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Автор: Grafiati
Опубліковано: 14 березня 2023

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Статті в журналах з теми "Cosmology of the early Universe"

1

Sato, K. "The Very Early Universe." Transactions of the International Astronomical Union 20, no. 1 (1988): 656–58. http://dx.doi.org/10.1017/s0251107x00007495.

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In recent years, the research on the very early universe has shown quite remarkable developments. As is well known, this development was brought about by the introduction of the Grand Unified Theories (GUTs) into cosmology. These theories have not only enabled us to trace the evolution of the Universe back to the very early stage at temperatures of 1016 GeV or higher, but also introduced various new aspects into cosmology, such as baryogenesis, phase transitions and topological defects (monopoles, etc.). In particular, inflation, which grew out of the study of GUT phase transition, is the most important and fascinating outcome.
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2

Smeenk, Chris. "Predictability crisis in early universe cosmology." Studies in History and Philosophy of Science Part B: Studies in History and Philosophy of Modern Physics 46 (May 2014): 122–33. http://dx.doi.org/10.1016/j.shpsb.2013.11.003.

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3

Singh, C. P. "Bulk viscous cosmology in early Universe." Pramana 71, no. 1 (July 2008): 33–48. http://dx.doi.org/10.1007/s12043-008-0139-4.

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4

Krauss, Lawrence M. "New gravitational tests of early universe cosmology." General Relativity and Gravitation 18, no. 7 (July 1986): 723–30. http://dx.doi.org/10.1007/bf00768636.

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5

Maggiore, Michele. "Gravitational wave experiments and early universe cosmology." Physics Reports 331, no. 6 (July 2000): 283–367. http://dx.doi.org/10.1016/s0370-1573(99)00102-7.

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6

Bojowald, Martin. "The early universe in loop quantum cosmology." Journal of Physics: Conference Series 24 (January 1, 2005): 77–86. http://dx.doi.org/10.1088/1742-6596/24/1/010.

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7

Brevik, Iver, Øyvind Grøn, Jaume de Haro, Sergei D. Odintsov, and Emmanuel N. Saridakis. "Viscous cosmology for early- and late-time universe." International Journal of Modern Physics D 26, no. 14 (December 2017): 1730024. http://dx.doi.org/10.1142/s0218271817300245.

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From a hydrodynamicist’s point of view the inclusion of viscosity concepts in the macroscopic theory of the cosmic fluid would appear most natural, as an ideal fluid is after all an abstraction (exluding special cases such as superconductivity). Making use of modern observational results for the Hubble parameter plus standard Friedmann formalism, we may extrapolate the description of the universe back in time up to the inflationary era, or we may go to the opposite extreme and analyze the probable ultimate fate of the universe. In this review, we discuss a variety of topics in cosmology when it is enlarged in order to contain a bulk viscosity. Various forms of this viscosity, when expressed in terms of the fluid density or the Hubble parameter, are discussed. Furthermore, we consider homogeneous as well as inhomogeneous equations of state. We investigate viscous cosmology in the early universe, examining the viscosity effects on the various inflationary observables. Additionally, we study viscous cosmology in the late universe, containing current acceleration and the possible future singularities, and we investigate how one may even unify inflationary and late-time acceleration. Finally, we analyze the viscosity-induced crossing through the quintessence-phantom divide, we examine the realization of viscosity-driven cosmological bounces, and we briefly discuss how the Cardy–Verlinde formula is affected by viscosity.
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Kafatos, Menas. "Limitations of Observational Cosmology." International Astronomical Union Colloquium 123 (1990): 543–50. http://dx.doi.org/10.1017/s0252921100077642.

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AbstractUnlike the usual situation with theoretical physics which is testable in the laboratory, in cosmological theories of the universe one faces the following problems: The observer is part of the system, the universe, and this system cannot be altered to test physical theory. Even though one can in principle consider any part of the observable universe as separate from the acts of observation, the very hypothesis of big bang implies that in the distant past, space-time regions containing current observers were part of the same system. One, therefore, faces a situation where the observer has to be considered as inherently a part of the entire system. The existence of horizons of knowledge in any cosmological view of the universe is then tantamount to inherent observational limits imposed by acts of observation and theory itself. For example, in the big bang cosmology the universe becomes opaque to radiation early on, and the images of extended distant galaxies merge for redshifts, z, of the order of a few. Moreover, in order to measure the distance of a remote galaxy to test any cosmological theory, one has to disperse its light to form a spectrum which would cause confusion with other background galaxies. Since the early universe should be described in quantum terms, it follows that the same problems regarding quantum reality and the role of the observer apply to the universe as a whole. One of the most fundamental properties of quantum theory, non-locality, may then apply equally well to the universe. Some of the problems facing big bang cosmology, like the horizon and flatness problems, may not then be preconditions on theoretical models but may instead be the manifestations of the quantum nature of the universe.
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Kafatos, Menas. "Knowledge Limits in Cosmology." Symposium - International Astronomical Union 168 (1996): 431–38. http://dx.doi.org/10.1017/s0074180900110307.

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In cosmology one faces the observational challenge that knowledge about distant regions of the universe is dependent on assumptions one makes about these regions which are themselves coupled to the observations. Within the framework of the Friedmann-Robertson-Walker big bang models the universe becomes opaque to its own radiation at z ≈ 1,000 and the earlier, and more distant, regions of the universe are not directly accessible through observations. Other challenges exist such as possible merging of extended distant sources and confusion of spectra from distant galaxies. One, therefore, encounters horizons in our understanding of the universe. Such horizons exist in any mode of description. To use the quantum analogy, the observer is always part of the system under study, the universe, and a description of the universe entails including the observer and observing apparatus. Since the early universe should be described in quantum terms, it follows that non-locality in the universe is not an a-priori requirement but the outcome of the observing process itself. As such, the flatness and horizon problems may not be preconditions on theoretical models.
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Al-Fadhli, Mohammed B. "On Spacetime Duality and Bounce Cosmology of a Dual Universe." Physical Sciences Forum 2, no. 1 (February 22, 2021): 61. http://dx.doi.org/10.3390/ecu2021-09291.

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The recent Planck Legacy 2018 release confirmed the existence of an enhanced lensing amplitude in the cosmic microwave background (CMB) power spectra. Notably, this amplitude is higher than that estimated by the lambda cold dark matter model, which prefers a positively curved early Universe with a confidence level greater than 99%. In this study, the pre-existing curvature is incorporated to extend the field equations where the space-time worldlines are utilised to model the evolution of the Universe with reference to the scale factor of the early Universe and its radius of curvature upon the emission of the CMB. The worldlines reveal both positive and negative solutions, implying that matter and antimatter of early Universe plasma evolved in opposite directions as distinct Universe sides during a first decelerating phase. The worldlines then indicate a second accelerated phase in reverse directions, whereby both sides free-fall towards each other under gravitational acceleration. The simulation of the predicted conformal curvature evolution demonstrates the fast orbital speed of the outer stars owing to external fields exerted on galaxies as they travel through conformally curved space-time. Finally, the worldlines predict an eventual time-reversal phase comprising rapid spatial contraction that culminates in a Big Crunch, signalling a cyclic Universe. These findings reveal that the early Universe’s plasma could be separated and evolved into distinct sides of the Universe that collectively and geometrically inducing its evolution, physically explaining the effects attributed to dark energy and dark matter.
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Дисертації з теми "Cosmology of the early Universe"

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Murray, Brian M. "Early and late universe cosmology /." view abstract or download file of text, 2006. http://proquest.umi.com/pqdweb?did=1276405191&sid=1&Fmt=2&clientId=11238&RQT=309&VName=PQD.

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Thesis (Ph. D.)--University of Oregon, 2006.
Typescript. Includes vita and abstract. Includes bibliographical references (leaves 75-80). Also available for download via the World Wide Web; free to University of Oregon users.
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2

Karouby, Johanna. "Topics in early universe cosmology." Thesis, McGill University, 2012. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=110537.

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The study of the Early Universe raises some of the most fundamental questions in theoretical physics. This thesis explores three main aspects of early universe cosmology. The first part discusses alternatives to the Big Bang scenario which is the current paradigm of cosmology. Namely, it discusses bouncing universe models where the initial Big Bang singularity is replaced by a finite size universe. After reviewing the necessary cosmology background in the introduction, we show a specific model of a bouncing universe that contains additional "Lee-Wick fields", partners to the standard fields. In particular we prove that a Lee-Wick matter bounce is unstable when one adds radiation to matter. In the second part of this thesis, we consider particle production via parametric resonance during preheating, at the end of cosmological inflation. Specifically, we prove that in the case of a speed-limited inflaton, non-canonical kinetic terms used to described any effective Lagrangian do not enhance particle production. Finally, the last topic involves topological defects during the Quantum Chromodynamics phase transition. Namely, we study cosmic strings coming from pionfields present in the Standard Model of particle physics and find a mechanism to stabilize them. We show how a thermal bath of photons reduces the effective vacuum manifold to a circle and thus allows the presence of topologically stable pionstrings.
L'etude de l'Univers primordial adresse quelques-unes des questions les plus fondamentales de la physique theorique. Cette these a pour objet l'exploration de trois aspects principaux de la cosmologie primordiale. Dans un premier temps, nous discutons d'une alternative au paradigme scientique qu'est le modele du Big Bang. A savoir, nous explorons un model d'univers a rebond qui evite la singularite initiale du Big Bang. Nous commencerons dans l'introduction par revoir les elements de base necessaires a la comprehension de la cosmologie. A la suite de quoi, nous montrerons un modele specifique d'Univers a rebond contenant des champs additionnels particuliers en complements des champs présents habituellement. Ces nouveaux champs proviennent de ce qui s'appelle le modele "Lee-Wick" de la physique des particules. En particulier, nous prouvons qu'un univers a rebond dans ce contexte est instable lorsque l'on ajoute une composante de radiation en plus de la matiere. Dans la seconde partie, nous considérons la production de particules via un phenomene de resonance parametrique durant la phase de "prechauffement", a la fin de l'inflation cosmologique. Plus précisément, nous prouvons que dans le cas ou l'inflaton a une limite de vitesse, les termes cinetiques non-canoniques d'écrivant n'importe quel Lagrangien effectif n'améliorent pas la production de particules. Finalement, le dernier sujet abordé concerne les défauts topologiques pendant la transition de phase de la chromodynamique quantique. A savoir, nous etudions les cordes cosmiques provenant des champs de pions presents dans le modele standard de la physique des particules et trouvons un méchanisme pour les stabiliser. Nous prouvons alors qu'un bain thermique de photons en contact avec ces cordes reduit la variete du vide a un cercle. Cela a pour effet d'autoriser la presence de "cordes pioniques" topologiquement stables.
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3

Fonseca, José. "Primordial perturbations from early universe cosmology." Thesis, University of Portsmouth, 2012. https://researchportal.port.ac.uk/portal/en/theses/primordial-perturbations-from-early-universe-cosmology(55ef947f-d828-44df-a168-c3b2895b4955).html.

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The very early universe is where we expect the observed primordial perturbations in the cosmic microwave background to have originated. In this thesis we study isocurvature field fluctuations during inflation and ekpyrotic contraction as sources of the primordial curvature perturbations. We start by introducing concepts of modern cosmology followed by an overview of early universe cosmology. After, we introduce perturbation theory and how to compute perturbations from early universe models. After reviewing all fundamental concepts necessary for this thesis, we estimate largescale curvature perturbations from isocurvature fluctuations in the waterfall field during hybrid inflation, in addition to the usual inflaton field perturbations. The tachyonic instability at the end of this inflation model leads to an explosive growth of super-Hubble scale perturbations, but they retain the steep blue spectrum characteristic of vacuum fluctuations in a massive field during inflation. We extend the usual δN formalism to include the essential role of small fluctuations when estimating the large-scale curvature perturbation. The following two chapters study perturbations within the curvaton proposal. Firstly, we consider how non-Gaussianity of the primordial density perturbation and the amplitude of gravitational waves from inflation can be used to determine parameters of the curvaton scenario for the origin of structure. We show that in the simplest quadratic model, where the curvaton evolves as a free scalar field, measurement of the bispectrum relative to the power spectrum, fNL, and the tensor-to-scalar ratio can determine both the expectation value of the curvaton field during inflation and its dimensionless decay rate relative to the curvaton mass. We show how these predictions are altered by the introduction of self-interactions. In the following chapter, we then characterise the primordial perturbations produced due to both inflaton and curvaton fluctuations. We show how observational bounds on non-linearity parameters and the tensor-scalar ratio can be used to constrain curvaton and inflaton parameters. The final research presented in this thesis, considers a simple model of cosmological collapse driven by canonical fields with exponential potentials. We generalise the two-field ekpyrotic collapse to consider non-orthogonal potentials and give the general condition for isocurvature field fluctuations to have a slightly red spectrum of perturbations as required by current observations. However a red spectrum of fluctuations implies that the two-field ekpyrotic phase must have a finite duration and requires a preceding phase which sets the initial conditions for what otherwise appears to be a fine-tuned trajectory in the phase space. We end this thesis with some concluding remarks and comments on possible future work.
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Feeney, S. M. "Novel algorithms for early-universe cosmology." Thesis, University College London (University of London), 2012. http://discovery.ucl.ac.uk/1380711/.

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Fluctuations in the cosmic microwave background (CMB), the radiation left over from the Big Bang, contain information which has been pivotal in establishing the current cosmological model. CMB data can also be used to test theoretically well-motivated additions to the model, including pre-inflationary relics (signatures of bubble collisions arising in eternal inflation) and topological defects that form after inflation (cosmic strings and textures). These relics typically leave sub-dominant, spatially localised signals, hidden in the “noise” of the primary CMB, the instrumental noise, foreground residuals and other systematics. Standard approaches for searching for such signals involve focusing on statistical anomalies, which carry the danger of extreme a posteriori biases. The self-consistent approach to this problem is Bayesian model comparison; however, the full implementation of this approach is computationally intractable with current CMB datasets, and will only become more difficult with data from the next generation of CMB experiments. I will describe a powerful modular algorithm, capable of coping with the volume of data, which combines a candidate-detection stage (using wavelets or optimal filters) with a full Bayesian parameter-estimation and model-selection stage performed in pixel space within the candidate regions. The algorithm is designed to fully account for the “look-elsewhere” effect, and its use of blind analysis techniques further enhances its robustness to unknown systematics. Finally, I will present the results of applying the algorithm to hunt for the signatures of bubble collisions and cosmic textures in the seven-year data from the Wilkinson Microwave Anisotropy Probe.
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5

Emond, William. "Dynamics of early & late universe cosmology." Thesis, University of Nottingham, 2018. http://eprints.nottingham.ac.uk/55493/.

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In this thesis we discuss two key problems: the cosmological constant problem (CCP), an issue that primarily manifests itself in late universe cosmology; and the process of thermalisation during the post-inflationary reheating phase of the early universe. We start by giving a brief review of general relativity, discussing both its successes and failures, in particular, why one might consider modifications of it. We then delve into the aspects of early and late universe cosmology that we aim to address in the research discussed in this thesis. Starting with an overview of the inflationary paradigm, and the need to reheat the universe post-inflation, we give a review of previous research that has been conducted in this area. We then move on to discuss the CCP in detail, in particular, why it is such an issue. After setting the scene for this problem, we proceed to discuss how to approach finding a resolution to it, highlighting certain stumbling blocks that one needs to be mindful of. Having set the scene, we then present a potential solution to the CCP, involving a scalar-tensor modifed theory of gravity, so-called Horndeski theory. Building upon a class of Horndeski theories providing self-tuning solutions to the CCP, we provide a generalisation in which matter interacts with gravity via a disformal coupling to the spacetime metric. We establish the form of the disformally self-tuning Lagrangian on a cosmological Friedmann-Robertson-Walker background, and show that there exist non-trivial self-tuning solutions. In the latter half of this thesis, we move on to review the literature on the non-perturbative description of the early stages of reheating, so-called preheating. With the motivation to study the less well understood thermalisation process that must necessarily take place in this phase, we then present a toy model preheating theory, in which we account for the effects of thermalisation from its onset. Within the density matrix formalism, we derive a (self-consistent) set of quantum Boltzmann equations, which are able to describe the evolution of an ensemble of self-interacting scalar particles that are subject to an oscillating mass term. In particular, we apply this to the preheating scenario in order to study the evolution of scalar particle number densities throughout this process. We then conclude by discussing our numerical analysis of the Boltzmann equations, drawing attention to some important results and features that manifest using this approach, in particular, how the process differs from the standard analysis through the inclusion of thermalisation.
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Chadburn, Sarah Elizabeth. "Signals of early-universe physics in cosmology." Thesis, Durham University, 2013. http://etheses.dur.ac.uk/7008/.

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This is a thesis on theoretical cosmology. The first and largest part is a study of cosmic strings, in particular their dynamics and signals in higher dimensional spacetimes. The second part is a study of black holes in a quintessence background. Cosmic strings are predicted by models of the early universe. They were thought to arise, originally, from Grand Unified Theories, and more recently from brane inflationary models based in string theory. In Chapter 3 we find exact solutions for cosmic string loop trajectories in higher dimensions, and find the regions of parameter space for which cusps exist. We find that winding the internal dimensions slows the average velocity of string loops, and conjecture that the periodicity of internal space may contribute to self-intersections. In Chapter 4, we calculate the gravitational wave signal from cosmic string cusps in higher dimensions, and find it is much reduced relative to the 4D case. The main reason for this is the large reduction in the probability of cusps occurring on loops in higher dimensions, as well as a slight reduction in signal from individual cusps. In Chapter 5, we study cosmic string trajectories in warped spacetimes, such as may be found in realistic brane inflation models. We find that contrary to claims in the literature, the warping of the internal space does not prevent the internal motion of strings. The energy associated with the warping of spacetime means that the energy of a loop appears to change over time from our 4D perspective. Finally, in Chapter 6, we find an analytic, general-relativistic solution describing a black hole in a quintessence universe. Quintessence is a model of late-time cosmic acceleration in which expansion is sourced by a scalar field. Our solution shows the interaction between this scalar field and a black hole. The scalar field is shown to continue its cosmological "rolling" behaviour everywhere, including on the black hole event horizon, and the black hole is shown slowly to accrete scalar field. This is a perturbative solution valid throughout all of space but only over a finite period of time.
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7

Zarikas, Vasilios. "Aspects of early universe phase transitions." Thesis, University of Newcastle Upon Tyne, 1996. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.318257.

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8

Shellard, E. P. S. "Quantum effects in the early universe." Thesis, University of Cambridge, 1986. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.233337.

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The subject of this dissertation lies in the region where modern particle physics and cosmology intersect. Broadly speaking, its context is provided by the shortcomings of the 'standard cosmology', and the more recent inflationary scenario. The particular aspects which are tackled - the origin of density fluctuations and the boundary conditions of the universe - are outlined below. A. The Cosmic String Scenario: Phase transitions in the early universe may have produced topological 'knots' or defects, such as monopoles cosmic strings and domain walls. Cosmic strings, in particular, have attracted much interest recently because of the alluring model of galaxy formation they have the potential to produce. The viability of this new scenario, however, rests on untested assumptions about string interaction properties - whether or not they intercommute. A detailed study of global U(1)-strings has demonstrated that under most circumstances they will intercommute, a result expected for other varieties of strings (Part A). Given this firmer foundation for the cosmic string scenario, some of their astrophysical implications are explored. In particular, the large scale peculiar velocities predicted in this model are examined. B. The domain wall problem of the Axion: The axion has attracted considerable interest as a cold dark matter candidate. In part B, we concentrate on what potentially is a cosmological flaw of the axion: The non-trivial vacuum topology of axion models gives rise to cosmic vortex strings and domain walls. The latter are catastrophic unless removed by some mechanism soon after formation. In the dissertation we demonstrate the efficacy of their removal through string/domain wall intercommuting and annihilation. Causality constraints purporting to restrict the rate of this mechanism are found to be circumvented. C. Quantum Cosmology and Recollapse: Regardless of whether all the physical laws of system are known, its boundary conditions must still be given. In a quantum cosmological context, Hartle and Hawking have proposed that these be specified by a path-integral over compact four geometries. In Part C detailed studies of the implications of this proposal are made for two restricted models, the Freidmann-Robertson-Walker universe with a massive scalar field and the anisotropic Kantowski-Sachs cosmology. We evaluate the respective wavefunctions and the trajectories to which they correspond in the classical limit. Attention is focussed on the fact that most classical trajectories will recollapse to a singularity - the difficulty that this presents for the H-H proposal is discussed. The Kantowski-Sachs universes generically evolve from isotropy during expansion to increasing anisotropy during recollapse, ending as a black hole interior. Some comment is made on the arrow of time thereby induced by the Hartle-Hawking proposal.
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9

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

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10

Ijjas, Anna. "Observational and theoretical issues in early universe cosmology." Doctoral thesis, Humboldt-Universität zu Berlin, Mathematisch-Naturwissenschaftliche Fakultät I, 2014. http://dx.doi.org/10.18452/16965.

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Wir bewerten und vergleichen konkurrierende kosmologische Modelle im Hinblick auf theoretische Konsistenz und empirische Kohärenz. Ferner finden wir neue Wege, aktuelle kosmologische Paradigmen des frühen Universums weiter zu entwickeln. Im ersten Teil der Arbeit zeigen wir, dass die empirischen Daten der Planck2013-Satellitenmission für eine spezielle Klasse inflationärer Modelle sprechen, nämlich sog. “plateauartige Modelle mit schmalem Feldbereich”; gleichsam werden die einfachsten inflationären Modelle von den Messdaten nicht gestärkt. Wir formulieren eine neuartige konzeptionelle Schwierigkeit für Plateau-Modelle. Diese besteht darin, dass in einer Energielandschaft, die sowohl plateauartige als auch einfachere Formen der inflationären Potenziale enthält, die plateauartigen weniger Inflation produzieren und es deshalb weniger wahrscheinlich ist, dass sie das observable Universum beschreiben. Wir zeigen ferner, dass dieselben Plateau-Modelle mit einem neuen Multiversumsproblem und einem neuen Anfangswertsproblem behaftet sind. Im zweiten Teil untersuchen wir die Implikationen einer einfachen und experimentell motivierten Zusatzbedingung, Skalenfreiheit. Wir zeigen, dass die uneingeschränkte Palette inflationärer Potenziale sich auf ein wohldefiniertes Bündel inflationärer Modelle reduziert. Dabei verwenden wir eine allgemeine hydrodynamische Beschreibung. Wir klassifizieren und bewerten diese skalenfreien inflationären Modelle im Licht von Planck2013. Anschließend wiederholen wir die Analyse, um ähnliche skalenfreie zyklische Modelle des Universums zu konstruieren. Diese Modelle vergleichen wir mit unseren Ergebnissen, die wir für die skalenfreie inflationäre Theorie gewonnen haben. Im dritten Teil der Arbeit führen wir eine neue Klasse stabiler zyklischer Modelle ein. Wir zeigen, dass diese Modelle weniger Feinabstimmung der Anfangswerte benötigen. Gleichsam generieren sie vernachlässigbare Nicht-Gaussianität in Übereinstimmung mit den Planck2013-Messdaten.
In this thesis we evaluate and compare competing cosmological models for empirical and theoretical consistency and identify new ways of improving current paradigms of early universe cosmology. In the first part, we show that the most recent experimental data from the Planck2013 satellite measuring fluctuations in the cosmic microwave background favors a special class of “small-field plateau-like” models of inflation and disfavors the simplest inflationary potentials. We then identify a new kind of conceptual difficulty for the plateau models that we call the unlikeliness problem – namely, in an energy landscape that includes both plateau-like and simpler potential shapes, the plateau-like produces less inflation and, hence, is less likely to explain our observable universe. In addition, we show that the very same plateau-like models suffer from a new multiverse problem and a new initial conditions problem because they require that inflation starts at energy densities well below the Planck scale. Third, we comment on the impact of these results on the standard view of inflation and more recent versions of the theory invoking the multiverse and complex energy landscapes. In the second part of this thesis, imposing a single, simple, well-motivated constraint – scale-freeness – and using a general hydrodynamic analysis, we show that the unrestricted range of inflationary potentials reduces to a well-defined bundle of inflationary models. We classify and evaluate the scale-free inflationary models in light of Planck2013. We then repeat the construction to produce analogous scale-free bouncing cyclic models of the universe and compare with the inflationary results. In the third part, we introduce a new class of stable ekpyrotic/cyclic models that require less fine-tuning and generate negligible non-Gaussianity consistent with Planck2013 data.
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Книги з теми "Cosmology of the early Universe"

1

Gibbons, G. W. Very early universe. Cambridge: CUP, 1985.

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2

Bari, Pasquale Di. Cosmology and the Early Universe. Boca Raton : CRC Press, [2018] | Series: Series in astronomy and astrophysics: CRC Press, 2018. http://dx.doi.org/10.1201/9781138496903.

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3

1936-, Johri V. B., ed. The early universe. Palm Harbor, FL, USA: Hadronic Press, 1996.

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4

G, Unruh W., Semenoff G. W, and North Atlantic Treaty Organization. Scientific Affairs Division., eds. The early universe. Dordrecht: D. Reidel, 1988.

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5

Stanley, Turner Michael, ed. The early universe. Reading, Mass: Addison-Wesley, 1994.

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6

Stanley, Turner Michael, ed. The early universe. Reading, Mass: Addison-Wesley, 1990.

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7

Stanley, Turner Michael, ed. The Moslem World. Redwood City, Calif: Addison-Wesley, 1990.

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8

Bretón, Nora, Jorge Luis Cervantes-Cota, and Marcelo Salgado, eds. The Early Universe and Observational Cosmology. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/b97189.

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9

Mexican School on Gravitation and Mathematical Physics (5th 2002 Playa del Carmen, Mexico). The early universe and observational cosmology. Berlin: Springer, 2004.

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10

W, Kolb Edward, Turner Michael Stanley, and Kolb Edward W, eds. The Early universe-reprints. Redwood City, Calif: Addison-Wesley Pub. Co., Advanced Book Program, 1988.

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Більше джерел

Частини книг з теми "Cosmology of the early Universe"

1

Barrow, John D. "Relativistic Cosmology." In The Early Universe, 125–201. Dordrecht: Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-4015-4_4.

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2

Keeton, Charles. "Cosmology: Early Universe." In Undergraduate Lecture Notes in Physics, 395–410. New York, NY: Springer New York, 2014. http://dx.doi.org/10.1007/978-1-4614-9236-8_20.

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3

Schmitz, Kai. "Early Universe Cosmology." In The B−L Phase Transition, 11–37. Cham: Springer International Publishing, 2013. http://dx.doi.org/10.1007/978-3-319-00963-6_2.

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4

Turner, Michael S. "Cosmology and Particle Physics." In The Early Universe, 19–113. Dordrecht: Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-4015-4_2.

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5

Piran, Tsvi. "Numerical Relativity and Cosmology." In The Early Universe, 261–82. Dordrecht: Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-4015-4_8.

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6

Povh, Bogdan, and Mitja Rosina. "Cosmology – The Early Universe." In Scattering and Structures, 207–18. Berlin, Heidelberg: Springer Berlin Heidelberg, 2017. http://dx.doi.org/10.1007/978-3-662-54515-7_17.

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7

Faraoni, Valerio. "The Early Universe." In Cosmology in Scalar-Tensor Gravity, 115–25. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-1989-0_5.

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8

Perlov, Delia, and Alex Vilenkin. "The Very Early Universe." In Cosmology for the Curious, 201–24. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-57040-2_14.

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9

Abraham, Eitan, and Andrés J. Kreiner. "Cosmology concepts." In Elementary Particles and the Early Universe, 7–13. Boca Raton: CRC Press, 2022. http://dx.doi.org/10.1201/9781003099581-3.

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10

Bari, Pasquale Di. "A Newtonian cosmology?" In Cosmology and the Early Universe, 27–36. Boca Raton : CRC Press, [2018] | Series: Series in astronomy and astrophysics: CRC Press, 2018. http://dx.doi.org/10.1201/9781138496903-3.

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Тези доповідей конференцій з теми "Cosmology of the early Universe"

1

Brandenberger, Robert Hans. "Introduction to Early Universe Cosmology." In 4th International Conference on Fundamental Interactions. Trieste, Italy: Sissa Medialab, 2011. http://dx.doi.org/10.22323/1.124.0001.

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2

Brandenberger, Robert H., Renato Dupke, Jailson Alcaniz, Ramiro de la Reza, and Simone Daflon. "Cosmology of the Very Early Universe." In GRADUATE SCHOOL IN ASTRONOMY: XIV Special Courses at the National Observatory of Rio de Janeiro. AIP, 2010. http://dx.doi.org/10.1063/1.3483879.

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3

Bromm, Volker, Abraham Loeb, Stefan Immler, and Kurt Weiler. "GRB Cosmology: Probing the Early Universe." In SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters. AIP, 2007. http://dx.doi.org/10.1063/1.2803621.

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4

Kaufman, Alexander, Daniel Sundy, and Michael McGuigan. "Quantum computation for early universe cosmology." In 2019 New York Scientific Data Summit (NYSDS). IEEE, 2019. http://dx.doi.org/10.1109/nysds.2019.8909801.

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5

Bromm, Volker, Abraham Loeb, Stefan Immler, and Kurt Weiler. "GRB Cosmology: Probing the Early Universe." In SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters. AIP, 2007. http://dx.doi.org/10.1063/1.3682957.

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6

Ciarcelluti, P., Jean-Michel Alimi, and André Fuözfa. "Early Universe cosmology with mirror dark matter." In INVISIBLE UNIVERSE: Proceedings of the Conference. AIP, 2010. http://dx.doi.org/10.1063/1.3462655.

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7

Cai, Yi-Fu, and Teruaki Suyama. "Summary of Parallel Session: “Cosmology — Early Universe”." In Second LeCosPA International Symposium: Everything about Gravity. WORLD SCIENTIFIC, 2017. http://dx.doi.org/10.1142/9789813203952_0058.

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8

SASAKI, MISAO. "B.2(I): COSMOLOGY (I). EARLY UNIVERSE." In Proceedings of the 17th International Conference. WORLD SCIENTIFIC, 2005. http://dx.doi.org/10.1142/9789812701688_0024.

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9

HAWKING, S. W. "LARGE N COSMOLOGY." In Proceedings of the Fourth International Workshop on Particle Physics and the Early Universe. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812799678_0009.

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10

Doré, Olivier. "First Year WMAP Results and Early Universe Cosmology." In PARTICLES, STRINGS, AND COSMOLOGY: 11th International Symposium on Particles, Strings, and Cosmology; PASCOS 2005. AIP, 2005. http://dx.doi.org/10.1063/1.2149666.

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Звіти організацій з теми "Cosmology of the early Universe"

1

Zurek, W. H., B. Bromley, and T. Brainerd. Experimental cosmology: The early universe after COBE. Office of Scientific and Technical Information (OSTI), December 1998. http://dx.doi.org/10.2172/560870.

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2

Giorgi, Elena Edi. Using Supercomputers to Probe the Early Universe. Office of Scientific and Technical Information (OSTI), May 2016. http://dx.doi.org/10.2172/1254250.

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3

Parisi, Luca. Dynamical Systems Techniques in Cosmology. An example: LQC and the Einstein Static Universe. GIQ, 2012. http://dx.doi.org/10.7546/giq-10-2009-211-226.

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4

Parisi, Luca. Dynamical Systems Techniques in Cosmology. An example: LQC and the Einstein Static Universe. Journal of Geometry and Symmetry in Physics, 2012. http://dx.doi.org/10.7546/jgsp-14-2009-67-83.

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5

Green, Daniel. Final Technical Report: Light Relics of the Early Universe. Office of Scientific and Technical Information (OSTI), January 2022. http://dx.doi.org/10.2172/1840603.

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6

Arkani-Hamed, Nima. Early Inflation and Cosmology in Theories with Sub-Millimeter Dimensions. Office of Scientific and Technical Information (OSTI), March 1999. http://dx.doi.org/10.2172/10022.

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7

Khoury, Justin. New Ideas for the Dark Sector and the Early Universe. Office of Scientific and Technical Information (OSTI), July 2018. http://dx.doi.org/10.2172/1458978.

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8

Turner, M. S. Thermal production of not so invisible axions in the early universe. Office of Scientific and Technical Information (OSTI), October 1986. http://dx.doi.org/10.2172/6926041.

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9

Mathews, G. Hydrodynamics and nucleosynthesis in neutron stars, supernovae, and the early universe. Office of Scientific and Technical Information (OSTI), March 1996. http://dx.doi.org/10.2172/278392.

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10

Arkani-Hamed, Nima. Rapid asymmetric inflation and early cosmology in theories with sub-millimeter dimensions. Office of Scientific and Technical Information (OSTI), March 1999. http://dx.doi.org/10.2172/10013.

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