Mostrando 381 - 400 Resultados de 7,249 Para Buscar '"inflation"', tiempo de consulta: 0.32s Limitar resultados
  1. 381
    por Hotchkiss, Shaun, Sarkar, Subir
    Publicado 2009
    “…Multiple inflation is a model based on N=1 supergravity wherein there are sudden changes in the mass of the inflaton because it couples to 'flat direction' scalar fields which undergo symmetry breaking phase transitions as the universe cools. …”
    Enlace del recurso
    Enlace del recurso
    info:eu-repo/semantics/article
  2. 382
    “…We present constraints on canonical single-field inflation derived from WMAP five year, ACBAR, QUAD, BICEP data combined with the halo power spectrum from SDSS LRG7. …”
    Enlace del recurso
    Enlace del recurso
  3. 383
  4. 384
    “…At quadratic order, we solve the equation of motion at next-to-leading leading order in a generalized slow-roll approximation for a very general theory of single-field inflation. We derive the resulting power spectrum, its tilt and running. …”
    Enlace del recurso
    Enlace del recurso
  5. 385
    “…We discuss the phenomenology of the minimal inflation scenario. We concentrate on two aspects: inflationary trajectories and particle production. …”
    Enlace del recurso
    Enlace del recurso
  6. 386
    “…We discuss and clarify the validity of effective single field theories of inflation obtained by integrating out heavy degrees of freedom in the regime where adiabatic perturbations propagate with a suppressed speed of sound. …”
    Enlace del recurso
    Enlace del recurso
  7. 387
  8. 388
  9. 389
  10. 390
    “…We discuss here how quadratic inflation can be accommodated within supergravity, focussing primarily on the no-scale case. …”
    Enlace del recurso
    Enlace del recurso
  11. 391
  12. 392
  13. 393
    “…We discuss inflaton decays and reheating in no-scale Starobinsky-like models of inflation, calculating the effective equation-of-state parameter, $w$, during the epoch of inflaton decay, the reheating temperature, $T_{\rm reh}$, and the number of inflationary e-folds, $N_*$, comparing analytical approximations with numerical calculations. …”
    Enlace del recurso
    Enlace del recurso
  14. 394
    “…Like the previous SU(5) GUT model, these yield a class of inflation models whose inflation predictions interpolate between those of the quadratic chaotic inflation and Starobinsky-like inflation, while also avoiding tension with proton decay limits. …”
    Enlace del recurso
    Enlace del recurso
  15. 395
  16. 396
    “…Primordial black holes (PBH) have been shown to arise from high peaks in the matter power spectra of multi-field models of inflation. Here we show, with a simple toy model, that it is also possible to generate a peak in the curvature power spectrum of single-field inflation. …”
    Enlace del recurso
    Enlace del recurso
  17. 397
  18. 398
  19. 399
    por Kamada, Kohei
    Publicado 2019
    “…<!--HTML-->Higgs inflation with the nonminimal coupling to gravity \xi H^2 R is the unique model to realize inflation driven by the Standard Model Higgs field in a classically scale invariant way. …”
    Enlace del recurso
  20. 400
    por Yamada, Masatoshi
    Publicado 2019
    “…I will discuss the effective potential for the coupled dilaton-scalaron system at one-loop order and demonstrate that it can be used to successfully realize a stage of slow-roll inflation in the early Universe. Remarkably enough, our predictions for the primordial scalar and tensor power spectra interpolate between those of standard R^2 inflation and linear chaotic inflation. …”
    Enlace del recurso
Herramientas de búsqueda: RSS