Academic literature on the topic 'Inflation'

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Journal articles on the topic "Inflation"

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GERMÁN, G., and A. DE LA MACORRA. "INFLATION AT THE MAXIMA OF SYMMETRIC POTENTIALS." International Journal of Modern Physics A 20, no. 28 (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
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Salvio, Alberto. "Natural-scalaron inflation." Journal of Cosmology and Astroparticle Physics 2021, no. 10 (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 scalaro
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Watson, Scott, Malcolm J. Perry, Gordon L. Kane, and Fred C. Adams. "Inflation without inflaton(s)." Journal of Cosmology and Astroparticle Physics 2007, no. 11 (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, and Luisa G. Jaime. "Cosmic inflation without inflaton." International Journal of Modern Physics D 28, no. 14 (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, and CHIA-MIN LIN. "COMMENTS ON SUSY INFLATION MODELS ON THE BRANE." Modern Physics Letters A 25, no. 24 (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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James, Harold. "Hyperinflation after the First World War in Central Europe: Causes, Remedies, Consequences." Financial and Economic Review 23, no. 4 (2024): 54–68. https://doi.org/10.33893/fer.23.4.54.

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The paper examines in detail Germany and Poland, two of the four post-First World War hyperinflations that provided the subject of Thomas Sargent’s classic comparative study of the circumstances in which inflations might be ended. It counterposes the Czechoslovak case, where stabilisation occurred without prior hyperinflation. Stabilisation brought substantial costs, most obviously in terms of recession and unemployment. The peripheral inflating countries had sought to use inflation to effect an international as well as an internal redistribution of wealth. Ending the inflation was thus politi
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Fujita, Tomohiro, Kyohei Mukaida, and Tenta Tsuji. "Reheating after axion inflation." Journal of Cosmology and Astroparticle Physics 2025, no. 07 (2025): 002. https://doi.org/10.1088/1475-7516/2025/07/002.

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Abstract We investigate the reheating process in an axion inflation model where the inflaton couples to non-Abelian gauge fields via the Chern-Simons coupling. The Chern-Simons coupling leads to the efficient production of gauge fields via a tachyonic instability during inflation, whose implications have been actively studied in the literatures. Moreover, it has been recently pointed out that the produced gauge fields can be even thermalized during inflation, leading to warm inflation. Apparently, these findings seem to imply that the reheating is completed immediately after inflation because
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CHOU, CHUNG-HSIEN, and HOI-LAI YU. "DIGITAL ORIGIN OF COSMIC INFLATION." Modern Physics Letters A 25, no. 18 (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
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Narita, Yuma, Fuminobu Takahashi, and Wen Yin. "QCD axion hybrid inflation." Journal of Cosmology and Astroparticle Physics 2023, no. 12 (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 detaile
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Morishita, Yukiyoshi, Tomo Takahashi, and Shuichiro Yokoyama. "Multi-chaotic inflation with and without spectator field." Journal of Cosmology and Astroparticle Physics 2022, no. 07 (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 predic
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Dissertations / Theses on the topic "Inflation"

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

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Rudenko, T., and 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 no
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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 dua
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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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Books on the topic "Inflation"

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

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

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

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Berlatsky, Noah. Inflation. Greenhaven Press, 2012.

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Day, Kathleen. Inflation. CQ Press, 2022. http://dx.doi.org/10.4135/cqr_ht_inflation_2022.

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

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

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

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Riksbank, Sveriges. Inflation and inflation expectations in Sweden. Sveriges Riksbank, 1995.

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Corkish, Jo. Inflation, inflation risks and asset returns. Bank of England, 1994.

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Book chapters on the topic "Inflation"

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O’Neill, Robert, Jeff Ralph, and Paul A. Smith. "Introduction." In Inflation. 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, and Paul A. Smith. "From the RPI to the CPI: 1990–2011." In Inflation. 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, and Paul A. Smith. "Measuring Inflation at a Detailed Level." In Inflation. 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, and Paul A. Smith. "What Should We Be Measuring?" In Inflation. 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, and Paul A. Smith. "Recent Developments: 2012–2016." In Inflation. 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, and Paul A. Smith. "Other Price Indices." In Inflation. 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, and Paul A. Smith. "A Look to the Future." In Inflation. 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, and Paul A. Smith. "What Is Inflation?" In Inflation. 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, and Paul A. Smith. "The Origins of Inflation Measurement: 1700–1879." In Inflation. 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, and Paul A. Smith. "What Is a Price Index?" In Inflation. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-64125-6_4.

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Conference papers on the topic "Inflation"

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Racioppi, Antonio, and Alberto Salvio. "Natural Metric-Affine Inflation." In 2nd Training School and General Meeting of the COST Action COSMIC WISPers (CA21106). Sissa Medialab, 2025. https://doi.org/10.22323/1.474.0007.

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Koziuk, Viktor, Nataliia Dziubanovska, and Volodymyr Uhryn. "Money Supply vs Inflation Expectations: What Better Explains Inflation Behavior in Ukraine." In 2024 14th International Conference on Advanced Computer Information Technologies (ACIT). IEEE, 2024. http://dx.doi.org/10.1109/acit62333.2024.10712465.

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Nuthi, Pavan, Yixin Gu, Aida Nasirian, et al. "Reduction of Whole Body Vibration in a Wide Frequency Range Using Inflation Pressure Control of Air Bladder Cushion." In 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 c
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Burgess, Cliff. "Inflation." In Cargèse Summer School: Cosmology and Particle Physics Beyond the Standard Models. Sissa Medialab, 2009. http://dx.doi.org/10.22323/1.049.0003.

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BAUMANN, DANIEL. "INFLATION." In 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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Arkhipova, N., and N. Fedorov. "The evolution of fields in the process of preheating in the early Universe." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.019.

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The long-term evolution of fields on the stage of primary heating of the Universe after inflation is investigated. Preheating is the stage of evolution of the Universe at which the inflaton, after the stage of slow rolling down on inflation, begins to oscillate near the minimum of its potential energy and act as a compelling external force in the equations of motion of other fields that were in a quantum state with a relatively small amplitude on inflation. Numerical calculations of the system's dynamics for long times shows that during the early phase of preheating, the energy of the material
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Tomfort, André. "The Dynamics of Inflation and Inflation Expectations." In 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." In 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." In 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." In Cosmology and particle physics. AIP, 2001. http://dx.doi.org/10.1063/1.1363506.

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Reports on the topic "Inflation"

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

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

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

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

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

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Martínez-Rivera, Wilmer, Edgar Caicedo-García, and Juan Bonilla-Pérez. Instantaneous Inflation as a Predictor of Inflation. Banco de la República, 2025. https://doi.org/10.32468/be.1296.

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This article studies the relationship between instantaneous and year-on-year inflation and the benefit of the forecast performance using instantaneous as a predictor. Instantaneous inflation is a transformation of year-on-year inflation, assigning different weights to each month of the Consumer Price Index (CPI) used to calculate the year-on-year inflation. We study the relationship using the Coincident Profile, which allows us to determine whether instantaneous inflation is coincident or anticipates the dynamic of year-on-year inflation. This finding establishes the lag order of the VAR, VECM
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Green, Dan. Inflation Basics. Office of Scientific and Technical Information (OSTI), 2014. http://dx.doi.org/10.2172/1304776.

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Stock, James, and Mark Watson. Forecasting Inflation. National Bureau of Economic Research, 1999. http://dx.doi.org/10.3386/w7023.

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

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

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