Imperial College London

Carlo R. Contaldi

Faculty of Natural SciencesDepartment of Physics

Professor of Theoretical Physics
 
 
 
//

Contact

 

+44 (0)20 7594 1527c.contaldi

 
 
//

Location

 

505Huxley BuildingSouth Kensington Campus

//

Summary

 

Publications

Citation

BibTex format

@article{Contaldi:2014:07/014,
author = {Contaldi, CR and Peloso, M and Sorbo, L},
doi = {07/014},
journal = {Journal of Cosmology and Astroparticle Physics},
pages = {1--14},
title = {Suppressing the impact of a high tensor-to-scalar ratio on the temperature anisotropies},
url = {http://dx.doi.org/10.1088/1475-7516/2014/07/014},
volume = {2014},
year = {2014}
}

RIS format (EndNote, RefMan)

TY  - JOUR
AB - The BICEP2 collaboration has reported a strong B mode signal in the CMB polarization, which is well fit by a tensor-to-scalar ratio of r sime 0.2. This is greater than the upper limit r < 0.11 obtained from the temperature anisotropies under the assumption of a constant scalar spectral index ns. This discrepancy can be reduced once the statistical error and the contamination from polarized dust are accounted for. If however a large value for r will be confirmed, it will need to be reconciled with the temperature anisotropies data. The most advocated explanation involves a variation of ns with scales (denoted as running) that has a magnitude significantly greater than the generic slow roll predictions. We instead study the possibility that the large scale temperature anisotropies are not enhanced because of a suppression of the scalar power at large scales. Such a situation can be achieved for instance by a sudden change of the speed of the inflaton (by about 14%), and we show that it fits the temperature anisotropies and polarization data considerably better than a constant running (its χ2 improves by ~ 7.5 over that of the constant running, at the cost of one more parameter). We also consider the possibility that the large scale temperature fluctuations are suppressed by an anti-correlation between tensor and scalar modes. Unfortunately, while such effect does affect the temperature fluctuations at large scales, it does not affect the temperature power spectrum and cannot, therefore, help in reconciling a large value of r with the limits from temperature fluctuations.
AU - Contaldi,CR
AU - Peloso,M
AU - Sorbo,L
DO - 07/014
EP - 14
PY - 2014///
SN - 1475-7516
SP - 1
TI - Suppressing the impact of a high tensor-to-scalar ratio on the temperature anisotropies
T2 - Journal of Cosmology and Astroparticle Physics
UR - http://dx.doi.org/10.1088/1475-7516/2014/07/014
UR - https://iopscience.iop.org/article/10.1088/1475-7516/2014/07/014
UR - http://hdl.handle.net/10044/1/73811
VL - 2014
ER -