Imperial College London

Carlo R. Contaldi

Faculty of Natural SciencesDepartment of Physics

Professor of Theoretical Physics
 
 
 
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Contact

 

+44 (0)20 7594 1527c.contaldi

 
 
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Location

 

505Huxley BuildingSouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@article{Horner:2014,
author = {Horner, JS and Contaldi, CR},
title = {BICEP's bispectrum},
url = {http://arxiv.org/abs/1407.6948v1},
year = {2014}
}

RIS format (EndNote, RefMan)

TY  - JOUR
AB - The simplest interpretation of the Bicep2 result is that the scalarprimordial power spectrum is slightly suppressed at large scales. These modelsresult in a large tensor-to-scalar ratio $r$. In this work we show that thetype of inflationary trajectory favoured by Bicep2 also leads to a largernon-Gaussian signal at large scales, roughly an order of magnitude larger thana standard slow-roll trajectory.
AU - Horner,JS
AU - Contaldi,CR
PY - 2014///
TI - BICEP's bispectrum
UR - http://arxiv.org/abs/1407.6948v1
ER -