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Inflación
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461“…The Poisson and Conway–Maxwell–Poisson (CMP) distributions, and their zero-Inflated (ZI) versions were applied to fit the data. …”
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462“…Our findings show that the pandemic inflation is higher than the official inflation rate during the first lockdown, suggesting a behavioral change in consumption. …”
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463“…While our investigation is preliminary, it provides insights into additional understanding of effectiveness of policy actions on inflation targeting.…”
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464“…Empirical findings show that the oil price and temperature can be significant factors for reducing food inflation. According to the result of variance decomposition, in general, a considerable part of food inflation was explained by the exchange rate, but its effect did not show any significant change in the long term. …”
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465por Craighead, William D.“…In the model, the relative demand shock leads to opposite movements in inflation and labor between the two sectors, while the shock to labor disutility is stagflationary, with inflation rising and output decreasing. …”
Publicado 2022
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466por Niazi, Sarfaraz K.“…WHAT IS KNOWN AND OBJECTIVE: After more than a year of negotiation, a $740 billion climate and health care bill known as The Inflation Reduction Act (IRA) became law on 16 August 2022. …”
Publicado 2022
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467por Klonner, Moriz Ettore, Mattaliano, Giorgio, Casoria, Vincenzo, Vogl, Claus, Braun, Christina“…Blind techniques for cuff inflation have been shown to rarely result in an optimal cuff pressure, even when used by experienced anaesthesiologists. …”
Publicado 2023
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468por Hunt, Katie A., Ali, Kamal, Dassios, Theodore, Milner, Anthony D., Greenough, Anne“…Some guidelines specify short inflations delivered at rates of 40–60/min, others recommend initial inflations lasting 2–3 s or sustained inflations lasting for ≥ 5 s for initial resuscitation. …”
Publicado 2017
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469“…We study Dirac-Born-Infeld (DBI) inflation models with multiple scalar fields. We show that the adiabatic and entropy modes propagate with a common effective sound speed and are thus amplified at the sound horizon crossing. …”
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470“…We study cosmological perturbations in general inflation models with multiple scalar fields and arbitrary kinetic terms, with special emphasis on the multi-field extension of Dirac-Born-Infeld (DBI) inflation. …”
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471“…We introduce a simple string model of inflation, in which the inflaton field can take trans-Planckian values while driving a period of slow-roll inflation. …”
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472“…We present new cosmological constraints on single-field inflation in light of the Wilkinson Microwave Anisotropy Probe satellite mission five-year results (WMAP5). …”
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473por Griebel, Hannes“…In this concept, the probe deploys an inflatable drag body out in space and may then enter the atmosphere either once or several times until it slowly descends towards the ground, taking continuous atmospheric and other readings across a large altitude and ground range. …”
Publicado 2010
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474por Achucarro, Ana, Gong, Jinn-Ouk, Hardeman, Sjoerd, Palma, Gonzalo A, Patil, Subodh P“…The resulting operator expansion is distinguishable from that of other scenarios, such as standard single inflation or DBI inflation. In particular, we re-derive how certain operators can become transiently strongly coupled along the inflaton trajectory, consistent with slow-roll and the validity of the EFT expansion, imprinting features in the primordial power spectrum, and we deduce the relevant cubic operators that imply distinct signatures in the primordial bispectrum which may soon be constrained by observations.…”
Publicado 2012
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477“…The supersymmetric extension of "Starobinsky" $R+\alpha R^2$ models of inflation is particularly simple in the "new minimal" formalism of supergravity, where the inflaton has no scalar superpartners. …”
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478“…Higgs inflation is attractive because it identifies the inflaton with the electroweak Higgs boson. …”
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479“…Here we study the question if this model can also lead to inflation by identifying the dilaton with the inflaton. …”
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480por Giovannini, Massimo“…Non-monotonic spectra with a maximum in the MHz region correspond to a limited variation of the refractive index terminating well before the end of inflation. After exploring a general approach encompassing the ones proposed so far, we estimate the required sensitivity for the direct detection of the predicted gravitational radiation and demonstrate that the allowed regions of the parameter space are within reach for some of the planned detectors operating either in the audio band (like Ligo/Virgo and Kagra) or in the mHz band (like Lisa, Bbo and Decigo).…”
Publicado 2018
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