CWRU PAT Coffee Agenda

Tuesdays 10:30 - 11:30 | Fridays 11:30 - 12:30

+1 Gravitational waves, CMB polarization, and the Hubble tension.

gds6 +1

+1 Shift symmetries, soft limits, and the double copy beyond leading order.

lxj154 +1

Showing votes from 2019-08-20 11:30 to 2019-08-23 12:30 | Next meeting is Tuesday Aug 5th, 10:30 am.

users

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astro-ph.CO

  • Using SPTpol, Planck 2015, and non-CMB data to constrain tilted spatially-flat and untilted non-flat $\Lambda$CDM, XCDM, and $\phi$CDM dark energy inflation cosmologies.- [PDF] - [Article]

    Chan-Gyung Park, Bharat Ratra
     

    We use six tilted spatially-flat and untilted non-flat dark energy cosmological models in analyses of South Pole Telescope polarization (SPTpol) cosmic microwave background (CMB) data, alone and in combination with Planck 2015 CMB data and non-CMB data. All best-fit cosmological models have CMB anisotropy power spectra that do not provide good fits to the SPTpol data, differing at the 2 to 3$\sigma$ level. In all models, there is no significant difference between the model that best fits the SPTpol data and the one that best fits the Planck CMB and non-CMB data. When the smaller angular scale SPTpol data are used jointly with either the Planck data alone or with the Planck CMB and the non-CMB data to constrain untilted non-flat models, spatially-closed models remain favored over their corresponding flat limits. When used in conjunction with Planck data, non-CMB data (baryon acoustic oscillation measurements in particular, from six experiments) have significantly more constraining power than the SPTpol data.

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