Large tensor-to-scalar ratio and running of the scalar spectral index with instep inflation

If a sizeable tensor-to-scalar ratio ~ 0.1 turns out to be detected and a negative running of the scalar spectral index ~ 10 super(-2) is significantly required by the data, the vast majority of single field models of inflation will be ruled out. We show that a flat tree-level effective potential, l...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Physical review. D, Particles, fields, gravitation, and cosmology Particles, fields, gravitation, and cosmology, 2015-02, Vol.91 (4), Article 043502
Hauptverfasser: Ballesteros, Guillermo, Casas, J. Alberto
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue 4
container_start_page
container_title Physical review. D, Particles, fields, gravitation, and cosmology
container_volume 91
creator Ballesteros, Guillermo
Casas, J. Alberto
description If a sizeable tensor-to-scalar ratio ~ 0.1 turns out to be detected and a negative running of the scalar spectral index ~ 10 super(-2) is significantly required by the data, the vast majority of single field models of inflation will be ruled out. We show that a flat tree-level effective potential, lifted by radiative corrections and by the imprints of a high energy scale (in the form of nonrenormalizable operators) can explain those features and produce enough inflation in the slow-roll regime.
doi_str_mv 10.1103/PhysRevD.91.043502
format Article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1709768955</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1709768955</sourcerecordid><originalsourceid>FETCH-LOGICAL-c324t-ce3b04446aebbdba1111cc7d320df6243adf307732d2ed4e4396f1fafc3d2da03</originalsourceid><addsrcrecordid>eNo1kMtOwzAURC0EEqXwA6y8ZJPiV-J6icpTigRCsGJhOfZ1G5Q6wXaB_j2pWmYzI925szgIXVIyo5Tw65fVNr3C9-1M0RkRvCTsCE1oWZKC8Wp-fMhSqfkpOkvpkxDOKikn6KM2cQk4Q0h9LHJfJGs6E3E0ue2xCQ7HTQhtWOLe47wCfLinAWyOpsNtcPCLf9q8GmPKMIzmu913OEcn3nQJLg4-Re_3d2-Lx6J-fnha3NSF5UzkwgJviBCiMtA0rjF0lLXScUacr5jgxnlOpOTMMXACBFeVp954yx1zhvAputrvDrH_2kDKet0mC11nAvSbpKkkSlZzVZZjle2rNvYpRfB6iO3axK2mRO9I6n-SWlG9J8n_AFKsapw</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1709768955</pqid></control><display><type>article</type><title>Large tensor-to-scalar ratio and running of the scalar spectral index with instep inflation</title><source>PROLA</source><creator>Ballesteros, Guillermo ; Casas, J. Alberto</creator><creatorcontrib>Ballesteros, Guillermo ; Casas, J. Alberto</creatorcontrib><description>If a sizeable tensor-to-scalar ratio ~ 0.1 turns out to be detected and a negative running of the scalar spectral index ~ 10 super(-2) is significantly required by the data, the vast majority of single field models of inflation will be ruled out. We show that a flat tree-level effective potential, lifted by radiative corrections and by the imprints of a high energy scale (in the form of nonrenormalizable operators) can explain those features and produce enough inflation in the slow-roll regime.</description><identifier>ISSN: 1550-7998</identifier><identifier>EISSN: 1550-2368</identifier><identifier>DOI: 10.1103/PhysRevD.91.043502</identifier><language>eng</language><subject>Cosmology ; Flats ; Gravitation ; Inflation ; Operators ; Running ; Scalars ; Spectra</subject><ispartof>Physical review. D, Particles, fields, gravitation, and cosmology, 2015-02, Vol.91 (4), Article 043502</ispartof><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c324t-ce3b04446aebbdba1111cc7d320df6243adf307732d2ed4e4396f1fafc3d2da03</citedby><cites>FETCH-LOGICAL-c324t-ce3b04446aebbdba1111cc7d320df6243adf307732d2ed4e4396f1fafc3d2da03</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,2876,2877,27924,27925</link.rule.ids></links><search><creatorcontrib>Ballesteros, Guillermo</creatorcontrib><creatorcontrib>Casas, J. Alberto</creatorcontrib><title>Large tensor-to-scalar ratio and running of the scalar spectral index with instep inflation</title><title>Physical review. D, Particles, fields, gravitation, and cosmology</title><description>If a sizeable tensor-to-scalar ratio ~ 0.1 turns out to be detected and a negative running of the scalar spectral index ~ 10 super(-2) is significantly required by the data, the vast majority of single field models of inflation will be ruled out. We show that a flat tree-level effective potential, lifted by radiative corrections and by the imprints of a high energy scale (in the form of nonrenormalizable operators) can explain those features and produce enough inflation in the slow-roll regime.</description><subject>Cosmology</subject><subject>Flats</subject><subject>Gravitation</subject><subject>Inflation</subject><subject>Operators</subject><subject>Running</subject><subject>Scalars</subject><subject>Spectra</subject><issn>1550-7998</issn><issn>1550-2368</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNo1kMtOwzAURC0EEqXwA6y8ZJPiV-J6icpTigRCsGJhOfZ1G5Q6wXaB_j2pWmYzI925szgIXVIyo5Tw65fVNr3C9-1M0RkRvCTsCE1oWZKC8Wp-fMhSqfkpOkvpkxDOKikn6KM2cQk4Q0h9LHJfJGs6E3E0ue2xCQ7HTQhtWOLe47wCfLinAWyOpsNtcPCLf9q8GmPKMIzmu913OEcn3nQJLg4-Re_3d2-Lx6J-fnha3NSF5UzkwgJviBCiMtA0rjF0lLXScUacr5jgxnlOpOTMMXACBFeVp954yx1zhvAputrvDrH_2kDKet0mC11nAvSbpKkkSlZzVZZjle2rNvYpRfB6iO3axK2mRO9I6n-SWlG9J8n_AFKsapw</recordid><startdate>20150203</startdate><enddate>20150203</enddate><creator>Ballesteros, Guillermo</creator><creator>Casas, J. Alberto</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20150203</creationdate><title>Large tensor-to-scalar ratio and running of the scalar spectral index with instep inflation</title><author>Ballesteros, Guillermo ; Casas, J. Alberto</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c324t-ce3b04446aebbdba1111cc7d320df6243adf307732d2ed4e4396f1fafc3d2da03</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Cosmology</topic><topic>Flats</topic><topic>Gravitation</topic><topic>Inflation</topic><topic>Operators</topic><topic>Running</topic><topic>Scalars</topic><topic>Spectra</topic><toplevel>online_resources</toplevel><creatorcontrib>Ballesteros, Guillermo</creatorcontrib><creatorcontrib>Casas, J. Alberto</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Physical review. D, Particles, fields, gravitation, and cosmology</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Ballesteros, Guillermo</au><au>Casas, J. Alberto</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Large tensor-to-scalar ratio and running of the scalar spectral index with instep inflation</atitle><jtitle>Physical review. D, Particles, fields, gravitation, and cosmology</jtitle><date>2015-02-03</date><risdate>2015</risdate><volume>91</volume><issue>4</issue><artnum>043502</artnum><issn>1550-7998</issn><eissn>1550-2368</eissn><abstract>If a sizeable tensor-to-scalar ratio ~ 0.1 turns out to be detected and a negative running of the scalar spectral index ~ 10 super(-2) is significantly required by the data, the vast majority of single field models of inflation will be ruled out. We show that a flat tree-level effective potential, lifted by radiative corrections and by the imprints of a high energy scale (in the form of nonrenormalizable operators) can explain those features and produce enough inflation in the slow-roll regime.</abstract><doi>10.1103/PhysRevD.91.043502</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 1550-7998
ispartof Physical review. D, Particles, fields, gravitation, and cosmology, 2015-02, Vol.91 (4), Article 043502
issn 1550-7998
1550-2368
language eng
recordid cdi_proquest_miscellaneous_1709768955
source PROLA
subjects Cosmology
Flats
Gravitation
Inflation
Operators
Running
Scalars
Spectra
title Large tensor-to-scalar ratio and running of the scalar spectral index with instep inflation
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-25T10%3A02%3A48IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Large%20tensor-to-scalar%20ratio%20and%20running%20of%20the%20scalar%20spectral%20index%20with%20instep%20inflation&rft.jtitle=Physical%20review.%20D,%20Particles,%20fields,%20gravitation,%20and%20cosmology&rft.au=Ballesteros,%20Guillermo&rft.date=2015-02-03&rft.volume=91&rft.issue=4&rft.artnum=043502&rft.issn=1550-7998&rft.eissn=1550-2368&rft_id=info:doi/10.1103/PhysRevD.91.043502&rft_dat=%3Cproquest_cross%3E1709768955%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1709768955&rft_id=info:pmid/&rfr_iscdi=true