http://arxiv.org/abs/1711.09674
The recent Planck data on the power spectrum of temperature anisotropies of the cosmic microwave background marginally support deviations from the $\Lambda$CDM model at several multipoles. With a view towards current and forthcoming observational surveys, we trace these features to other observables like the scalar bispectrum and the tensor power spectrum. A possible detection of such bumps in these channels would increase their statistical significance shedding light on the ultra violet mechanisms responsible for their appearance in the data.
S. Sypsas
Tue, 28 Nov 17
33/82
Comments: 7 pp., 1 figure. Contribution to the proceedings of “STARS2017 – 4th Caribbean Symposium on Cosmology, Gravitation, Nuclear and Astroparticle Physics / SMFNS2017 – 5th International Symposium on Strong Electromagnetic Fields and Neutron Stars”, 7 to 13 of May, 2017, Havana and Varadero, Cuba. Talk also given in PASCOS-17 and COSMO-17