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               <dc:title>Prospects for constraining the shape of non-Gaussianity with the scale-dependent bias</dc:title>
               <dc:creator>Noreña, Jorge</dc:creator>
               <dc:creator>Verde, Licia</dc:creator>
               <dc:creator>Barenboim, Gabriela</dc:creator>
               <dc:creator>Bosch, Cristian</dc:creator>
               <dc:subject>Cosmologia</dc:subject>
               <dc:subject>Astrofísica</dc:subject>
               <dc:subject>Cosmology</dc:subject>
               <dc:subject>Astrophysics</dc:subject>
               <dc:description>We consider whether the non-Gaussian scale-dependent halo bias can be used not only to constrain the local form of non-Gaussianity but also to distinguish among different shapes. In particular, we ask whether it can constrain the behavior of the primordial three-point function in the squeezed limit where one of the momenta is much smaller than the other two. This is potentially interesting since the observation of a three-point function with a squeezed limit that does not go like the local nor equilateral templates would be a signal of non-trivial dynamics during inflation. To this end we use the quasi-single field inflation model of Chen &amp; Wang [1, 2] as a representative two-parameter model, where one parameter governs the amplitude of non-Gaussianity and the other the shape. We also perform a model-independent analysis by parametrizing the scale-dependent bias as a power-law on large scales, where the power is to be constrained from observations. We find that proposed large-scale structure surveys (with characteristics similar to the dark energy task force stage IV surveys) have the potential to distinguish among the squeezed limit behavior of different bispectrum shapes for a wide range of fiducial model parameters. Thus the halo bias can help discriminate between different models of inflation.</dc:description>
               <dc:date>2019-01-22T13:47:49Z</dc:date>
               <dc:date>2019-01-22T13:47:49Z</dc:date>
               <dc:date>2012-08</dc:date>
               <dc:date>2019-01-22T13:47:50Z</dc:date>
               <dc:type>info:eu-repo/semantics/article</dc:type>
               <dc:type>info:eu-repo/semantics/acceptedVersion</dc:type>
               <dc:relation>Versió postprint del document publicat a: https://doi.org/10.1088/1475-7516/2012/08/019</dc:relation>
               <dc:relation>Journal of Cosmology and Astroparticle Physics, 2012, vol. 2012, num. 019</dc:relation>
               <dc:relation>https://doi.org/10.1088/1475-7516/2012/08/019</dc:relation>
               <dc:relation>info:eu-repo/grantAgreement/EC/FP7/240117/EU//PHYS.LSS</dc:relation>
               <dc:rights>(c) IOP Publishing and Sissa Medialab, 2012</dc:rights>
               <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
               <dc:publisher>Institute of Physics (IOP)</dc:publisher>
               <dc:source>Articles publicats en revistes (Institut de Ciències del Cosmos (ICCUB))</dc:source>
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