Loading…

Axionic Festina Lente

The swampland conjecture known as Festina Lente (FL) imposes a lower bound on the mass of all charged particles in a quasi-de Sitter space. In this paper, we propose the aFL (axionic Festina Lente) bound, an extension of FL to axion-like particles arising from type II string theory. We find that the...

Full description

Saved in:
Bibliographic Details
Published in:arXiv.org 2023-01
Main Authors: Guidetti, Veronica, Righi, Nicole, Venken, Gerben, Westphal, Alexander
Format: Article
Language:English
Subjects:
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by
cites
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
creator Guidetti, Veronica
Righi, Nicole
Venken, Gerben
Westphal, Alexander
description The swampland conjecture known as Festina Lente (FL) imposes a lower bound on the mass of all charged particles in a quasi-de Sitter space. In this paper, we propose the aFL (axionic Festina Lente) bound, an extension of FL to axion-like particles arising from type II string theory. We find that the product of the instanton action and the axion decay constant is bounded from below by the vacuum energy. This is achieved indirectly, using dimensional reduction on Calabi-Yau threefolds, and translating the FL result for dipoles into a purely geometric bound. We discuss axionic black holes evolution, and aFL constraints on Euclidean wormholes, showing that the gravitational arguments leading to the FL bound for U\((1)\) charged particles cannot be directly applied to axions. Moreover, we discuss phenomenological implications of the aFL bound, including constraints on string inflation models and the axion-photon coupling via kinetic mixing.
doi_str_mv 10.48550/arxiv.2206.03494
format article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2674531023</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2674531023</sourcerecordid><originalsourceid>FETCH-LOGICAL-a954-f9e3a870f64b8c379d38e993af7e613e54f87326bb9ad5bad914440482f98da83</originalsourceid><addsrcrecordid>eNotzk9rwkAQhvGlUKhYjz30JvScODsz-2eOIlULgV68y8TsQqQkbaLFj99APb235_0Z82qh5OgcrHS4tb8lIvgSiIUfzAyJbBEZ8cksxvEMAOgDOkcz87K-tX3XnpbbNF7aTpdV6i7p2Txm_RrT4r5zc9i-Hzb7ovrcfWzWVaHiuMiSSGOA7LmOJwrSUEwipDkkbyk5zjEQ-roWbVytjVhmBo6YJTYaaW7e_rPfQ_9znQDHc38duunxOAHZkYWJ_geyeTo0</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2674531023</pqid></control><display><type>article</type><title>Axionic Festina Lente</title><source>Publicly Available Content Database</source><creator>Guidetti, Veronica ; Righi, Nicole ; Venken, Gerben ; Westphal, Alexander</creator><creatorcontrib>Guidetti, Veronica ; Righi, Nicole ; Venken, Gerben ; Westphal, Alexander</creatorcontrib><description>The swampland conjecture known as Festina Lente (FL) imposes a lower bound on the mass of all charged particles in a quasi-de Sitter space. In this paper, we propose the aFL (axionic Festina Lente) bound, an extension of FL to axion-like particles arising from type II string theory. We find that the product of the instanton action and the axion decay constant is bounded from below by the vacuum energy. This is achieved indirectly, using dimensional reduction on Calabi-Yau threefolds, and translating the FL result for dipoles into a purely geometric bound. We discuss axionic black holes evolution, and aFL constraints on Euclidean wormholes, showing that the gravitational arguments leading to the FL bound for U\((1)\) charged particles cannot be directly applied to axions. Moreover, we discuss phenomenological implications of the aFL bound, including constraints on string inflation models and the axion-photon coupling via kinetic mixing.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2206.03494</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Charged particles ; Constraint modelling ; Decay rate ; Dipoles ; Instantons ; Lower bounds ; String theory</subject><ispartof>arXiv.org, 2023-01</ispartof><rights>2023. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2674531023?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>780,784,25753,27925,37012,44590</link.rule.ids></links><search><creatorcontrib>Guidetti, Veronica</creatorcontrib><creatorcontrib>Righi, Nicole</creatorcontrib><creatorcontrib>Venken, Gerben</creatorcontrib><creatorcontrib>Westphal, Alexander</creatorcontrib><title>Axionic Festina Lente</title><title>arXiv.org</title><description>The swampland conjecture known as Festina Lente (FL) imposes a lower bound on the mass of all charged particles in a quasi-de Sitter space. In this paper, we propose the aFL (axionic Festina Lente) bound, an extension of FL to axion-like particles arising from type II string theory. We find that the product of the instanton action and the axion decay constant is bounded from below by the vacuum energy. This is achieved indirectly, using dimensional reduction on Calabi-Yau threefolds, and translating the FL result for dipoles into a purely geometric bound. We discuss axionic black holes evolution, and aFL constraints on Euclidean wormholes, showing that the gravitational arguments leading to the FL bound for U\((1)\) charged particles cannot be directly applied to axions. Moreover, we discuss phenomenological implications of the aFL bound, including constraints on string inflation models and the axion-photon coupling via kinetic mixing.</description><subject>Charged particles</subject><subject>Constraint modelling</subject><subject>Decay rate</subject><subject>Dipoles</subject><subject>Instantons</subject><subject>Lower bounds</subject><subject>String theory</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNotzk9rwkAQhvGlUKhYjz30JvScODsz-2eOIlULgV68y8TsQqQkbaLFj99APb235_0Z82qh5OgcrHS4tb8lIvgSiIUfzAyJbBEZ8cksxvEMAOgDOkcz87K-tX3XnpbbNF7aTpdV6i7p2Txm_RrT4r5zc9i-Hzb7ovrcfWzWVaHiuMiSSGOA7LmOJwrSUEwipDkkbyk5zjEQ-roWbVytjVhmBo6YJTYaaW7e_rPfQ_9znQDHc38duunxOAHZkYWJ_geyeTo0</recordid><startdate>20230123</startdate><enddate>20230123</enddate><creator>Guidetti, Veronica</creator><creator>Righi, Nicole</creator><creator>Venken, Gerben</creator><creator>Westphal, Alexander</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20230123</creationdate><title>Axionic Festina Lente</title><author>Guidetti, Veronica ; Righi, Nicole ; Venken, Gerben ; Westphal, Alexander</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a954-f9e3a870f64b8c379d38e993af7e613e54f87326bb9ad5bad914440482f98da83</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Charged particles</topic><topic>Constraint modelling</topic><topic>Decay rate</topic><topic>Dipoles</topic><topic>Instantons</topic><topic>Lower bounds</topic><topic>String theory</topic><toplevel>online_resources</toplevel><creatorcontrib>Guidetti, Veronica</creatorcontrib><creatorcontrib>Righi, Nicole</creatorcontrib><creatorcontrib>Venken, Gerben</creatorcontrib><creatorcontrib>Westphal, Alexander</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Guidetti, Veronica</au><au>Righi, Nicole</au><au>Venken, Gerben</au><au>Westphal, Alexander</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Axionic Festina Lente</atitle><jtitle>arXiv.org</jtitle><date>2023-01-23</date><risdate>2023</risdate><eissn>2331-8422</eissn><abstract>The swampland conjecture known as Festina Lente (FL) imposes a lower bound on the mass of all charged particles in a quasi-de Sitter space. In this paper, we propose the aFL (axionic Festina Lente) bound, an extension of FL to axion-like particles arising from type II string theory. We find that the product of the instanton action and the axion decay constant is bounded from below by the vacuum energy. This is achieved indirectly, using dimensional reduction on Calabi-Yau threefolds, and translating the FL result for dipoles into a purely geometric bound. We discuss axionic black holes evolution, and aFL constraints on Euclidean wormholes, showing that the gravitational arguments leading to the FL bound for U\((1)\) charged particles cannot be directly applied to axions. Moreover, we discuss phenomenological implications of the aFL bound, including constraints on string inflation models and the axion-photon coupling via kinetic mixing.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2206.03494</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2023-01
issn 2331-8422
language eng
recordid cdi_proquest_journals_2674531023
source Publicly Available Content Database
subjects Charged particles
Constraint modelling
Decay rate
Dipoles
Instantons
Lower bounds
String theory
title Axionic Festina Lente
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-29T06%3A22%3A17IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Axionic%20Festina%20Lente&rft.jtitle=arXiv.org&rft.au=Guidetti,%20Veronica&rft.date=2023-01-23&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.2206.03494&rft_dat=%3Cproquest%3E2674531023%3C/proquest%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a954-f9e3a870f64b8c379d38e993af7e613e54f87326bb9ad5bad914440482f98da83%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2674531023&rft_id=info:pmid/&rfr_iscdi=true