Configuration, was written by Ibn al-Haytham. Later writers continued to produce works in the spirit of On the Configuration. In the east, al-Tusi and his followers developed new models; in the west, a group of thinkers tried to rediscover the models which, so they thought, were the ones endorsed by Aristotle himself.
Styles APA, Harvard, Vancouver, ISO, etc.
3

Elizaga Navascués, Beatriz, Mercedes Martín-Benito et Guillermo A. Mena Marugán. « Hybrid models in loop quantum cosmology ». International Journal of Modern Physics D 25, no 08 (juillet 2016) : 1642007. http://dx.doi.org/10.1142/s0218271816420074.

Texte intégral
Résumé :
In the framework of Loop Quantum Cosmology (LQC), inhomogeneous models are usually quantized by means of a hybrid approach that combines loop quantization techniques with standard quantum field theory methods. This approach is based on a splitting of the phase space in a homogeneous sector, formed by global, zero-modes and an inhomogeneous sector, formed by the remaining, infinite number of modes, that describe the local degrees of freedom. Then, the hybrid quantization is attained by adopting a loop representation for the homogeneous gravitational sector, while a Fock representation is used for the inhomogeneities. The zero-mode of the Hamiltonian constraint operator couples the homogeneous and inhomogeneous sectors. The hybrid approach, therefore, is expected to provide a suitable quantum theory in regimes where the main quantum effects of the geometry are those affecting the zero-modes, while the inhomogeneities, still being quantum, can be treated in a more conventional way. This hybrid strategy was first proposed for the simplest cosmological midisuperspaces: the Gowdy models, and it has been later applied to the case of cosmological perturbations. This paper reviews the construction and main applications of hybrid LQC.
Styles APA, Harvard, Vancouver, ISO, etc.
4

DEL CAMPO, SERGIO, RAMÓN HERRERA et JOEL SAAVEDRA. « CLOSED INFLATIONARY UNIVERSE MODELS IN BRANE WORLD COSMOLOGY ». International Journal of Modern Physics D 14, no 05 (mai 2005) : 861–72. http://dx.doi.org/10.1142/s0218271805007036.

Texte intégral
Résumé :
In this article we study closed inflationary universe models proposed by Linde in a brane world cosmological context. In this scenario we determine and characterize the existence of a closed universe, in presence of one self-interacting scalar field with an inflationary stage. We have found that our model, which takes into account a Brane World Cosmology, is less restrictive than the one that uses standard Einstein's General Relativity cosmology.
Styles APA, Harvard, Vancouver, ISO, etc.
5

COLEY, A. A. « BRANE-WORLD COSMOLOGY ». International Journal of Modern Physics D 11, no 10 (décembre 2002) : 1609–14. http://dx.doi.org/10.1142/s0218271802002979.

Texte intégral
Résumé :
It is argued that typically the initial singularity is isotropic in brane world cosmological models. Consequently brane cosmology naturally gives rise to a set of initial data that provide the conditions for inflation to subsequently take place, leading to a self-consistent and viable cosmological scenario.
Styles APA, Harvard, Vancouver, ISO, etc.
6

SAHNI, VARUN, et YURI SHTANOV. « NEW VISTAS IN BRANEWORLD COSMOLOGY ». International Journal of Modern Physics D 11, no 10 (décembre 2002) : 1515–21. http://dx.doi.org/10.1142/s0218271802002827.

Texte intégral
Résumé :
Traditionally, higher-dimensional cosmological models have sought to provide a description of the fundamental forces in terms of a unifying geometrical construction. In this essay we discuss how, in their present incarnation, higher-dimensional "braneworld" models might provide answers to a number of cosmological puzzles including the issue of dark energy and the nature of the big bang singularity.
Styles APA, Harvard, Vancouver, ISO, etc.
7

MACÍAS, ALFREDO, ECKEHARD W. MIELKE et JOSÉ SOCORRO. « SUPERSYMMETRIC QUANTUM COSMOLOGY FOR BIANCHI CLASS A MODELS ». International Journal of Modern Physics D 07, no 05 (octobre 1998) : 701–12. http://dx.doi.org/10.1142/s0218271898000462.

Texte intégral
Résumé :
The canonical theory of [Formula: see text] supergravity, with a matrix representation for the gravitino covector–spinor, is applied to the Bianchi class A spatially homogeneous cosmologies. The full Lorentz constraint and its implications for the wave function of the universe are analyzed in detail. We found that in this model no physical states other than the trivial "rest frame" type occur.
Styles APA, Harvard, Vancouver, ISO, etc.
8

Stornaiolo, Cosimo. « Tomographic analysis of quantum and classical de Sitter cosmological models ». International Journal of Modern Physics D 28, no 16 (15 octobre 2019) : 2040009. http://dx.doi.org/10.1142/s021827182040009x.

Texte intégral
Résumé :
In this work, we show the importance of introducing the quantum tomography formalism to analyze the properties of wave functions in quantum cosmology. In particular, we examine the initial conditions of the universe proposed by various authors in the context of de Sitter’s cosmology studying their classical limit and comparing it with the classical tomogram obtained from the Hamiltonian constraint in General Relativity. This comparison gives us the opportunity to find under which conditions there is a transition from the quantum universe to the classical one. A relevant result is that in these models the decay of the cosmological constant is a sufficient condition for this transition.
Styles APA, Harvard, Vancouver, ISO, etc.
9

Jawad, Abdul, Shamaila Rani, Ines G. Salako et Faiza Gulshan. « Pilgrim dark energy models in fractal universe ». International Journal of Modern Physics D 26, no 06 (22 novembre 2016) : 1750049. http://dx.doi.org/10.1142/s0218271817500493.

Texte intégral
Résumé :
We discuss the cosmological implications of interacting pilgrim dark energy (PDE) models (with Hubble, Granda–Oliveros and generalized ghost cutoffs) with cold dark matter ([Formula: see text]CDM) in fractal cosmology by assuming the flat universe. We observe that the Hubble parameter lies within observational suggested ranges while deceleration parameter represents the accelerated expansion behavior of the universe. The equation of state (EoS) parameter ([Formula: see text]) corresponds to the quintessence region and phantom region for different cases of [Formula: see text]. Further, we can see that [Formula: see text]–[Formula: see text] (where prime indicates the derivative with respect to natural logarithmic of scale factor) plane describes the freezing and thawing regions and also corresponds to [Formula: see text] limit for some cases of [Formula: see text] (PDE parameter). It is also noted that the [Formula: see text]–[Formula: see text] (state-finder parameters) plane corresponds to [Formula: see text] limit and also shows the Chaplygin as well as phantom/quintessence behavior. It is observed that pilgrim dark energy models in fractal cosmology expressed the consistent behavior with recent observational schemes.
Styles APA, Harvard, Vancouver, ISO, etc.
10

COTSAKIS, SPIROS. « STRUCTURE OF INFINITY IN COSMOLOGY ». International Journal of Modern Physics D 22, no 03 (mars 2013) : 1330003. http://dx.doi.org/10.1142/s0218271813300036.

Texte intégral
Résumé :
We discuss recent developments related to certain blow-up methods suitable for the analysis of cosmological singularities and asymptotics. We review results obtained in a variety of currently popular themes and describe ongoing research about universes with various kinds of extreme states, higher-order gravity and certain models of braneworlds.
Styles APA, Harvard, Vancouver, ISO, etc.
Plus de sources

Thèses sur le sujet "Cosmology Mathematical models"

1

Hervik, Sigbjørn. « Mathematical cosmology : Bianchi models, asymptotics and extra dimensions ». Thesis, University of Cambridge, 2004. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.616093.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
2

Campbell, Robert Alan. « Inhomogeneous conformal cosmological models / ». Title page, contents and summary only, 1985. http://web4.library.adelaide.edu.au/theses/09PH/09phc1888.pdf.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
3

Dechant, Pierre-Philippe. « Models of the early universe ». Thesis, University of Cambridge, 2011. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.609618.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
4

Ng, Shao-Chin Cindy. « Cosmological models with quintessence : dynamical properties and observational constraints ». Title page, table of contents and abstract only, 2001. http://web4.library.adelaide.edu.au/theses/09PH/09phn5758.pdf.

Texte intégral
Résumé :
Bibliography: leaves 100-106. Studies different models of "quintessence", in particular, a quintessence arising from an ultra-light pseudo Nambu-Goldstone boson. Overviews dynamical properties for these models using phase-space analyses to study attractor and tracker solutions. Studies high-redshift type Ia supernovae constraints on these models. Studies the impact of a simple phenomenological model for supernovae luminosity evolution on the PNGB models and the potentials of a future supernovae data set to discriminate the PNGB models over the other quintessence models. Studies gravitational lensing statistics of high luminosity quasars upon the quintessence models.
Styles APA, Harvard, Vancouver, ISO, etc.
5

Luo, Xianghui 1983. « Symmetries of Cauchy Horizons and Global Stability of Cosmological Models ». Thesis, University of Oregon, 2011. http://hdl.handle.net/1794/11543.

Texte intégral
Résumé :
ix, 111 p.
This dissertation contains the results obtained from a study of two subjects in mathematical general relativity. The first part of this dissertation is about the existence of Killing symmetries in spacetimes containing a compact Cauchy horizon. We prove the existence of a nontrivial Killing symmetry in a large class of analytic cosmological spacetimes with a compact Cauchy horizon for any spacetime dimension. In doing so, we also remove the restrictive analyticity condition and obtain a generalization to the smooth case. The second part of the dissertation presents our results on the global stability problem for a class of cosmological models. We investigate the power law inflating cosmological models in the presence of electromagnetic fields. A stability result for such cosmological spacetimes is proved. This dissertation includes unpublished co-authored material.
Committee in charge: James Brau, Chair; James Isenberg, Advisor; Paul Csonka, Member; John Toner, Member; Peng Lu, Outside Member
Styles APA, Harvard, Vancouver, ISO, etc.
6

Foster, Scott. « Singularity structure of scalar field cosmologies / ». Title page, contents and abstract only, 1996. http://web4.library.adelaide.edu.au/theses/09PH/09phf757.pdf.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
7

Howell, Eric John. « The characterization and temporal distribution of cosmological gravitational wave treatments ». University of Western Australia. School of Physics, 2009. http://theses.library.uwa.edu.au/adt-WU2010.0095.

Texte intégral
Résumé :
[Truncated abstract] As gravitational wave detectors approach sensitivities that will allow observations to become routine, astrophysics lies on the cusp of an exciting new era. Potential sources will include transients such as merging neutron stars and black holes, supernova explosions or the engines that power gamma-ray bursts. This thesis will be devoted to the astrophysical gravitational wave background signal produced by cosmological populations of such transient signals. Particular attention will be devoted to the observation-time dependence imposed on the individual sources that accumulate to produce a gravitational wave background signal. The ultimate aim is to determine what information is encoded in the temporal evolution of such a signal. To lay the foundations for further investigation, the stochastic gravitational wave background signal from neutron star birth throughout the Universe has been calculated. In view of the uncertainties in both the single-source emissions and source rate histories, several models of each are employed. The results show that that the resulting signals are only weakly dependent on the source-rate evolution model and that prominent features in the single-source spectra can be related to the background spectra. In comparison with previous studies, the use of relativistic single-source gravitational wave waveforms rather than Newtonian models and a more slowly evolving source-rate density results in a 1 { 2 order of magnitude reduction in signal. ... A comparison with the more commonly used brightness distribution of events shows that when applying both methods to a data stream containing a background of Gaussian distributed false alarms, the brightness distribution yielded lower standard errors, but was biased by the false alarms. In comparison, a fitting procedure based on the time evolution of events was less prone to errors resulting from false alarms, but as fewer events contributed to the data, had a lower resolution. In further support of the time dependent signature of transient events, an alternative technique is fiapplied to the same source population. In this case, the local rate density is probed by measuring the statistical compatibility of the filtered data against synthetic time dependent data. Although this method is not as compact as the fitting procedure, the rate estimates are compatible. To further investigate how the observation time dependence of transient populations can be used to constrain global parameters, the method is applied to Swift long gamma-ray burst data. By considering a distribution in peak °ux rather than a gravitational wave amplitude, gamma-ray bursts can be considered as a surrogate for resolved gravitational wave transients. For this application a peak °ux{observation time relation is described that takes the form of a power law that is invariant to the luminosity distribution of the sources. Additionally, the method is enhanced by invoking time reversal invariance and the temporal cosmological principle. Results are presented to show that the peak °ux{observation time relation is in good agreement with recent estimates of source parameters. Additionally, to show that the intrinsic time dependence allows the method to be used as a predictive tool, projections are made to determine the upper limits in peak °ux of future gamma-ray burst detections for Swift.
Styles APA, Harvard, Vancouver, ISO, etc.
8

Osano, Bob Otieno. « Beyond the standard model of cosmology : a perturbative approach ». Doctoral thesis, University of Cape Town, 2007. http://hdl.handle.net/11427/4918.

Texte intégral
Résumé :
Includes abstract.
Includes bibliographical references (p. 171-185).
This thesis concerns higher order perturbations of the standard model of cosmology. The theme is addressed in two distinct research areas. The first area deals with linear perturbations of Bianchi type I model filled with dust whose flow is irrotational, and which is an analogue to second order perturbations about the standard model. We investigate both density perturbations and gravitational waves in the shear dominated and the matter dominated regimes. We find that whereas the analysis of the perturbations in the matter dominated regime recovers the standard FLRW results, the analysis of perturbations in the shear dominated regime reveals that density perturbations and gravitational waves decouple only when the background shear is locally rotational symmetric.
Styles APA, Harvard, Vancouver, ISO, etc.
9

Delbem, Nilton Flávio [UNESP]. « Introdução matemática aos modelos cosmológicos ». Universidade Estadual Paulista (UNESP), 2010. http://hdl.handle.net/11449/94340.

Texte intégral
Résumé :
Made available in DSpace on 2014-06-11T19:27:09Z (GMT). No. of bitstreams: 0 Previous issue date: 2010-10-15Bitstream added on 2014-06-13T20:47:45Z : No. of bitstreams: 1 delbem_nf_me_rcla.pdf: 885461 bytes, checksum: 9ba35dff1d53b0378c1e134087c575b7 (MD5)
Universidade Estadual Paulista (UNESP)
Esta dissertação tem a proposta de organizar, discutir e apresentar de maneira precisa os conceitos matemáticos de variedade diferenciável e de tensores envolvidos no estudo da Cosmologia sob o ponto de vista da Teoria da Relatividade Geral para o modelo de Friedmann-Lemaître-Robertson-Walker. Busca-se assim apresentar um texto didático que possa ser utilizado tanto nos cursos de graduação em Matemática como de Física para uma disciplina optativa de Introdução Matemática à Cosmologia
The goal of this dissertation is to organize and discuss in a rigorous way the mathematical concepts of manifolds and tensors needed to the study of Cosmology and the Friedmann-Lemaître-Robertson-Walker model under the point of view of the General Relativity. In this way, this dissertation was written as textbook that could be used in an undergraduate course of Physics and Mathematics
Styles APA, Harvard, Vancouver, ISO, etc.
10

Delbem, Nilton Flávio. « Introdução matemática aos modelos cosmológicos / ». Rio Claro : [s.n.], 2010. http://hdl.handle.net/11449/94340.

Texte intégral
Résumé :
Orientador: Wladimir Seixas
Banca: Manoel Borges Ferreira Neto
Banca: Henrique Lazari
Resumo: Esta dissertação tem a proposta de organizar, discutir e apresentar de maneira precisa os conceitos matemáticos de variedade diferenciável e de tensores envolvidos no estudo da Cosmologia sob o ponto de vista da Teoria da Relatividade Geral para o modelo de Friedmann-Lemaître-Robertson-Walker. Busca-se assim apresentar um texto didático que possa ser utilizado tanto nos cursos de graduação em Matemática como de Física para uma disciplina optativa de Introdução Matemática à Cosmologia
Abstract: The goal of this dissertation is to organize and discuss in a rigorous way the mathematical concepts of manifolds and tensors needed to the study of Cosmology and the Friedmann-Lemaître-Robertson-Walker model under the point of view of the General Relativity. In this way, this dissertation was written as textbook that could be used in an undergraduate course of Physics and Mathematics
Mestre
Styles APA, Harvard, Vancouver, ISO, etc.
Plus de sources

Livres sur le sujet "Cosmology Mathematical models"

1

Arcidiacono, Giuseppe. Projective relativity, cosmology, and gravitation. Nonantum, Mass., U.S.A : Hadronic Press, 1986.

Trouver le texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
2

Chemical cosmology. Dordrecht : Springer, 2010.

Trouver le texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
3

Krasiński, Andrzej. Inhomogeneous cosmological models. Cambridge, UK : Cambridge University Press, 1996.

Trouver le texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
4

Krasiński, Andrzej. Inhomogeneous cosmological models. Cambridge : Cambridge University Press, 2006.

Trouver le texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
5

1963-, Cotsakis Spiros, et Papantonopoulos E, dir. Cosmological crossroads : An advanced course in mathematical, physical, and string cosmology. Berlin : Springer, 2002.

Trouver le texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
6

Scheen, Christian. Contribution à l'étude de la dynamique de modèles cosmologiques anistropes au voisinage de la singularité initiale. [Bruxelles] : Académie royale de Belgique, 2001.

Trouver le texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
7

Tifft, W. G., et W. J. Cocke, dir. Modern Mathematical Models of Time and their Applications to Physics and Cosmology. Dordrecht : Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5628-8.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
8

Cosmology in (2+1)- dimensions, cyclic models, and deformations of M2,1. Princeton, N.J : Princeton University Press, 1989.

Trouver le texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
9

A, Molina, et Senovilla J. M. M, dir. Proceedings of the Spanish Relativity Meeting on Inhomogeneous Cosmological Models. Singapore : World Scientific, 1995.

Trouver le texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
10

Pekka, Teerikorpi, et SpringerLink (Online service), dir. Fundamental Questions of Practical Cosmology : Exploring the Realm of Galaxies. Dordrecht : Springer Science+Business Media B.V., 2012.

Trouver le texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
Plus de sources

Chapitres de livres sur le sujet "Cosmology Mathematical models"

1

Kokus, Martin. « Spherical Rotation, Particles and Cosmology ». Dans Modern Mathematical Models of Time and their Applications to Physics and Cosmology, 353–56. Dordrecht : Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5628-8_30.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
2

Tifft, W. G. « Three-Dimensional Quantized Time in Cosmology ». Dans Modern Mathematical Models of Time and their Applications to Physics and Cosmology, 187–210. Dordrecht : Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5628-8_16.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
3

Keresztes, Z., M. Forsberg, M. Bradley, P. K. S. Dunsby et L. Á. Gergely. « Perturbations of Kantowski–Sachs Models with a Cosmological Constant ». Dans Progress in Mathematical Relativity, Gravitation and Cosmology, 289–93. Berlin, Heidelberg : Springer Berlin Heidelberg, 2013. http://dx.doi.org/10.1007/978-3-642-40157-2_40.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
4

Rozas-Fernández, Alberto, Marco Bruni et Ruth Lazkoz. « Phenomenology of Unified Dark Matter Models with Fast Transition ». Dans Progress in Mathematical Relativity, Gravitation and Cosmology, 387–90. Berlin, Heidelberg : Springer Berlin Heidelberg, 2013. http://dx.doi.org/10.1007/978-3-642-40157-2_58.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
5

Radicella, Ninfa, Vincenzo F. Cardone et Stefano Camera. « Accelerating f(T) Gravity Models Constrained by Recent Cosmological Data ». Dans Progress in Mathematical Relativity, Gravitation and Cosmology, 367–70. Berlin, Heidelberg : Springer Berlin Heidelberg, 2013. http://dx.doi.org/10.1007/978-3-642-40157-2_54.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
6

Arp, Halton. « The Pair of X-ray Sources across NGC 4258 : Its Relation to Intrinsic Redshifts, Ejection and Quantization ». Dans Modern Mathematical Models of Time and their Applications to Physics and Cosmology, 9–22. Dordrecht : Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5628-8_1.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
7

Napier, W. M., et B. N. G. Guthrie. « Testing for Quantized Redshifts. II. The Local Supercluster ». Dans Modern Mathematical Models of Time and their Applications to Physics and Cosmology, 111–26. Dordrecht : Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5628-8_10.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
8

Newman, W. I., et Y. Terzian. « Power Spectrum Analysis and Redshift Data ». Dans Modern Mathematical Models of Time and their Applications to Physics and Cosmology, 127–41. Dordrecht : Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5628-8_11.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
9

Cocke, W. J., C. L. Devito et A. Pitucco. « Statistical Analysis of the Occurrence of Periodicities in Galaxy Redshift Data ». Dans Modern Mathematical Models of Time and their Applications to Physics and Cosmology, 143–57. Dordrecht : Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5628-8_12.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
10

Sturrock, P. A. « Zooming in on the Redshift Problem ». Dans Modern Mathematical Models of Time and their Applications to Physics and Cosmology, 159–66. Dordrecht : Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5628-8_13.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.

Actes de conférences sur le sujet "Cosmology Mathematical models"

1

Ignat'ev, Yu G., A. A. Agathonov, M. L. Mikhailov et D. Yu Ignatyev. « Mathematical models of cosmological evolution of statistical system of scalar charged particles ». Dans Twelfth Asia-Pacific International Conference on Gravitation, Astrophysics, and Cosmology. WORLD SCIENTIFIC, 2016. http://dx.doi.org/10.1142/9789814759816_0009.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
2

Pérez-Lorenzana, Abdel. « Cosmological Radion Problem in Models with Extra Dimensions ». Dans GRAVITATION AND COSMOLOGY : 2nd Mexican Meeting on Mathematical and Experimental Physics. AIP, 2005. http://dx.doi.org/10.1063/1.1900519.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
3

Sussman, Roberto A. « Scalar averaging in Szekeres dust models ». Dans IX MEXICAN SCHOOL ON GRAVITATION AND MATHEMATICAL PHYSICS : COSMOLOGY FOR THE XXIST CENTURY : Gravitation and Mathematical Physics Division of the Mexican Physical Society (DGFM-SMF). AIP, 2013. http://dx.doi.org/10.1063/1.4817058.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
4

Hernández-Aguayo, César, Arturo Avelino et L. Arturo Ureña-López. « Cosmological constraints on the roll parameter of freezing and thawing quintessence models ». Dans IX MEXICAN SCHOOL ON GRAVITATION AND MATHEMATICAL PHYSICS : COSMOLOGY FOR THE XXIST CENTURY : Gravitation and Mathematical Physics Division of the Mexican Physical Society (DGFM-SMF). AIP, 2013. http://dx.doi.org/10.1063/1.4817054.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
5

Gómez, L. Gabriel, et Yeinzon Rodríguez. « Statistical anisotropy in inflationary models with many vector fields and/or prolonged anisotropic expansion ». Dans IX MEXICAN SCHOOL ON GRAVITATION AND MATHEMATICAL PHYSICS : COSMOLOGY FOR THE XXIST CENTURY : Gravitation and Mathematical Physics Division of the Mexican Physical Society (DGFM-SMF). AIP, 2013. http://dx.doi.org/10.1063/1.4817056.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
6

Cortez, Jerónimo, William Cuervo et Hugo A. Morales-Técotl. « On the geometric resolution of the Schwarzschild black hole singularity within effective loop quantum gravity models ». Dans IX MEXICAN SCHOOL ON GRAVITATION AND MATHEMATICAL PHYSICS : COSMOLOGY FOR THE XXIST CENTURY : Gravitation and Mathematical Physics Division of the Mexican Physical Society (DGFM-SMF). AIP, 2013. http://dx.doi.org/10.1063/1.4817038.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
7

Muñoz-Andrade, Juan Daniel. « A Mathematical Model for Plasticity and Cosmology ». Dans MATERIALS PROCESSING AND DESIGN ; Modeling, Simulation and Applications ; NUMIFORM '07 ; Proceedings of the 9th International Conference on Numerical Methods in Industrial Forming Processes. AIP, 2007. http://dx.doi.org/10.1063/1.2740995.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
8

Socorro, J., Juan M. Ramírez, Luis O. Pimentel, Gustavo López et Rafael Hernández. « Searching solutions by Lagrange-Charpit method in cosmology : Bianchi type I toy model in self creation cosmology ». Dans RECENT DEVELOPMENTS ON PHYSICS IN STRONG GRAVITATIONAL FIELDS : V Leopoldo García-Colín Mexican Meeting on Mathematical and Experimental Physics. AIP Publishing LLC, 2014. http://dx.doi.org/10.1063/1.4861961.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
9

Khadekar, G. S., Vaishali Kamdi et Vitthal Miskin. « HIGHER DIMENSIONAL COSMOLOGI CAL MODEL OF THE UNIVERSE WITH VARIABLE EQUTION OF STATE PARAMETER IN THE PRESENCE OF G AND Λ ». Dans ICMS INTERNATIONAL CONFERENCE ON MATHEMATICAL SCIENCE. American Institute of Physics, 2010. http://dx.doi.org/10.1063/1.3525180.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
10

Espinoza-García, Abraham, Omar Núñes et J. Socorro. « Quintom potentials from a quantum anisotropic model ». Dans IX MEXICAN SCHOOL ON GRAVITATION AND MATHEMATICAL PHYSICS : COSMOLOGY FOR THE XXIST CENTURY : Gravitation and Mathematical Physics Division of the Mexican Physical Society (DGFM-SMF). AIP, 2013. http://dx.doi.org/10.1063/1.4817050.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
Vous pouvez également être intéressé par les bibliographies sur le sujet « Cosmology Mathematical models » pour d’autres types de sources :
Articles de revues Thèses Livres
Nous offrons des réductions sur tous les plans premium pour les auteurs dont les œuvres sont incluses dans des sélections littéraires thématiques. Contactez-nous pour obtenir un code promo unique!

Vers la bibliographie