Bibliografías temáticas / Inflation

Literatura académica sobre el tema "Inflation"

Autor: Grafiati

Publicado: 4 de junio de 2021

Última modificación: 1 de junio de 2024

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Artículos de revistas sobre el tema "Inflation"

GERMÁN, G. y A. DE LA MACORRA. "INFLATION AT THE MAXIMA OF SYMMETRIC POTENTIALS". International Journal of Modern Physics A 20, n.º 28 (10 de noviembre de 2005): 6451–59. http://dx.doi.org/10.1142/s0217751x05025541.

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We construct a two-stage inflationary model which can accommodate early inflation at a scale Λ1 as well as a second stage of inflation at Λ2 with a single scalar field ϕ. We use a symmetric potential, valid in a frictionless world, in which the two inflationary periods have exactly the same scale, i.e. Λ1 = Λ2. However, we see today Λ1 ≫ Λ2 due to the friction terms (expansion of the universe and interaction with matter). These type of models can be motivated from supergravity. Inflation occurs close to the maxima of the potential. As a consequence both inflations are necessarily finite. This opens the interesting possibility that the second inflation has already or is about to end. A first inflation is produced when fluctuations displace the inflaton field from its higher maximum rolling down the potential as in new inflation. Instead of rolling towards a global minimum the inflaton approaches a lower maximum where a second inflation takes place.

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Salvio, Alberto. "Natural-scalaron inflation". Journal of Cosmology and Astroparticle Physics 2021, n.º 10 (1 de octubre de 2021): 011. http://dx.doi.org/10.1088/1475-7516/2021/10/011.

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Abstract A pseudo Nambu-Goldstone boson (such as an axion-like particle) is a theoretically well-motivated inflaton as it features a naturally flat potential (natural inflation). This is because Goldstone's theorem protects its potential from sizable quantum corrections. Such corrections, however, generically generates an R 2 term in the action, which leads to another inflaton candidate because of the equivalence between the R 2 term and a scalar field, the scalaron, with a quasi flat potential (Starobinsky inflation). Here it is investigated a new multifield scenario in which both the scalaron and a pseudo Nambu-Goldstone boson are active (natural-scalaron inflation). For generality, also a non-minimal coupling is included, which is shown to emerge from microscopic theories. It is demonstrated that a robust inflationary attractor is present even when the masses of the two inflatons are comparable. Moreover, the presence of the scalaron allows to satisfy all observational bounds in a large region of the parameter space, unlike what happens in pure-natural inflation.

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Watson, Scott, Malcolm J. Perry, Gordon L. Kane y Fred C. Adams. "Inflation without inflaton(s)". Journal of Cosmology and Astroparticle Physics 2007, n.º 11 (21 de noviembre de 2007): 017. http://dx.doi.org/10.1088/1475-7516/2007/11/017.

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Arciniega, Gustavo, Pablo Bueno, Pablo A. Cano, José D. Edelstein, Robie A. Hennigar y Luisa G. Jaime. "Cosmic inflation without inflaton". International Journal of Modern Physics D 28, n.º 14 (octubre de 2019): 1944008. http://dx.doi.org/10.1142/s0218271819440085.

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We propose a novel explanation for universe’s inflationary period. We argue that when the Einstein–Hilbert action is supplemented by an infinite tower of higher-curvature terms — selected order by order by the criterium that they give rise to a well-posed cosmological evolution — the usual Big Bang characteristic of Einstein gravity is replaced by a singularity-free period of exponential growth of the scale factor, which is gracefully connected with standard late-time [Formula: see text]CDM cosmology. No inflaton or any additional fields besides the metric are required.

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LEE, LU-YUN, KINGMAN CHEUNG y CHIA-MIN LIN. "COMMENTS ON SUSY INFLATION MODELS ON THE BRANE". Modern Physics Letters A 25, n.º 24 (10 de agosto de 2010): 2105–10. http://dx.doi.org/10.1142/s0217732310033487.

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In this paper we consider a class of inflation models on the brane where the dominant part of the inflaton scalar potential does not depend on the inflaton field value during inflation. In particular, we consider supernatural inflation, its hilltop version, A-term inflation, and supersymmetric (SUSY) D- and F-term hybrid inflation on the brane. We show that the parameter space can be broadened, the inflation scale generally can be lowered, and still possible to have the spectral index ns = 0.96.

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CHOU, CHUNG-HSIEN y HOI-LAI YU. "DIGITAL ORIGIN OF COSMIC INFLATION". Modern Physics Letters A 25, n.º 18 (14 de junio de 2010): 1483–89. http://dx.doi.org/10.1142/s0217732310033219.

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Assuming our physical universe processes and registers information to determine its dynamical evolution, one can put serious constraints on the cosmology that our universe can bear, in particular, the origin of cosmic inflation. The universe evolves to gain her computation capacity which is linear in time t. On the other hand, the growth in content of degrees of freedom (i.e. by integrating in more galaxies) is as t3/2 through expansion. When the in flux of degrees of freedom of the universe grows beyond some value, the computation capacity of the universe becomes insufficient to determine its evolution, the universe fixes its Hubble radius and inflates away its degrees of freedom within its horizon to regain dynamical evolution. The length of inflation is determined by the communication time required by the universe to become aware of the dropping in the degrees of freedom below some critical value by inflation and is proportional to its Hubble radius. We predict that there can be multiple cosmic inflations. The next inflation era will stop after inflating for a period of 1019 sec if the past inflation period of our universe was 10-33 sec.

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Narita, Yuma, Fuminobu Takahashi y Wen Yin. "QCD axion hybrid inflation". Journal of Cosmology and Astroparticle Physics 2023, n.º 12 (1 de diciembre de 2023): 039. http://dx.doi.org/10.1088/1475-7516/2023/12/039.

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Abstract When the inflaton is coupled to the gluon Chern-Simons term for successful reheating, mixing between the inflaton and the QCD axion is generally expected given the solution of the strong CP problem by the QCD axion. This is particularly natural if the inflaton is a different, heavier axion. We propose a scenario in which the QCD axion plays the role of the inflaton by mixing with heavy axions. In particular, if the energy scale of inflation is lower than the QCD scale, a hybrid inflation is realized where the QCD axion plays the role of the inflaton in early stages. We perform detailed numerical calculations to take account of the mixing effects. Interestingly, the initial misalignment angle of the QCD axion, which is usually a free parameter, is determined by the inflaton dynamics. It is found to be close to π in simple models. This is the realization of the pi-shift inflation proposed in previous literature, and it shows that QCD axion dark matter and inflation can be closely related. The heavy axion may be probed by future accelerator experiments.

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Morishita, Yukiyoshi, Tomo Takahashi y Shuichiro Yokoyama. "Multi-chaotic inflation with and without spectator field". Journal of Cosmology and Astroparticle Physics 2022, n.º 07 (1 de julio de 2022): 042. http://dx.doi.org/10.1088/1475-7516/2022/07/042.

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Abstract Motivated by the result of Planck+BICEP/Keck recently released, we investigate the consistency of the multi-field inflation models in terms of the spectral index ns and the tensor-to-scalar ratio r. In this study, we focus on double-inflaton models with and without a spectator field. We find that inflaton with a quadratic potential can become viable when three fields with a specific hierarchical mass spectrum are realized such that two fields act as inflatons and the other one is the spectator. We also discuss the conditions to avoid the fine-tuning, by careful study of how the prediction depends on the background trajectory in the inflaton-field space.

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Salunkhe, Bhavesh y Anuradha Patnaik. "Inflation Dynamics and Monetary Policy in India: A New Keynesian Phillips Curve Perspective". South Asian Journal of Macroeconomics and Public Finance 8, n.º 2 (28 de agosto de 2019): 144–79. http://dx.doi.org/10.1177/2277978719861186.

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The present study estimates various specifications of the New Keynesian Phillips Curve (NKPC) models for India over 1996Q2 to 2017Q2 using Consumer Price Index (CPI) and Wholesale Price Index (WPI) inflation, separately. The empirical results suggest that the data support all the specifications of the Phillips curve models based on both the CPI and WPI inflations. However, the backward looking and hybrid models provide robust results for both the inflation indices. While the forward-looking behaviour dominates the CPI inflation trajectory, the backward-looking behaviour greatly influences the trajectory of WPI inflation. Also, a small-to-moderate degree of persistence is evident in both the CPI and WPI inflation. The output gap, which mainly represents the demand side pressures, turns up the major force determining both the CPI and WPI inflations. Besides the output gap, real effective exchange rate (reer), international crude oil price inflation, global non-fuel commodity price inflation and rainfall have a modest impact on the CPI and WPI inflations. JEL Classification: E12, E52, C36, C14

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Aliraqi, Ali. "Inflation’s Impact on Sudan Exports 1990-2020: An ARDL Approach". World Journal of Entrepreneurship, Management and Sustainable Development 18, n.º 6 (10 de enero de 2023): 707–27. http://dx.doi.org/10.47556/j.wjemsd.18.6.2022.2.

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Purpose: This study investigates the inflation-export nexus in Sudan over the period 1990- 2020. Design/methodology: The study is based on quantitative and qualitative methods, estimating the export function and measuring the impact of its determinants over a prolonged period of time; the Autoregressive Distributed Lag (ARDL) methodology was used to analyse the co-integration. Findings: Findings have undoubtedly shown inflation’s negative impact on exports over the period 1990-2020. Broadly speaking, the long-term results indicated that the most important variable affecting exports is the gross domestic product (GDP), followed by inflation. Interestingly, the results indicated that the exchange rate was not significant, neither in the short nor in the long term. Implications: The study recommends inflation's control policy as a perquisite for an export development strategy; this overcomes barriers and paves the road for shifting Sudan's economy to productive agendas. Therefore, targeting inflation will contribute to export diversification and strengthening the product's value chain. The research findings reconsider the weight of export’s determinants and will reposition focusing to inflation control rather than exchange rate policy. Originality/value: The paper introduces a new approach in modelling the inflation-export nexus: (1) elaborate on export's determinants and their weights; and (2) recommending guidelines to adapt inflation policy with export development strategy.

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Tesis sobre el tema "Inflation"

Lozanov, Kaloian Dimitrov. "Expansion after inflation and reheating with a charged inflaton". Thesis, University of Cambridge, 2017. https://www.repository.cam.ac.uk/handle/1810/267822.

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Within the inflationary paradigm, our patch of the universe near the end of inflation is highly homogeneous and isotropic as necessitated by cosmic microwave background observations. This patch, however, is also in a cold and non-thermal state. A successful model of an inflationary primordial universe should account for how the universe transitioned from an inflationary to a radiation-dominated, hot, thermal phase required for the production of light elements via big-bang nucleosynthesis. It is desirable for such a model also to include a mechanism for the generation of the observed matter-antimatter asymmetry and perhaps a primordial mechanism for the generation of cosmic magnetic fields. The transition from an inflationary to a radiation-dominated, thermal phase (reheating) is likely to be phenomenologically rich. Reheating could include explosive particle production and various other non-perturbative, non-linear and non-equilibrium phenomena. Reheating can leave its own observational signatures in the form of gravitational waves and non-Gaussianities. Importantly, reheating can also affect the observational predictions of the preceding phase of inflation. Reheating remains an active field of research, with significant gaps in our understanding of the process. This thesis is an attempt to improve our understanding of the period following inflation, including reheating, through an exploration and analysis of realistic post-inflationary models with the aid of detailed numerical simulations. The focus of the studies is on aspects of the models with potential observational implications. In Part I of this thesis, we provide an overview of inflation and its end, concentrating on our current understanding of reheating and the challenges we face in trying to constrain reheating observationally. In Part II, we consider the post-inflationary expansion history in a broad class of observationally-favoured single-field models of inflation. Generally, the ambiguity in the expansion history of reheating can cause significant uncertainty in predictions for inflationary observables such as the spectral index, n_s, and the tensor-to-scalar ratio, r. The work in this part considers the full non-linear evolution of the inflaton during the initial stages of reheating and places bounds on the post-inflationary expansion history when perturbative couplings of the inflaton to other relativistic fields are included. In Part III, we investigate non-perturbative particle production and non-linear dynamics after inflation in models where the inflaton is charged under global/local symmetries. We first explore the effects of the non-linear inflaton dynamics for the generation of matter-antimatter asymmetry in the case where a global U(1) symmetry of the inflaton is weakly broken. We find a parameter range in which the model successfully predicts the observed baryon-to-photon ratio. We then consider the particle production during and after inflation in models with a charged inflaton under Abelian, U(1), and non-Abelian, SU(2) and U(1) x SU(2), gauge symmetries. Finally, we present a novel algorithm for evolving the full set of coupled, non-linear equations describing the U(1) charged inflaton and accompanying gauge fields on a lattice in an expanding universe. The novel feature here is that the gauge constraints are satisfied to machine precision when the gravitational dynamics are self-consistently included at the background level, and there are no restrictions on the order of the time-integrators.

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Schildt, Erik. "Higgs inflation". Thesis, Uppsala universitet, Teoretisk fysik, 2018. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-355063.

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In this project a recent model of inflation in which the Standard Model Higgs field with a nonminimal coupling to gravity takes on the role of the inflaton field is investigated. The tensor to scalar ratio, spectral index and the running of the spectral index is calculated for a tree level analysis and compared with the Planck experiment. The value of the nonminimal coupling constant $\xi$ is estimated by obtaining a relation between the amplitude of scalar perturbations and the Higgs mass, it is found that $\xi \sim 10^4$. The basic aspects of how the results are modified through quantum corrections and what the consequences of the nonminimal coupling are for the effective field theory description is discussed. It is found that a tree level analysis yields predictions which are inside the allowed regions of the cosmological parameters given by the Planck experiment. The large value of the nonminimal coupling leads to unitarity problems for this model of inflation. However quantum effects will have a significant effect and how they modify the results of the tree level analysis is what decides if Higgs inflation is a viable theory.
I detta projekt undersöker vi en modell av kosmisk inflation där Higgsfältet med en ickeminimal koppling till tyngdkraften är mekanismen bakom inflation. Vi utför en klassisk analys och beräknar modellens föresägelser för ett antal kosmologiska parametrar som jämförs med Planck experimentet. Vi uppskattar värdet på den ickeminimala kopplingen $\xi$ och finner att $\xi \sim 10^4$. De grundläggande aspekterna bakom kvantanalysen samt vad effekten av den ickeminimala kopplingen har på beskrivningen i termer av en effektiv fältteori diskuteras. Vi finner att en klassisk analys ger förutsägelser som passar väl med Planckexperimentet men att den ickeminimala kopplingen leder till unitaritetsproblem för denna modell av inflation. Kvanteffekter kan dock ha en avsevärd effekt på resultat och en utförlig analys som tar dem till hänsyn krävs för att avgöra om Higgsinflation är en möjlig modell för inflation.

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Морозова, Ірина Анатоліївна, Ирина Анатольевна Морозова, Iryna Anatoliivna Morozova y N. Prihodko. "Inflation". Thesis, Видавництво СумДУ, 2010. http://essuir.sumdu.edu.ua/handle/123456789/17505.

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Rudenko, T. y T. M. Burenko. "Inflation". Thesis, Вид-во СумДУ, 2009. http://essuir.sumdu.edu.ua/handle/123456789/16749.

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Wieland, Elisabeth. "Essays on inflation uncertainty and inflation expectations". Diss., Ludwig-Maximilians-Universität München, 2013. http://nbn-resolving.de/urn:nbn:de:bvb:19-165216.

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Jeke, Leward. "Inflation targeting and inflation indicators: the case for inflation targeting in South Africa". Thesis, University of Fort Hare, 2012. http://hdl.handle.net/10353/d1007091.

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The control of inflation requires a forecast of the future path of the price level and its indicators. Targeting inflation directly requires that the central bank (SARB) form forecasts of the likely path of prices paying close attention to a variety of indicators that shows the predictive power of inflation in the past periods. Inflation indicators might be cointegrated with the rate of inflation to predict the future inflation rates. Forecasting inflation may be very difficult at a particular period due to the fact that the array candidate indicators of inflation may neither be very stable nor very strong in their relationships with the rate of inflation. Although this might be the case, this research uses testable effects of each of the South African inflation indicators to the rate of inflation using econometrics tools to find that they have a long run trend with the rate of inflation in South Africa. It has been found that each of the indicator variables has a long run relationship with the rate of inflation. The major conclusion is that inflation indicator variables like money supply (M3), oil price, gold price, total employment, interest rates, exchange rates and output growth can be useful inflation indicators in targeting the future trends of inflation in South Africa according to the data used in this research although some studies in some countries find that inflation targeting is an insufficient framework for monetary policy in the presence of financial exuberance. The money supply, the oil prices, interest rates, the exchange rates, prices of gold, the employment and output growth are co-integrated with the rate of inflation representing a long-run relationship.

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Ghorbani-Aghilabadi, Payman. "Modelling monetary transmission mechanism, inflation, and inflation uncertainty". Thesis, University of Essex, 2006. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.428960.

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Henzel, Steffen. "Inflation Dynamics and the Role of Inflation Expectation Formation". Diss., lmu, 2008. http://nbn-resolving.de/urn:nbn:de:bvb:19-89335.

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Dias, Mafalda. "Ultraviolet complete inflation : looking at inflation from fundamental physics". Thesis, University of Sussex, 2013. http://sro.sussex.ac.uk/id/eprint/44139/.

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To completely describe the inflationary era in the early universe is an extremely ambitious task. The main reason is that its dynamics are highly sensitive to ultraviolet physics, making the knowledge of inflation dependent on our ignorance of what is happening at these energy scales. This is not necessarily a weakness of inflation as a paradigm; it is ultimately its most interesting characteristic. Accepting this lack of control on the details of inflationary dynamics brings observational cosmology and the search for an ultraviolet complete theory of gravity together. In this thesis, this duality is explored with the aim of making steps towards an efficient way of studying inflation and its predictions and signatures. This challenge is twofold; first, since fundamental theories are far from being able to explicitly determine the early universe physics, the construction of approximate toy models is unavoidable. For this reason, I identify the key issues for the building of a realistic inflation model, in particular the delicate flatness of the inflaton potential, the strong possibility of multifield dynamics and the necessity of a viable reheating, and in the light of these analyze how best to approximate an ultraviolet complete inflation. For this analysis, two different classes of case studies are presented: inflation in the brane picture and in a holography inspired scenario. On the other hand, since any toy model of an ultraviolet complete inflation necessarily presents a high level of complexity, the computation of predictions for observables is not trivial. For this purpose, I develop numerical tools that manage to compute these parameters efficiently and with a high level of accuracy for a broad range of inflation classes with more than one active field. For each case study, I determine the impact of the inclusion of microphysics contributions in the resulting observational signatures and confront them with data.

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Lin, Chia-Min. "Inflation Models in the Era of Precision Observations : Modified D-term Inflation and Hilltop Inflation Models". Thesis, Lancaster University, 2008. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.518205.

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Libros sobre el tema "Inflation"

Cecchetti, Stephen G. Inflation indicators and inflation policy. Cambridge, MA: National Bureau of Economic Research, 1995.

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O'Neill, Robert, Jeff Ralph y Paul A. Smith. Inflation. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-64125-6.

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Inflation. London: Chapman & Hall, 1992.

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Hall, Robert E. Inflation. Chicago: University of Chicago Press, 2009.

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Bacon, Peter. Inflation. Dublin: Confederation of Irish Industry, 1989.

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Berlatsky, Noah. Inflation. Detroit, MI: Greenhaven Press, 2012.

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Day, Kathleen. Inflation. 2455 Teller Road, Thousand Oaks California 91320 United States: CQ Press, 2022. http://dx.doi.org/10.4135/cqr_ht_inflation_2022.

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Sveriges Riksbank. Economics Department., ed. Inflation and inflation expectations in Sweden. Stockholm: Sveriges Riksbank, Economics Department, 1994.

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Library of Congress. Congressional Research Service, ed. Inflation indexing: Does it exacerbate inflation? Washington, D.C: Congressional Research Service, Library of Congress, 1986.

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Riksbank, Sveriges. Inflation and inflation expectations in Sweden. [Stockholm]: Sveriges Riksbank, 1995.

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Capítulos de libros sobre el tema "Inflation"

O’Neill, Robert, Jeff Ralph y Paul A. Smith. "Introduction". En Inflation, 1–20. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-64125-6_1.

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O’Neill, Robert, Jeff Ralph y Paul A. Smith. "From the RPI to the CPI: 1990–2011". En Inflation, 221–41. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-64125-6_10.

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O’Neill, Robert, Jeff Ralph y Paul A. Smith. "Measuring Inflation at a Detailed Level". En Inflation, 243–63. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-64125-6_11.

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O’Neill, Robert, Jeff Ralph y Paul A. Smith. "What Should We Be Measuring?" En Inflation, 265–86. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-64125-6_12.

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O’Neill, Robert, Jeff Ralph y Paul A. Smith. "Recent Developments: 2012–2016". En Inflation, 287–332. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-64125-6_13.

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O’Neill, Robert, Jeff Ralph y Paul A. Smith. "Other Price Indices". En Inflation, 333–54. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-64125-6_14.

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O’Neill, Robert, Jeff Ralph y Paul A. Smith. "A Look to the Future". En Inflation, 355–69. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-64125-6_15.

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O’Neill, Robert, Jeff Ralph y Paul A. Smith. "What Is Inflation?" En Inflation, 21–43. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-64125-6_2.

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O’Neill, Robert, Jeff Ralph y Paul A. Smith. "The Origins of Inflation Measurement: 1700–1879". En Inflation, 45–67. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-64125-6_3.

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O’Neill, Robert, Jeff Ralph y Paul A. Smith. "What Is a Price Index?" En Inflation, 69–90. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-64125-6_4.

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Actas de conferencias sobre el tema "Inflation"

Nuthi, Pavan, Yixin Gu, Aida Nasirian, Alexandra Lindsay, Himanshu Purandare, Nischita Haldipurkar, Kashish Shah y Muthu B. J. Wijesundara. "Reduction of Whole Body Vibration in a Wide Frequency Range Using Inflation Pressure Control of Air Bladder Cushion". En ASME 2021 International Design Engineering Technical Conferences and Computers and Information in Engineering Conference. American Society of Mechanical Engineers, 2021. http://dx.doi.org/10.1115/detc2021-71374.

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Abstract Several types of interfaces like foam and inflated air cells exist to reduce the effect of mechanical vibration experienced in human-machine interfaces in different scenarios such as transportation. However, their vibration attenuation performance in a wide frequency range relevant to whole body vibration (1–80 Hz) leaves much to be desired. In this study, we investigate the effect of inflation pressure on the vibration attenuation behavior of an air cell cushion. An experimental setup capable of conducting frequency sweep tests and regulating inflation pressure in an air cell array cushion was developed. Frequency sweep tests were conducted at various inflations and the vibration transmissibilities at static inflations were plotted. A dynamic inflation scheme was developed based on the apriori knowledge of inflation dependent transmissibilities. Furthermore, the closed loop behavior of the inflation scheme was evaluated with a frequency sweep test. The resulting closed loop transmissibility indicated better vibration attenuation performance than any single static inflation for the air cell array cushion in the range of frequencies relevant to whole body vibration. This result lays the groundwork for potential air cell cushions which modify their inflation dynamically through a direct feedback from sensors like accelerometers to attenuate vibration in a wide frequency range.

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Burgess, Cliff. "Inflation". En Cargèse Summer School: Cosmology and Particle Physics Beyond the Standard Models. Trieste, Italy: Sissa Medialab, 2009. http://dx.doi.org/10.22323/1.049.0003.

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BAUMANN, DANIEL. "INFLATION". En Proceedings of the Theoretical Advanced Study Institute in Elementary Particle Physics. WORLD SCIENTIFIC, 2011. http://dx.doi.org/10.1142/9789814327183_0010.

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Tomfort, André. "The Dynamics of Inflation and Inflation Expectations". En Annual International Conference on Qualitative and Quantitative Economics Research. Global Science and Technology Forum (GSTF), 2011. http://dx.doi.org/10.5176/978-981-08-8957-9_qqe-047.

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ROSS, G. G. "MULTIPLE INFLATION". En Proceedings of the First International Workshop on Particle Physics and the Early Universe. WORLD SCIENTIFIC, 1998. http://dx.doi.org/10.1142/9789814447263_0039.

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Mukhanov, V. "Cosmic Inflation". En COSMOLOGY AND GRAVITATION: XIIth Brazilian School of Cosmololy and Gravitation. AIP, 2007. http://dx.doi.org/10.1063/1.2752479.

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Turok, Neil. "Before inflation". En Cosmology and particle physics. AIP, 2001. http://dx.doi.org/10.1063/1.1363506.

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Alawaq, Abdulhamid. "constitutional inflation". En INTERNATIONAL CONFERENCE OF DEFICIENCIES AND INFLATION ASPECTS IN LEGISLATION. University of Human Development, 2021. http://dx.doi.org/10.21928/uhdicdial.pp1-17.

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Resumen

One of the methods that the authority uses to empty the constitutional text of its content and prevent it from achieving its goal is its resort to the two phenomena of “constitutional inflation” in sites that the nation does not need, and “constitutional failure” in sites that are expected from the text to protect public rights and freedoms or prevent an authority from overpowering the rest of the authorities. This is how the authority did in the Syrian constitution of 2012. It resorted to both phenomena together to achieve its goal of using the constitution as a tool and not as a control of the authority’s work. If legislative inflation is clear to legal jurisprudence, constitutional inflation is shrouded in ambiguity, so it resorted to a procedural definition of the research paper and considered every constitutional rule that does not bear the status of binding as a type of inflation. then I applied this definition to the general principles contained in the Syrian constitution in 32 articles, unlike democratic constitutions, which are shortened to articles regulating the general principles of the state. It became clear to me that only five articles are binding and the rest are non-binding guiding articles that are not suitable for reliance on judicial review. I have studied the rule (Islamic jurisprudence is a major source of legislation) in Syria and Egypt, and it has become clear to me that the authority intends to put it into place as a kind of distraction from paying attention to the rest of the constitution’s rules regulating public liberties and powers, even though the constitutional doctrine considers them to be non-binding. The struggle between the components of the people is still going on when drafting any constitution on general principles, most of which do not carry legal value.

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Garcia-Saenz, Sebastian, Sébastien Renaux-Petel y John Ronayne. "Sidetracked inflation". En Proceedings of the MG15 Meeting on General Relativity. WORLD SCIENTIFIC, 2022. http://dx.doi.org/10.1142/9789811258251_0208.

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Filippas, Apostolos, John Joseph Horton y Joseph Golden. "Reputation Inflation". En EC '18: ACM Conference on Economics and Computation. New York, NY, USA: ACM, 2018. http://dx.doi.org/10.1145/3219166.3219222.

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Informes sobre el tema "Inflation"

Holman, R., Yun Wang y E. W. Kolb. Gravitational couplings of the inflaton in extended inflation. Office of Scientific and Technical Information (OSTI), febrero de 1990. http://dx.doi.org/10.2172/6965978.

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Cecchetti, Stephen. Inflation Indicators and Inflation Policy. Cambridge, MA: National Bureau of Economic Research, junio de 1995. http://dx.doi.org/10.3386/w5161.

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Stock, James y Mark Watson. Core Inflation and Trend Inflation. Cambridge, MA: National Bureau of Economic Research, junio de 2015. http://dx.doi.org/10.3386/w21282.

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Ball, Laurence. Why Does High Inflation Raise Inflation Uncertainty? Cambridge, MA: National Bureau of Economic Research, enero de 1990. http://dx.doi.org/10.3386/w3224.

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Mishkin, Frederic y Niklas Westelius. Inflation Band Targeting and Optimal Inflation Contracts. Cambridge, MA: National Bureau of Economic Research, julio de 2006. http://dx.doi.org/10.3386/w12384.

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Green, Dan. Inflation Basics. Office of Scientific and Technical Information (OSTI), marzo de 2014. http://dx.doi.org/10.2172/1304776.

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Stock, James y Mark Watson. Forecasting Inflation. Cambridge, MA: National Bureau of Economic Research, marzo de 1999. http://dx.doi.org/10.3386/w7023.

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Berkin, A. L., Kei-ichi Maeda y Jun'ichi Yokoyama. Soft inflation. Office of Scientific and Technical Information (OSTI), abril de 1990. http://dx.doi.org/10.2172/6917229.

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Svensson, Lars E. O. Inflation Targeting. Cambridge, MA: National Bureau of Economic Research, diciembre de 2010. http://dx.doi.org/10.3386/w16654.

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Green, Dan. Inflation Basics. Office of Scientific and Technical Information (OSTI), enero de 2014. http://dx.doi.org/10.2172/1163143.

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