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A Note on Inflation and the Swampland
We provide some comments about the constraints on the inflationary models inferred from the two Swampland criteria which have been recently proposed. In particular we argue that, in the absence of any knowledge about the origin of the adiabatic curvature perturbations, within the slow‐roll single fi...
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Published in: | Fortschritte der Physik 2018-10, Vol.66 (10), p.n/a |
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description | We provide some comments about the constraints on the inflationary models inferred from the two Swampland criteria which have been recently proposed. In particular we argue that, in the absence of any knowledge about the origin of the adiabatic curvature perturbations, within the slow‐roll single field models of inflation there is no tension between the swampland criteria and the current lower bound on the tensor‐to‐scalar ratio.
The authors provide some comments about the constraints on the inflationary models inferred from the two Swampland criteria which have been recently proposed. In particular they argue that, in the absence of any knowledge about the origin of the adiabatic curvature perturbations, within the slow‐roll single field models of inflation there is no tension between the swampland criteria and the current lower bound on the tensor‐to‐scalar ratio. |
doi_str_mv | 10.1002/prop.201800052 |
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The authors provide some comments about the constraints on the inflationary models inferred from the two Swampland criteria which have been recently proposed. In particular they argue that, in the absence of any knowledge about the origin of the adiabatic curvature perturbations, within the slow‐roll single field models of inflation there is no tension between the swampland criteria and the current lower bound on the tensor‐to‐scalar ratio.</description><subject>Constraint modelling</subject><subject>Curvature</subject><subject>Inflation</subject><subject>Lower bounds</subject><subject>Swampland</subject><issn>0015-8208</issn><issn>1521-3978</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNqFkM1Lw0AQxRdRMFavngPiMXFms5vsHkvRWii2-HFedtMNpqRJ3E0p_e_dEtGjp5mB35vHe4TcIqQIQB961_UpBRQAwOkZiZBTTDJZiHMSASBPBAVxSa683waEosSI3E_jl26wcdfGi7Zq9FCHTbebePi08dtB7_omXNfkotKNtzc_c0I-nh7fZ8_JcjVfzKbLpGQ0o4nmhpWUAhNFFnxBI0qGTFa82GBOq1KaXBbGGmMKCULkupQgCyszUQLjJpuQu_FvyPK1t35Q227v2mCpKCIXLAcGgUpHqnSd985Wqnf1TrujQlCnKtSpCvVbRRDIUXCoG3v8h1br19X6T_sNdZVfXQ</recordid><startdate>201810</startdate><enddate>201810</enddate><creator>Kehagias, A.</creator><creator>Riotto, A.</creator><general>Wiley Subscription Services, Inc</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>201810</creationdate><title>A Note on Inflation and the Swampland</title><author>Kehagias, A. ; Riotto, A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c4232-a5b4c22048733970a1194149f57d162fc9b697bebbb790886ac9097e938c045b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>Constraint modelling</topic><topic>Curvature</topic><topic>Inflation</topic><topic>Lower bounds</topic><topic>Swampland</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Kehagias, A.</creatorcontrib><creatorcontrib>Riotto, A.</creatorcontrib><collection>CrossRef</collection><jtitle>Fortschritte der Physik</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kehagias, A.</au><au>Riotto, A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A Note on Inflation and the Swampland</atitle><jtitle>Fortschritte der Physik</jtitle><date>2018-10</date><risdate>2018</risdate><volume>66</volume><issue>10</issue><epage>n/a</epage><issn>0015-8208</issn><eissn>1521-3978</eissn><abstract>We provide some comments about the constraints on the inflationary models inferred from the two Swampland criteria which have been recently proposed. In particular we argue that, in the absence of any knowledge about the origin of the adiabatic curvature perturbations, within the slow‐roll single field models of inflation there is no tension between the swampland criteria and the current lower bound on the tensor‐to‐scalar ratio.
The authors provide some comments about the constraints on the inflationary models inferred from the two Swampland criteria which have been recently proposed. In particular they argue that, in the absence of any knowledge about the origin of the adiabatic curvature perturbations, within the slow‐roll single field models of inflation there is no tension between the swampland criteria and the current lower bound on the tensor‐to‐scalar ratio.</abstract><cop>Weinheim</cop><pub>Wiley Subscription Services, Inc</pub><doi>10.1002/prop.201800052</doi><tpages>4</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Constraint modelling Curvature Inflation Lower bounds Swampland |
title | A Note on Inflation and the Swampland |
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