Mostrando 1,681 - 1,700 Resultados de 7,249 Para Buscar '"inflation"', tiempo de consulta: 0.11s Limitar resultados
  1. 1681
    por Rajagukguk, Wilson
    Publicado 2022
    “…Higher internet use was also associated with higher access to electricity, higher GDP, lower inflation rate, and higher foreign direct investment inflow. …”
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  2. 1682
    “…People’s estimates are also shaped by affective dynamics, in particular a more pessimistic outlook that leads to overestimation of official unemployment and inflation (but not growth) figures. We find that emotive factors can bias inflation and unemployment estimates of respondents who find themselves in a privileged economic situation in a direction that incidentally also makes them more accurate, even though respondents are not necessarily being better informed. …”
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  3. 1683
  4. 1684
    “…Results showed that with the increases in carbon tax, the inflation rate was increased, the rate of carbon emission reduction was increased, and the negative effects on GDP and employment were also increased. …”
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  5. 1685
    por King, B. B.
    Publicado 1983
    Tabla de Contenidos: “…Inflation blues -- Broken heart -- Sell my monkey -- Heed my warning -- Teardrops from my eyes -- Rainbow riot -- Darlin' you know I love you -- Make love to me -- I can't let you go.…”
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  6. 1686
    por Liddle, Andrew
    Publicado 2015
    “…Properties of the very early Universe are also covered, including the motivation for a rapid period of expansion known as cosmological inflation. The third edition brings this established undergraduate textbook up-to-date with the rapidly evolving observation…”
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  7. 1687
    “…Subjects covered include primordial nubleosynthesis, baryogenesis, phases transitions, inflation, dark matter, and galaxy formation, relics such as axions, neutrinos and monopoles, and speculations about the Universe at the Planck time. …”
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  8. 1688
    Publicado 2016
    “…This Colloquium is within the astrofundamental physics spirit of the Chalonge School, focalised on recent observational and theoretical progress in the CMB, dark matter, dark energy, the new WDM framework to galaxy formation, and the effective theory of the early universe inflation with predictive power in the context of the LambdaWDM Standard Model of the Universe. …”
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  9. 1689
    por Narlikar, Jayant Vishnu
    Publicado 2002
    “…The physical aspects of cosmology, including primordial nucleosynthesis, the astroparticle physics of inflation, and the current ideas on structure formation are discussed. …”
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  10. 1690
    “…The design target of 400 GeV with a beam intensity of 10/sup 13/ protons/pulse was reached on the 4th of November 1976 within the original budget, allowing for inflation. The technical aspects of the SPS are reviewed, together with operating experience since May 1976. (2 refs).…”
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  11. 1691
    por Moore, Guy
    Publicado 2016
    “…It should be possible to make a clean theoretical prediction relating the dark matter density in axions and the axion mass (under reasonable assumptions about inflation). But the axion's early-Universe dynamics, which establish its density as dark matter, are unexpectedly rich in a way which is only starting to yield to quantitative numerical study.…”
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  12. 1692
    por Melville, Scott
    Publicado 2021
    “…For example, these new bounds place UV constraints on the shapes of cosmological correlators in the CMB which can arise from the effective field theory of single-field inflation.…”
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  13. 1693
    por Carmeli, Moshe
    Publicado 1997
    “…A new law of addition of cosmic times is obtained, and the inflation of the space at the early universe is derived, both from the cosmological transformation. …”
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  14. 1694
    por Veneziano, Gabriele
    Publicado 2000
    “…After discussing how pre-big bang inflation naturally arises from an almost trivial initial state of the Universe, I describe how present or near-future experiments can provide sensitive probes of how the Universe behaved in the pre-bang era. (32 refs).…”
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  15. 1695
    por Felder, G, Tkachev, I
    Publicado 2000
    “…The program is particularly useful for the study of reheating and thermalization after inflation. The program and its full documentation are available on the Web at http://physics.stanford.edu/gfelder/latticeeasy. …”
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  16. 1696
    por Maroto, A L, Peláez, J R
    Publicado 2000
    “…The problem is thus reduced to the standard (Majorana) fermion production after inflation. Comparison between helicity 3/2 and 1/2 production and with the results obtained in the unitary gauge is also presented.…”
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  17. 1697
    Publicado 2004
    “…The Finance Committee is invited to agree to the taking-up of an option with ABB POWER SYSTEMS (SE) for the supply and installation of a set of thyristor controlled reactors for an amount not exceeding 2 301 650 Swiss francs, subject to revision for inflation from the time of tendering, bringing the total amount to 7 745 950 Swiss francs.…”
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  18. 1698
    por García-Bellido, J
    Publicado 2005
    “…I will make special emphasis on the recent developments in observational cosmology, mainly the acceleration of the universe, the precise measurements of the microwave background anisotropies, and the formation of structure like galaxies and clusters of galaxies from tiny primodial fluctuations generated during inflation.…”
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  19. 1699
    Publicado 2005
    “…For the reasons explained in this document, the Finance Committee is invited to approve an amendment to the existing contract with the consortium INTERTEC (DK), CEGELEC (FR) and AMEC SPIE (FR) for the assembly of the LHC cryomagnets for an amount not exceeding 6 586 741 euros (10 284 537 Swiss francs), subject to revision for inflation, bringing the total amount of the contract to an amount of 24 690 595 euros (38 551 895 Swiss francs). …”
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  20. 1700
    “…Second, we consider the possibility that the instability in the Higgs potential leads to the formation of primordial black holes while avoiding vacuum decay during inflation. We show that the nonminimal Higgs coupling to gravity must be as small as allowed by quantum corrections, |ξH|<0.01. …”
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