<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-04-14T02:40:41Z</responseDate><request verb="GetRecord" identifier="oai:www.recercat.cat:2445/127526" metadataPrefix="oai_dc">https://recercat.cat/oai/request</request><GetRecord><record><header><identifier>oai:recercat.cat:2445/127526</identifier><datestamp>2025-12-05T16:10:18Z</datestamp><setSpec>com_2072_1057</setSpec><setSpec>col_2072_478904</setSpec><setSpec>col_2072_478917</setSpec></header><metadata><oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
   <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:identifier>1475-7516</dc:identifier>
   <dc:identifier>https://hdl.handle.net/2445/127526</dc:identifier>
   <dc:identifier>619880</dc:identifier>
   <dc:language>eng</dc:language>
   <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:format>12 p.</dc:format>
   <dc:format>application/pdf</dc:format>
   <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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