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Relevant bibliographies by topics / Inflationary Models

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Academic literature on the topic 'Inflationary Models'

Author: Grafiati

Published: 4 June 2021

Last updated: 18 May 2024

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Journal articles on the topic "Inflationary Models"

1

Ellis, G. F. R., D. H. Lyth, and M. B. Mijić. "Inflationary models with." Physics Letters B 271, no. 1-2 (1991): 52–60. http://dx.doi.org/10.1016/0370-2693(91)91277-3.

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Yuanjie, Li, and Wang Zhijun. "InhomogeneousR 2 inflationary models." International Journal of Theoretical Physics 31, no. 12 (1992): 2053–59. http://dx.doi.org/10.1007/bf00679964.

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olyaei, Abbas. "Phenomenology of inflationary models." Modern Physics Letters A 33, no. 03 (2018): 1850018. http://dx.doi.org/10.1142/s0217732318500189.

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There are many inflationary models compatible with observational data. One can investigate inflationary models by looking at their general features, which are common in most of the models. Here we have investigated some of the single-field models without considering their origin in order to find the phenomenology of them. We have shown how to adjust the simple harmonic oscillator model in order to be in good agreement with observational data.

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Gr�n, �. "Viscous inflationary universe models." Astrophysics and Space Science 173, no. 2 (1990): 191–225. http://dx.doi.org/10.1007/bf00643930.

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Fernández-Jambrina, Leonardo. "Singularities in Inflationary Cosmological Models." Universe 7, no. 12 (2021): 491. http://dx.doi.org/10.3390/universe7120491.

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Due to the accelerated expansion of the universe, the possibilities for the formation of singularities has changed from the classical Big Bang and Big Crunch singularities to include a number of new scenarios. In recent papers it has been shown that such singularities may appear in inflationary cosmological models with a fractional power scalar field potential. In this paper we enlarge the analysis of singularities in scalar field cosmological models by the use of generalised power expansions of their Hubble scalars and their scalar fields in order to describe all possible models leading to a

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Herrera, Ramón, Sergio del Campo, and Cuauhtemoc Campuzano. "Tachyon warm inflationary universe models." Journal of Cosmology and Astroparticle Physics 2006, no. 10 (2006): 009. http://dx.doi.org/10.1088/1475-7516/2006/10/009.

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Mignemi, S., and H. J. Schmidt. "Classification of multidimensional inflationary models." Journal of Mathematical Physics 39, no. 2 (1998): 998–1010. http://dx.doi.org/10.1063/1.532366.

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Barrow, John D., and Paul Parsons. "Inflationary models with logarithmic potentials." Physical Review D 52, no. 10 (1995): 5576–87. http://dx.doi.org/10.1103/physrevd.52.5576.

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Demianski, M., R. De Ritis, G. Platania, P. Scudellaro, and C. Stornaiolo. "Inflationary models in ECSK theory." Physics Letters A 116, no. 1 (1986): 13–16. http://dx.doi.org/10.1016/0375-9601(86)90347-6.

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Bessada, Dennis, William H. Kinney, and Konstantinos Tzirakis. "Inflationary potentials in DBI models." Journal of Cosmology and Astroparticle Physics 2009, no. 09 (2009): 031. http://dx.doi.org/10.1088/1475-7516/2009/09/031.

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Dissertations / Theses on the topic "Inflationary Models"

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PINTUS, NICOLA. "On Inflationary cosmological models." Doctoral thesis, Università degli Studi di Cagliari, 2016. http://hdl.handle.net/11584/266648.

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The most common mechanisms leading to in ation are based on models of gravity minimally coupled to a scalar field rolling on a suitable potential V. We discuss such a model defined by the action I = ∫√-g p [R -2 (ϕ)2 )] d4x, in order to find exact general isotropic and homogeneous cosmological solutions displaying an in ationary behavior at early times and a power-law expansion at late times. We also study the effect of the inclusion of matter (in the form of a perfect uid): in this case, we do not find exact solutions because of the non-integrability of the field equations, but we

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Senoguz, Vedat Nefer. "Aspects of inflationary models and unification." Access to citation, abstract and download form provided by ProQuest Information and Learning Company; downloadable PDF file, 114 p, 2007. http://proquest.umi.com/pqdweb?did=1251906411&sid=1&Fmt=2&clientId=8331&RQT=309&VName=PQD.

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Paul, Bikash Chandra. "The Inflationary models of the early universe." Thesis, University of North Bengal, 1990. http://hdl.handle.net/123456789/619.

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De, Martino Danilo. "String inflationary models with non-monotonic slow-roll and detectable tensor modes." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2015. http://amslaurea.unibo.it/8391/.

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The first chapter of this work has the aim to provide a brief overview of the history of our Universe, in the context of string theory and considering inflation as its possible application to cosmological problems. We then discuss type IIB string compactifications, introducing the study of the inflaton, a scalar field candidated to describe the inflation theory. The Large Volume Scenario (LVS) is studied in the second chapter paying particular attention to the stabilisation of the Kähler moduli which are four-dimensional gravitationally coupled scalar fields which parameterise the size of the

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Pieroni, Mauro. "Classification of inflationary models and constraints on fundamental physics." Thesis, Sorbonne Paris Cité, 2016. http://www.theses.fr/2016USPCC258/document.

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Ce travail est concentré sur l'étude de la cosmologie primordiale et en particulier sur l'étude de l'inflation. Après une introduction sur la théorie standard du Big Bang, nous discutons de la physique du CMB et nous expliquons comment ses observations peuvent être utilisées pour définir des contraintes sur les modèles cosmologiques. Nous introduisons l'inflation et nous expliquons sa réalisation la plus simple. Nous présentons les observables et les contraintes expérimentales qui peuvent être utilisées pour mettre des contraintes sur les modèles d'inflation. La possibilité d'observer des onde

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Dimastrogiovanni, Emanuela. "Cosmological correlation functions in scalar and vector inflationary models." Doctoral thesis, Università degli studi di Padova, 2010. http://hdl.handle.net/11577/3427056.

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This thesis is centered on three main subjects within the theory of inflation and cosmological perturbations: loop corrections to the power spectrum of curvature fluctuations generated during inflation; evolution of cosmological fluctuations in anisotropic pre-inflationary cosmologies; statistical anisotropy and non-Gaussianity predictions of models of inflation populated with vector fields. Currently, what makes even more interesting the study of 2-nd and higher order corrections to cosmological correlation functions as well as the computation of higher-than-two order correlators, is the almo

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Barone, Alessandro. "The cosmological moduli problem in multi-field string inflationary models." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2019. http://amslaurea.unibo.it/18080/.

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The 4D low-energy limit of string compactifications is characterised by the ubiquitous presence of string moduli which are new gravitationally coupled scalar fields which develop mass via supersymmetry breaking effects. During inflation it is generically expected that these fields receive large contributions to their mass of order the Hubble constant. They are therefore shifted from their minimum and after the end of inflation start oscillating around it behaving as non-relativistic matter. Given that matter redshifts slower than radiation, the moduli quickly come to dominate the energy densit

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Huston, Ian. "Constraining inflationary scenarios with braneworld models and second order cosmological perturbations." Thesis, Queen Mary, University of London, 2010. http://qmro.qmul.ac.uk/xmlui/handle/123456789/584.

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Inflationary cosmology is the leading explanation of the very early universe. Many diff erent models of inflation have been constructed which fit current observational data. In this work theoretical and numerical methods for constraining the parameter space of a wide class of such models are described. First, string-theoretic models with large non-Gaussian signatures are investigated. An upper bound is placed on the amplitude of primordial gravitational waves produced by ultra-violet Dirac-Born-Infeld inflation. In all but the most finely tuned cases, this bound is incompatible with a lower bo

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Barnaby, Neil. "Cosmological instabilities." Thesis, McGill University, 2007. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=103365.

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Though historically the word "tachyon" has been used to describe hypothetical particles which propagate faster than the speed of light, in a more modern context the term has been recycled to refer to certain unstable states in field theory. This thesis explores the role of tachyonic instabilities in cosmology considering tachyons which arise in string theory and also more conventional, field theoretic instabilities. Our study of such instabilities is, in part, motivated by attempts to embed inflation into string theory. We will argue that the study of string theory models of inflation is well-

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Robinson, Kenneth James. "Random-coefficients models of the inflationary consequences of discretionary central-bank behavior." Connect to resource, 1986. http://rave.ohiolink.edu/etdc/view.cgi?acc%5Fnum=osu1262786327.

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Books on the topic "Inflationary Models"

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Villarreal, Cuauhtémoc Calderón, and Thomas M. Fullerton. Inflationary studies for Latin America. Universidad Autónoma de Ciudad Juárez, 2000.

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Fair, Ray C. Inflationary expectations and price setting behavior. National Bureau of Economic Research, 1989.

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Ndung'u, Njuguna. Dynamics of the inflationary process in Kenya. Göteborgs universitet], 1993.

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Hoeller, Peter. P-star as an indicator of inflationary pressure. Organisation forEconomic Co-opertion and Development, 1991.

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Pierre, Poret, ed. P star as an indicator of inflationary pressure. Organisation for Economic Co-operationa dn Development, 1991.

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Johansen, Søren. Controlling inflation in a cointegrated vector autoregressive model with an application to US data. European University Institute, Department of Economics, 2001.

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Gerali, Andrea. On the "conquest" of inflation. Banca d'Italia, 2002.

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Stanley, Turner Michael, Fermi National Accelerator Laboratory, and United States. National Aeronautics and Space Administration., eds. Second-order reconstruction of the inflationary potential. Fermi National Accelerator Laboratory, 1994.

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Stanley, Turner Michael, Fermi National Accelerator Laboratory, and United States. National Aeronautics and Space Administration., eds. Second-order reconstruction of the inflationary potential. Fermi National Accelerator Laboratory, 1994.

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Stanley, Turner Michael, Fermi National Accelerator Laboratory, and United States. National Aeronautics and Space Administration., eds. Second-order reconstruction of the inflationary potential. Fermi National Accelerator Laboratory, 1994.

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Book chapters on the topic "Inflationary Models"

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del Campo, Sergio. "Exact Approach to Inflationary Universe Models." In Springer Handbook of Spacetime. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-41992-8_31.

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Brandenberger, Robert H. "Inflationary Universe Models and the Formation of Structure." In Nearly Normal Galaxies. Springer New York, 1987. http://dx.doi.org/10.1007/978-1-4612-4762-3_41.

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Arya, Richa, and Raghavan Rangarajan. "Estimation of the Parameters of Warm Inflationary Models." In Springer Proceedings in Physics. Springer Singapore, 2021. http://dx.doi.org/10.1007/978-981-33-4408-2_46.

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Sivaram, C. "Inflationary Universe Models and Clustering Of Quasar Red Shifts." In Quasars. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4716-0_118.

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Klein, Lawrence R. "Did Mainstream Econometric Models Fail to Anticipate the Inflationary Surge?" In Issues in Contemporary Macroeconomics and Distribution. Palgrave Macmillan UK, 1985. http://dx.doi.org/10.1007/978-1-349-06879-1_12.

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Năstase, Horaţiu. "Problems to Be Solved by Inflation and How They Are Solved in Inflationary Models." In Fundamental Theories of Physics. Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-15077-8_8.

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Prescott, Anne Lake. "Urquhart’s Inflationary Universe." In The Culture of Translation in Early Modern England and France, 1500–1660. Palgrave Macmillan UK, 2015. http://dx.doi.org/10.1057/9781137401496_11.

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Saxena, Seema, Vikramjeet Singh, Rajesh Kumar Gupta, Pushpinder Singh, and Nitin Kumar Mishra. "A Supply Chain Replenishment Inflationary Inventory Model with Trade Credit." In Advances in Intelligent Systems and Computing. Springer Singapore, 2019. http://dx.doi.org/10.1007/978-981-15-0324-5_19.

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Anguelova, Lilia. "Primordial Black Hole Generation in a Two-Field Inflationary Model." In Springer Proceedings in Mathematics & Statistics. Springer Nature Singapore, 2022. http://dx.doi.org/10.1007/978-981-19-4751-3_13.

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Meisenheimer, Wolfgang. "Die Welt geht uns verloren. Modelle aber vermehren sich inflationär." In Modelle als Denkräume, Beispiele und Ebenbilder. Springer Fachmedien Wiesbaden, 2018. http://dx.doi.org/10.1007/978-3-658-20115-9_78.

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Conference papers on the topic "Inflationary Models"

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Leeper, Emily. "Exploring Inflationary Braneworld Models." In ALBERT EINSTEIN CENTURY INTERNATIONAL CONFERENCE. AIP, 2006. http://dx.doi.org/10.1063/1.2399679.

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Cohn, J. D. "Update on Open Universe Inflationary Models." In Proceedings of the First International Workshop on Particle Physics and the Early Universe. WORLD SCIENTIFIC, 1998. http://dx.doi.org/10.1142/9789814447263_0048.

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Mikheeva, E. "CURRENT OBSERVATIONAL CONSTRAINTS ON INFLATIONARY MODELS." In Proceedings of the Thirteenth Lomonosov Conference on Elementary Particle Physics. WORLD SCIENTIFIC, 2009. http://dx.doi.org/10.1142/9789812837592_0035.

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Polarski, David. "Gravitational wave background in inflationary models." In Cosmology and particle physics. AIP, 2001. http://dx.doi.org/10.1063/1.1363569.

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Nakayama, Kazunori, Hideo Kodama, and Kunihito Ioka. "Inflationary cosmology of axion models in supergravity." In KEK COSMOPHYSICS GROUP INAUGURAL CONFERENCE “ACCELERATORS IN THE UNIVERSE”: Interplay between High Energy Physics and Cosmophysics. AIP, 2008. http://dx.doi.org/10.1063/1.2981554.

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Das, Suratna, Kinjalk Lochan, Satyabrata Sahu, Shreya Banerjee, and T. P. Singh. "Classicalization of inflationary perturbations by collapse models." In Proceedings of the MG14 Meeting on General Relativity. WORLD SCIENTIFIC, 2017. http://dx.doi.org/10.1142/9789813226609_0341.

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Fomin, I. V. "High-frequency gravitational waves in exact inflationary models." In Twelfth Asia-Pacific International Conference on Gravitation, Astrophysics, and Cosmology. WORLD SCIENTIFIC, 2016. http://dx.doi.org/10.1142/9789814759816_0050.

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OLIVEIRA, H. P. DE, I. DAMIÃO SOARES, and E. V. TONINI. "CHAOS AND UNIVERSALITY IN THE DYNAMICS OF INFLATIONARY MODELS." In Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF). World Scientific Publishing Company, 2006. http://dx.doi.org/10.1142/9789812704030_0222.

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Landau, Susana J. "Testing non-standard inflationary models with the cosmic microwave background." In II COSMOSUR: COSMOLOGY AND GRAVITATION IN THE SOUTHERN CONE. AIP Publishing LLC, 2015. http://dx.doi.org/10.1063/1.4913328.

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Elizalde, E., E. O. Pozdeeva, and S. Yu Vernov. "Cosmological models with non-minimally coupled scalar fields and renormalization-group inflationary scenarios." In Twelfth Asia-Pacific International Conference on Gravitation, Astrophysics, and Cosmology. WORLD SCIENTIFIC, 2016. http://dx.doi.org/10.1142/9789814759816_0055.

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Reports on the topic "Inflationary Models"

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L'Huillier, Jean-Paul, and Gregory Phelan. Can Supply Shocks Be Inflationary with a Flat Phillips Curve? Federal Reserve Bank of Cleveland, 2023. http://dx.doi.org/10.26509/frbc-wp-202336.

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Not in standard models. With conventional pricing frictions, imposing a flat Phillips curve also imposes a price level that is rigid with respect to supply shocks. In the New Keynesian model, price markup shocks need to be several orders of magnitude bigger than other shocks in order to fit the data, leading to unreasonable assessments of the magnitude of the increase in costs during inflationary episodes. To account for the facts, we propose a strategic microfoundation of shock-dependent price stickiness: prices are sticky with respect to demand shocks but flexible with respect to supply shoc

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Storm, Servaas. Tilting at Windmills: Bernanke and Blanchard’s Obsession with the Wage-Price Spiral. Institute for New Economic Thinking Working Paper Series, 2024. http://dx.doi.org/10.36687/inetwp220.

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Bernanke and Blanchard (2023) use a simple dynamic New Keynesian model of wage-price determination to explain the sharp acceleration in U.S. inflation during 2021-2023. They claim their model closely tracks the pandemic-era inflation and they confidently conclude that “… we don’t think that the recent experience justifies throwing out existing models of wage-price dynamics.” This paper argues that this confidence is misplaced. The Bernanke and Blanchard is another failed attempt to salvage establishment macroeconomics after the massive onslaught of adverse inflationary circumstances with which

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Hauzenberger, Niko, Florian Huber, Gary Koop, and James Mitchell. Bayesian modeling of time-varying parameters using regression trees. Federal Reserve Bank of Cleveland, 2023. http://dx.doi.org/10.26509/frbc-wp-202305.

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In light of widespread evidence of parameter instability in macroeconomic models, many time-varying parameter (TVP) models have been proposed. This paper proposes a nonparametric TVP-VAR model using Bayesian additive regression trees (BART). The novelty of this model stems from the fact that the law of motion driving the parameters is treated nonparametrically. This leads to great flexibility in the nature and extent of parameter change, both in the conditional mean and in the conditional variance. In contrast to other nonparametric and machine learning methods that are black box, inference us

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Lawrence, David. UK trade and the war in Ukraine. Royal Institute of International Affairs, 2022. http://dx.doi.org/10.55317/9781784135379.

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- The UK is less exposed to the direct effects of Russia’s invasion of Ukraine than its European neighbours. However, the indirect and longer-term effects of the war on UK trade could still be significant. - Inflationary pressure worldwide will contribute to price rises in the UK, particularly for food and energy. The ongoing effects of both Brexit – which has caused cross-border supply frictions and worker shortages – and the COVID-19 pandemic – which led to pent-up domestic demand and further reduced the labour force – will only increase this upward pressure. - The war has prompted increased

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Stein, Ernesto H., and Jorge M. Streb. Political Stabilization Cycles in High Inflation Economies. Inter-American Development Bank, 1995. http://dx.doi.org/10.18235/0011614.

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High inflation economies often do not exhibit smooth inflationary processes, but rather stop-go cycles. This paper relates these stop-go episodes of inflation to a political cycle. The government can try to repress inflation until after the elections in order to increase the chances of being reelected. It is modeled as a two-period game of incomplete information where voters try to pick the most competent government, and inflation can be lowered by the government in the short run through foreign debt accumulation. Several stabilization episodes in Latin America, such as the Primavera Plan in A

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Ghomi, Morteza, Samuel Hurtado, and José Manuel Montero. Analysis of recent inflation dynamics in Spain. An approach based on the Blanchard and Bernanke (2023) model. Banco de España, 2024. http://dx.doi.org/10.53479/36294.

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The recent inflationary episode is the result of a series of shocks that have taken place over a short period of time. In this article we use the Blanchard and Bernanke (2023) model as an analytical framework to assess the relative importance of different factors over the course of this episode. Two main conclusions can be drawn from our results. First, supply-side shocks (related to energy, food and bottlenecks) have played a major role in recent inflation developments in the Spanish economy. Second, now that these supply shocks have been absorbed, labour market tightness is becoming more imp

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Lopez, Pierlauro, David Lopez-Salido, and Francisco Vazquez-Grande. Nominal rigidities and the term structures of equity and bond returns. Federal Reserve Bank of Cleveland, 2023. http://dx.doi.org/10.26509/frbc-wp-202311.

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We present a production economy with nominal price rigidities that explains several asset pricing facts, including a downward-sloping term structure of the equity premium, upward sloping term structures of nominal and real interest rates, and the cyclical variation of the term structures. In the model, after a productivity shock a countercyclical labor share exacerbates the procyclicality of dividends, and hence their riskiness, and generates countercyclical inflation. The dividend share gradually increases after a negative productivity shock as the price level increases sluggishly, so the pay

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Monetary Policy Report, January 2024. Banco de la República, 2024. http://dx.doi.org/10.32468/inf-pol-mont-eng.tr1-2024.

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Inflation continues to decline but remains well above 3%. It is anticipated to decrease significantly in 2024 and draw closer to the established target in the first half of 2025. The ongoing moderation in the economy's price levels is evidenced by the decline in headline inflation from 11% to 9.3% between September and December 2023. A noteworthy contributor to the decrease in inflation has been the reduction of food prices adjustments throughout 2023, complemented by favorable trends in the price of goods. The decrease in inflation has, however, been constrained by the behavior of the price o

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