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A Chern-Simons pandemic
A bstract In this paper we study the consistency of generalized global symmetries in theories of quantum gravity, in particular string theory. Such global symmetries arise in theories with ( p + 1)-form gauge fields, and for spacetime dimension d ≤ p + 3 there are obstructions to their breaking even...
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Published in: | The journal of high energy physics 2017-07, Vol.2017 (7), p.1-49, Article 123 |
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container_title | The journal of high energy physics |
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creator | Montero, Miguel Uranga, Angel M. Valenzuela, Irene |
description | A
bstract
In this paper we study the consistency of generalized global symmetries in theories of quantum gravity, in particular string theory. Such global symmetries arise in theories with (
p
+ 1)-form gauge fields, and for spacetime dimension
d
≤
p
+ 3 there are obstructions to their breaking even by quantum effects of charged objects. In 4d theories with a 2-form gauge field (or with an axion scalar), these fields endow Schwarzschild black holes with quantum hair, a global charge leading to usual trouble with remnants. We describe precise mechanisms, and examples from string compactifications and holographic pairs, in which these problems are evaded by either gauging or breaking the global symmetry, via (suitable versions of) Stuckelberg or 4-form couplings. We argue that even in the absence of such couplings, the generic solution in string theory is the breaking of the global symmetries by cubic Chern-Simons terms involving different antisymmetric tensor fields. We conjecture that any theory with (standard or higher-degree antisymmetric tensor) gauge fields is in the Swampland unless its effective action includes such Chern-Simons terms. This conjecture implies that many familiar theories, like QED (even including the charged particles required by the Weak Gravity Conjecture) or
N
=
8
supergravity in four dimensions, are inconsistent in quantum gravity unless they are completed by these Chern-Simons terms. |
doi_str_mv | 10.1007/JHEP07(2017)123 |
format | article |
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bstract
In this paper we study the consistency of generalized global symmetries in theories of quantum gravity, in particular string theory. Such global symmetries arise in theories with (
p
+ 1)-form gauge fields, and for spacetime dimension
d
≤
p
+ 3 there are obstructions to their breaking even by quantum effects of charged objects. In 4d theories with a 2-form gauge field (or with an axion scalar), these fields endow Schwarzschild black holes with quantum hair, a global charge leading to usual trouble with remnants. We describe precise mechanisms, and examples from string compactifications and holographic pairs, in which these problems are evaded by either gauging or breaking the global symmetry, via (suitable versions of) Stuckelberg or 4-form couplings. We argue that even in the absence of such couplings, the generic solution in string theory is the breaking of the global symmetries by cubic Chern-Simons terms involving different antisymmetric tensor fields. We conjecture that any theory with (standard or higher-degree antisymmetric tensor) gauge fields is in the Swampland unless its effective action includes such Chern-Simons terms. This conjecture implies that many familiar theories, like QED (even including the charged particles required by the Weak Gravity Conjecture) or
N
=
8
supergravity in four dimensions, are inconsistent in quantum gravity unless they are completed by these Chern-Simons terms.</description><identifier>ISSN: 1029-8479</identifier><identifier>EISSN: 1029-8479</identifier><identifier>DOI: 10.1007/JHEP07(2017)123</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Black Holes ; Black Holes in String Theory ; Charged particles ; Classical and Quantum Gravitation ; Couplings ; Elementary Particles ; Gaging ; Global Symmetries ; Hair ; High energy physics ; Obstructions ; Physics ; Physics and Astronomy ; Quantum electrodynamics ; Quantum Field Theories ; Quantum Field Theory ; Quantum gravity ; Quantum Physics ; Regular Article - Theoretical Physics ; Relativity Theory ; String Theory ; Supergravity ; Superstring Vacua</subject><ispartof>The journal of high energy physics, 2017-07, Vol.2017 (7), p.1-49, Article 123</ispartof><rights>The Author(s) 2017</rights><rights>Journal of High Energy Physics is a copyright of Springer, 2017.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c417t-23bee44b181385974faab2df6fcca7c7a229c495f9ffd489a4910c381f4fa0193</citedby><cites>FETCH-LOGICAL-c417t-23bee44b181385974faab2df6fcca7c7a229c495f9ffd489a4910c381f4fa0193</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.proquest.com/docview/1923934273/fulltextPDF?pq-origsite=primo$$EPDF$$P50$$Gproquest$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/1923934273?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,25753,27924,27925,37012,44590,75126</link.rule.ids></links><search><creatorcontrib>Montero, Miguel</creatorcontrib><creatorcontrib>Uranga, Angel M.</creatorcontrib><creatorcontrib>Valenzuela, Irene</creatorcontrib><title>A Chern-Simons pandemic</title><title>The journal of high energy physics</title><addtitle>J. High Energ. Phys</addtitle><description>A
bstract
In this paper we study the consistency of generalized global symmetries in theories of quantum gravity, in particular string theory. Such global symmetries arise in theories with (
p
+ 1)-form gauge fields, and for spacetime dimension
d
≤
p
+ 3 there are obstructions to their breaking even by quantum effects of charged objects. In 4d theories with a 2-form gauge field (or with an axion scalar), these fields endow Schwarzschild black holes with quantum hair, a global charge leading to usual trouble with remnants. We describe precise mechanisms, and examples from string compactifications and holographic pairs, in which these problems are evaded by either gauging or breaking the global symmetry, via (suitable versions of) Stuckelberg or 4-form couplings. We argue that even in the absence of such couplings, the generic solution in string theory is the breaking of the global symmetries by cubic Chern-Simons terms involving different antisymmetric tensor fields. We conjecture that any theory with (standard or higher-degree antisymmetric tensor) gauge fields is in the Swampland unless its effective action includes such Chern-Simons terms. This conjecture implies that many familiar theories, like QED (even including the charged particles required by the Weak Gravity Conjecture) or
N
=
8
supergravity in four dimensions, are inconsistent in quantum gravity unless they are completed by these Chern-Simons terms.</description><subject>Black Holes</subject><subject>Black Holes in String Theory</subject><subject>Charged particles</subject><subject>Classical and Quantum Gravitation</subject><subject>Couplings</subject><subject>Elementary Particles</subject><subject>Gaging</subject><subject>Global Symmetries</subject><subject>Hair</subject><subject>High energy physics</subject><subject>Obstructions</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum electrodynamics</subject><subject>Quantum Field Theories</subject><subject>Quantum Field Theory</subject><subject>Quantum gravity</subject><subject>Quantum Physics</subject><subject>Regular Article - Theoretical Physics</subject><subject>Relativity Theory</subject><subject>String Theory</subject><subject>Supergravity</subject><subject>Superstring Vacua</subject><issn>1029-8479</issn><issn>1029-8479</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><sourceid>DOA</sourceid><recordid>eNp1kEFPAjEQRhujiYieuZJ40cPKTNul7ZEQFAyJJuq56XZbXAJbbOHgv7e4xnjx1EnzvjeTj5ABwh0CiNHjfPYM4oYCiluk7IT0EKgqJBfq9M98Ti5SWgNgiQp6ZDAZTt9dbIuXZhvaNNyZtnbbxl6SM282yV39vH3ydj97nc6L5dPDYjpZFpaj2BeUVc5xXqFEJksluDemorUfe2uNsMJQqixXpVfe11wqwxWCZRJ9JgEV65NF562DWetdbLYmfupgGv39EeJKm7hv7MZpy9i4BGEZl4bz2lXonAFbeQnluKptdl13rl0MHweX9nodDrHN52tUlCnGqWCZGnWUjSGl6PzvVgR9bFJ3Tepjkzo3mRPQJVIm25WLf7z_RL4AGAly2A</recordid><startdate>20170701</startdate><enddate>20170701</enddate><creator>Montero, Miguel</creator><creator>Uranga, Angel M.</creator><creator>Valenzuela, Irene</creator><general>Springer Berlin Heidelberg</general><general>Springer Nature B.V</general><general>SpringerOpen</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>DOA</scope></search><sort><creationdate>20170701</creationdate><title>A Chern-Simons pandemic</title><author>Montero, Miguel ; Uranga, Angel M. ; Valenzuela, Irene</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c417t-23bee44b181385974faab2df6fcca7c7a229c495f9ffd489a4910c381f4fa0193</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Black Holes</topic><topic>Black Holes in String Theory</topic><topic>Charged particles</topic><topic>Classical and Quantum Gravitation</topic><topic>Couplings</topic><topic>Elementary Particles</topic><topic>Gaging</topic><topic>Global Symmetries</topic><topic>Hair</topic><topic>High energy physics</topic><topic>Obstructions</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum electrodynamics</topic><topic>Quantum Field Theories</topic><topic>Quantum Field Theory</topic><topic>Quantum gravity</topic><topic>Quantum Physics</topic><topic>Regular Article - Theoretical Physics</topic><topic>Relativity Theory</topic><topic>String Theory</topic><topic>Supergravity</topic><topic>Superstring Vacua</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Montero, Miguel</creatorcontrib><creatorcontrib>Uranga, Angel M.</creatorcontrib><creatorcontrib>Valenzuela, Irene</creatorcontrib><collection>Springer Nature OA Free Journals</collection><collection>CrossRef</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</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>Open Access: DOAJ - Directory of Open Access Journals</collection><jtitle>The journal of high energy physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Montero, Miguel</au><au>Uranga, Angel M.</au><au>Valenzuela, Irene</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A Chern-Simons pandemic</atitle><jtitle>The journal of high energy physics</jtitle><stitle>J. High Energ. Phys</stitle><date>2017-07-01</date><risdate>2017</risdate><volume>2017</volume><issue>7</issue><spage>1</spage><epage>49</epage><pages>1-49</pages><artnum>123</artnum><issn>1029-8479</issn><eissn>1029-8479</eissn><abstract>A
bstract
In this paper we study the consistency of generalized global symmetries in theories of quantum gravity, in particular string theory. Such global symmetries arise in theories with (
p
+ 1)-form gauge fields, and for spacetime dimension
d
≤
p
+ 3 there are obstructions to their breaking even by quantum effects of charged objects. In 4d theories with a 2-form gauge field (or with an axion scalar), these fields endow Schwarzschild black holes with quantum hair, a global charge leading to usual trouble with remnants. We describe precise mechanisms, and examples from string compactifications and holographic pairs, in which these problems are evaded by either gauging or breaking the global symmetry, via (suitable versions of) Stuckelberg or 4-form couplings. We argue that even in the absence of such couplings, the generic solution in string theory is the breaking of the global symmetries by cubic Chern-Simons terms involving different antisymmetric tensor fields. We conjecture that any theory with (standard or higher-degree antisymmetric tensor) gauge fields is in the Swampland unless its effective action includes such Chern-Simons terms. This conjecture implies that many familiar theories, like QED (even including the charged particles required by the Weak Gravity Conjecture) or
N
=
8
supergravity in four dimensions, are inconsistent in quantum gravity unless they are completed by these Chern-Simons terms.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1007/JHEP07(2017)123</doi><tpages>49</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Black Holes Black Holes in String Theory Charged particles Classical and Quantum Gravitation Couplings Elementary Particles Gaging Global Symmetries Hair High energy physics Obstructions Physics Physics and Astronomy Quantum electrodynamics Quantum Field Theories Quantum Field Theory Quantum gravity Quantum Physics Regular Article - Theoretical Physics Relativity Theory String Theory Supergravity Superstring Vacua |
title | A Chern-Simons pandemic |
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