1 / 1

Beyond Vanilla

Beyond Vanilla CMB and LSS will measure standard cosmological parameters like Wmh², Wbh², n, As, and h to a percent level in the coming years. While this progress is significant, numerous questions remain about dark energy, dark matter, primordial spectra, non-Gaussianity, isocurvature admixtures, neutrino masses, gravitational waves from the early universe, and particle decays. Addressing these concerns is crucial for advancing our understanding of the cosmos and is a primary focus of future research initiatives and discussions from Eisenstein's recent talk at ON.

reeves
Télécharger la présentation

Beyond Vanilla

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Beyond Vanilla • CMB+LSS will measure the standard cosmological parameters (Wmh2, Wbh2, n, AS, h) to percent level in the next few years. • But there's lots more to do, e.g., • Dark Energy: cosmological constant or not? If not, what? • Dark Matter, deviations from CDM • Primordial spectrum • Primordial non-Gaussianity • Isocurvature admixtures • Neutrino Masses • Gravitational waves from the early Universe. • Particle decays • Galaxy physics From Eisenstein’s talk at ON

More Related