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  1. 4761
    “…We find that the predictions for $n_s$ and $r$ for $\alpha$-attractor cosmological models, compatible with the current cosmological data, are preserved in the presence of the neutrino sector.…”
    Enlace del recurso
    Enlace del recurso
    Sneutrino Inflation with $\alpha$-attractors
  2. 4762
    por Kirilova, D.P.
    Publicado 2001
    “…The production of helium-4 during the cosmological nucleosynthesis in the presence of active--sterile neutrino oscillations, efficient after decoupling of electron neutrino, is analyzed. …”
    Enlace del recurso
    Enlace del recurso
    Overproduction of primordial helium-4 in the presence of neutrino oscillations
  3. 4763
    por Giovannini, Massimo
    Publicado 2008
    “…In this plausible extension of the current cosmological paradigm, hereby dubbed Tensor-$\Lambda$CDM (i.e. …”
    Enlace del recurso
    Enlace del recurso
    Stochastic backgrounds of relic gravitons, T$\Lambda$CDM paradigm and the stiff ages
  4. 4764
    por Bellini, Emilio, Jimenez, Raul
    Publicado 2013
    “…The effective equation of state is indistinguishable from that of a cosmological constant w = -1 and the data constraint it to have no temporal variations of more than at the few % level. …”
    Enlace del recurso
    Enlace del recurso
    The parameter space of Cubic Galileon models for cosmic acceleration
  5. 4765
    “…Including the metric fluctuations of a realistic cosmological geometry we reconsider an earlier suggestion that measuring the relative time-of-flight of ultra-relativistic particles can provide interesting constraints on fundamental cosmological and/or particle parameters. …”
    Enlace del recurso
    Enlace del recurso
    Time of flight of ultra-relativistic particles in a realistic Universe: a viable tool for fundamental physics?
  6. 4766
    “…Cosmological parameter estimation from forthcoming experiments promise to reach much greater precision than current constraints. …”
    Enlace del recurso
    Enlace del recurso
    Beware of commonly used approximations: Part II. Estimating systematic biases in the best-fit parameters
  7. 4767
    “…We used IllustrisTNG cosmological simulations to study the effect of magnetized galactic wind bubbles on the secondary γ-ray flux.Results. …”
    Enlace del recurso
    Enlace del recurso
    Account of the baryonic feedback effect in γ-ray measurements of intergalactic magnetic fields
  8. 4768
    por Overbye, D
    Publicado 2002
    “…Article describing the cosmological theory of multiple universes (2 page).…”
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    A new view of our universe: only one of many
  9. 4769
    por Angelantonj, Carlo
    Publicado 1999
    “…Generically, these vacua generate a non-vanishing cosmological constant. However, one can construct particular kinds of Scherk-Schwarz compactifications with vanishing cosmological constant, at least for low orders, based on asymmetric orbifolds. …”
    Enlace del recurso
    Enlace del recurso
    Non-Supersymmetric Open String Vacua
  10. 4770
    “…Our model also allows for the anthropic solution of the cosmological constant problem.…”
    Enlace del recurso
    Enlace del recurso
    Massive graviton as a testable cold dark matter candidate
  11. 4771
    por Jones, A. W., Lasenby, A. N.
    Publicado 1998
    “…New predictions for cosmological defect theories and an overview of the inflationary theory are discussed. …”
    Enlace del recurso
    Enlace del recurso
    Enlace del recurso
    Online Artículo Texto
    The Cosmic Microwave Background
  12. 4772
    por Laine, M.
    Publicado 1999
    “…We review the motivation for, lattice results on, and some implications of, external magnetic fields present at the time of the cosmological electroweak phase transition.…”
    Enlace del recurso
    Magnetic fields and the EW phase transition
  13. 4773
    “…These equations allow to follow the time evolution of the cosmic microwave background anisotropies at all angular scales from the early epoch, when the cosmological perturbations were generated, to the present, through the recombination era. …”
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    Cosmic Microwave Background Anisotropies up to Second Order
  14. 4774
    “…The recent measurements of the cosmological parameter H0 from the direct local observations and the inferred value from the cosmic microwave background show approximately 4σ discrepancy. …”
    Enlace del recurso
    Enlace del recurso
    Light gravitino dark matter: LHC searches and the Hubble tension
  15. 4775
    “…The solutions simplify considerably in the presence of a negative cosmological constant, particularly for the limiting cases of a very large cosmological constant or very small gauge field. …”
    Enlace del recurso
    Enlace del recurso
    Infinitely Coloured Black Holes
  16. 4776
    por Rostworowski, Andrzej
    Publicado 2016
    “…On the other hand the negative cosmological constant allows for the existence of stable, time-periodic, asymptotically AdS solutions of Einstein equations [arXiv:1303.3186].…”
    Enlace del recurso
    Current status of AdS instability
  17. 4777
    “…We consider spherically symmetric higher-dimensional solutions of Einstein's equations with a bulk cosmological constant and n transverse dimensions. In contrast to the case of one or two extra dimensions we find no solutions that localize gravity when $n\geq 3$, for strictly local topological defects. …”
    Enlace del recurso
    Enlace del recurso
    Living Inside a Hedgehog: Higher-dimensional Solutions that Localize Gravity
  18. 4778
    “…The solutions are characterized by a non-trivial warping along the extra dimension, even in the case of a vanishing bulk cosmological constant, and lead to a variety of inflationary, time-dependent solutions of the 3D scale factor on the brane. …”
    Enlace del recurso
    Enlace del recurso
    Stable, Time-Dependent, Exact Solutions for Brane Models with a Bulk Scalar Field
  19. 4779
    por Vannerom, David
    Publicado 2019
    “…Numerous cosmological observations support the existence of a large amount of non-radiating matter in the universe which cannot originate from any Standard Model (SM) particle. …”
    Enlace del recurso
    Enlace del recurso
    Dark Matter searches with CMS
  20. 4780
    “…Within the low scale resonant leptogenesis scenario, the cosmological CP asymmetry may arise by radiative corrections through the charged lepton Yukawa couplings. …”
    Enlace del recurso
    Enlace del recurso
    Texture Zero Neutrino Models and Their Connection with Resonant Leptogenesis
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