Mostrando 2,141 - 2,160 Resultados de 7,249 Para Buscar '"inflation"', tiempo de consulta: 0.16s Limitar resultados
  1. 2141
  2. 2142
    “…OBJECTIVE: To study if protocolized monitoring of endotracheal tube (ETT) cuff pressure every 6 hours is better than adjusting endotracheal tube cuff inflation by the only bedside clinical assessment. …”
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  3. 2143
    “…Participants will receive either RIC (four 5-min cycles of inflation [20 mmHg above systolic blood pressure] and deflation of an automated blood pressure cuff placed on the upper arm) or sham control (similar protocol but with low-pressure inflation of 20 mmHg and deflation) within 1 h of thrombolysis and applied daily for the next 2 days. …”
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  4. 2144
    “…The compounded annual growth rates of different medication costs were compared with the annual inflation rate and the consumer price index for prescription drugs. …”
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  5. 2145
    “…Fifth, we measured the external diameter of both lumens and the tubules for tracheal and bronchial cuff inflation. Finally, we measured various cross-sectional areas including the tracheal lumen, bronchial lumen, and tubules for cuff inflation. …”
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  6. 2146
    “…OBJECTIVES: The aim of this study was to compare the effects of a sustained inflation alveolar recruiting maneuver (ARM) followed by 5 cmH(2)O of PEEP and a stepwise ARM, in dogs undergoing laparoscopic surgery. …”
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  7. 2147
    “…Second, the targeted segmental arteries were ligated, and the intersegmental plane was determined by the inflation-deflation technique. The waiting time for the appearance of the inflation-deflation line was recorded. …”
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  8. 2148
    “…RESULTS: A significant decrease in the mean StO2 from the baseline was observed during tourniquet inflation in the operative legs. The average decrease in the mean StO2 was 58%. …”
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  9. 2149
    “…A crucial role is played by the inflation--induced scalar masses, whereas thermal effects are often irrelevant.…”
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  10. 2150
    por Peter, Patrick, Uzan, Jean-Philippe
    Publicado 2009
    “…Part 2 describes the standard model of cosmology and includes cosmological solutions of Einstein equations, the hot big bang model, cosmological perturbation theory, cosmic microwave background anisotropies, lensing and evidence for dark matter, and inflation. Part 3 describes extensions of this model and opens up current research in the field: scalar-tensor theories, supersymmetry, the cosmological constant problem and acceleration of the universe, topology of the universe, grand unification and baryogenesis, topological defects and phase transitions, string inspired cosmology including branes and the latest developments. …”
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  11. 2151
    “…These effects could be important during inflation, which could lead to detectable effects in upcoming observations.…”
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    info:eu-repo/semantics/article
  12. 2152
    “…We argue that baryonic and dark matter abundances can be explained naturally in these setups where reheating takes place by bubble collisions at the end of the strongly first-order phase transition characterizing conformal symmetry breaking, even if the reheating temperature is below the electroweak scale $\sim 100$ GeV. We also discuss inflation as well as gravity wave smoking gun signatures of this class of models.…”
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  13. 2153
    “…Stability at finite temperature implies an upper bound on the reheat temperature after inflation, which depends critically on the precise values of the Higgs and top masses. …”
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  14. 2154
    “…This new interest is motivated by one of the original ideas that topological defects are inevitable in symmetry breaking by the Kibble (1976) mechanism and the introduction of new ideas such as brane-cosmology/inflation and the realization that cosmic strings may be the only acceptable such defect. …”
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  15. 2155
    “…We also review some issues about the causality of nonlocal theories, and we point out that these nonlocal models can be modified so to nicely interpolate between Starobinski inflation in the primordial universe and accelerated expansion in the recent epoch.…”
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  16. 2156
    por Perlov, Delia, Vilenkin, Alex
    Publicado 2017
    “…It is the subject of the theory of cosmic inflation, which was developed in the last few decades and has led to a radically new global view of the universe. …”
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  17. 2157
    “…Three complementary issues in cosmology are examined: observable predictions of inflation in the early universe, effects of dark energy/modified gravity in the large-scale structure of the universe, and neutrinos in cosmology and large-scale structures. …”
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  18. 2158
    por Schober, Jennifer
    Publicado 2021
    “…I will address the possible origin of magnetic fields in the very early Universe, during inflation and the cosmological phase transitions, as well as their pre-recombination evolution in magnetohydrodynamical (MHD) turbulence. …”
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  19. 2159
    “…We combine NANOGrav 15-years and EPTA-DR2new data sets and confront them against backgrounds from supermassive black hole binaries (SMBHBs) and cosmological signals from inflation, cosmic (super)strings, first-order phase transitions, Gaussian and non-Gaussian large scalar fluctuations, and audible axions. …”
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  20. 2160
    “…In this article, we discuss the current status of metastable cosmic strings, with a focus on possible GUT embeddings and connections to inflation, neutrinos, and gravitational waves (GWs). …”
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