.png){kind=icon}
Return
K-bounce
.png){kind=icon}
PRE
AI
DOI：10.1088/1475-7516/2007/09/001.png)
.png){kind=icon}
Original request for help.png){kind=icon}
Share.png){kind=icon}
Save
Abstract
En 中文
By requiring that a bounce is non-singular and that perturbations are well behaved at all times, we narrow the scope of possible models with one degree of freedom that can describe a bounce in the absence of spatial curvature. We compute the general properties of the transfer matrix of perturbations through the bounce, and show that spectral distortions of the Bardeen potential F are generically produced only for small wavelengths, although the spectrum of long wavelength curvature perturbations produced in a contracting phase gets propagated unaffected through such a bounce.
Keywords:
cosmological perturbation theory
inflation
physics of the early universe
AI Summary
Key information extracted from the uploaded paper, including a brief overview, abstract, background, key highlights, visual analysis, and future outlook.
Journal
IF:
5.9
Papers:
1.3W
Citations:
4.7W
Organization
No organization information available
Cited Papers
.png){kind=icon}
ShareSaveShareSaveEffect of indomethacin on glomerular permselectivity and hemodynamics in nephrotoxic serum nephritis
OAAI
OAAIShareSaveShareSaveShareSaveShareSave
ShareSaveShareSave
View more