Strings in Ramond-Ramond backgrounds from the Neveu-Schwarz-Ramond formalism
A bstract We treat RR flux backgrounds of type II string theory in the framework of closed superstring field theory based on the NSR formalism, focusing on two examples: (1) the pp-wave background supported by 5-form flux, and (2) AdS 3 × S 3 × M 4 supported by mixed 3-form fluxes. In both cases, we...
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container_title | The journal of high energy physics |
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creator | Cho, Minjae Collier, Scott Yin, Xi |
description | A
bstract
We treat RR flux backgrounds of type II string theory in the framework of closed superstring field theory based on the NSR formalism, focusing on two examples: (1) the pp-wave background supported by 5-form flux, and (2) AdS
3
×
S
3
×
M
4
supported by mixed 3-form fluxes. In both cases, we analyze the classical string field solution perturbatively, and compute the correction to the dispersion relation of string states to quadratic order in the RR flux. In the first example, our result is in a delicate way consistent with that obtained from lightcone quantization of the Green-Schwarz string. In the second example, we will obtain numerically the mass corrections to pulsating type IIB strings in AdS
3
×
S
3
×
M
4
. Our results, valid at finite AdS radius, agree with previously known answers in the semiclassical limit and in the BMN limit respectively. |
doi_str_mv | 10.1007/JHEP12(2020)123 |
format | Article |
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bstract
We treat RR flux backgrounds of type II string theory in the framework of closed superstring field theory based on the NSR formalism, focusing on two examples: (1) the pp-wave background supported by 5-form flux, and (2) AdS
3
×
S
3
×
M
4
supported by mixed 3-form fluxes. In both cases, we analyze the classical string field solution perturbatively, and compute the correction to the dispersion relation of string states to quadratic order in the RR flux. In the first example, our result is in a delicate way consistent with that obtained from lightcone quantization of the Green-Schwarz string. In the second example, we will obtain numerically the mass corrections to pulsating type IIB strings in AdS
3
×
S
3
×
M
4
. Our results, valid at finite AdS radius, agree with previously known answers in the semiclassical limit and in the BMN limit respectively.</description><identifier>ISSN: 1029-8479</identifier><identifier>EISSN: 1029-8479</identifier><identifier>DOI: 10.1007/JHEP12(2020)123</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Classical and Quantum Gravitation ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; Elementary Particles ; Field theory ; Fluxes ; Formalism ; High energy physics ; Physical Sciences ; Physics ; Physics and Astronomy ; Physics, Particles & Fields ; Quantum Field Theories ; Quantum Field Theory ; Quantum Physics ; Regular Article - Theoretical Physics ; Relativity Theory ; Science & Technology ; String Field Theory ; String Theory ; Superstrings and Heterotic Strings</subject><ispartof>The journal of high energy physics, 2020-12, Vol.2020 (12), p.1-44, Article 123</ispartof><rights>The Author(s) 2020</rights><rights>The Author(s) 2020. This work is published under https://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>true</woscitedreferencessubscribed><woscitedreferencescount>17</woscitedreferencescount><woscitedreferencesoriginalsourcerecordid>wos000601400500009</woscitedreferencesoriginalsourcerecordid><citedby>FETCH-LOGICAL-c510t-5d55d537c7963f5eea898ff1571fb3f81d70223d70819e75e5126b9c24bde77d3</citedby><cites>FETCH-LOGICAL-c510t-5d55d537c7963f5eea898ff1571fb3f81d70223d70819e75e5126b9c24bde77d3</cites><orcidid>0000-0002-8647-6653</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/JHEP12(2020)123$$EPDF$$P50$$Gspringer$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://doi.org/10.1007/JHEP12(2020)123$$EHTML$$P50$$Gspringer$$Hfree_for_read</linktohtml><link.rule.ids>230,315,781,785,865,886,2103,2115,27928,27929,41124,42193,51580</link.rule.ids><backlink>$$Uhttps://www.osti.gov/servlets/purl/1851018$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Cho, Minjae</creatorcontrib><creatorcontrib>Collier, Scott</creatorcontrib><creatorcontrib>Yin, Xi</creatorcontrib><creatorcontrib>Harvard Univ., Cambridge, MA (United States)</creatorcontrib><title>Strings in Ramond-Ramond backgrounds from the Neveu-Schwarz-Ramond formalism</title><title>The journal of high energy physics</title><addtitle>J. High Energ. Phys</addtitle><addtitle>J HIGH ENERGY PHYS</addtitle><description>A
bstract
We treat RR flux backgrounds of type II string theory in the framework of closed superstring field theory based on the NSR formalism, focusing on two examples: (1) the pp-wave background supported by 5-form flux, and (2) AdS
3
×
S
3
×
M
4
supported by mixed 3-form fluxes. In both cases, we analyze the classical string field solution perturbatively, and compute the correction to the dispersion relation of string states to quadratic order in the RR flux. In the first example, our result is in a delicate way consistent with that obtained from lightcone quantization of the Green-Schwarz string. In the second example, we will obtain numerically the mass corrections to pulsating type IIB strings in AdS
3
×
S
3
×
M
4
. Our results, valid at finite AdS radius, agree with previously known answers in the semiclassical limit and in the BMN limit respectively.</description><subject>Classical and Quantum Gravitation</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>Elementary Particles</subject><subject>Field theory</subject><subject>Fluxes</subject><subject>Formalism</subject><subject>High energy physics</subject><subject>Physical Sciences</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Physics, Particles & Fields</subject><subject>Quantum Field Theories</subject><subject>Quantum Field Theory</subject><subject>Quantum Physics</subject><subject>Regular Article - Theoretical Physics</subject><subject>Relativity Theory</subject><subject>Science & Technology</subject><subject>String Field Theory</subject><subject>String Theory</subject><subject>Superstrings and Heterotic Strings</subject><issn>1029-8479</issn><issn>1029-8479</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><sourceid>C6C</sourceid><sourceid>AOWDO</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>DOA</sourceid><recordid>eNqNkUGPFCEQhTtGE9fVs9eOXjSm3YJuBjiayequmahx9UxoKGYYp2EWGDf662VsXb2YmBCqQt77qMprmscEXhIAfvb24vwDoc8oUHhOaH-nOSFAZScGLu_-1d9vHuS8BSCMSDhpVlcl-bDOrQ_tRz3FYLu5tKM2X9YpHoLNrUtxassG23f4FQ_dldnc6PT9t9LFNOmdz9PD5p7Tu4yPftXT5vPr80_Li271_s3l8tWqM4xA6Zhl9fTccLnoHUPUQgrnCOPEjb0TxHKgtK-3IBI5Q0boYpSGDqNFzm1_2lzOXBv1Vu2Tn3T6pqL26udDTGulU_Fmh2oh-eiMACdADohUaAFccy0tNRYGXllPZlbMxatsfEGzMTEENEURUQcmooqezqJ9itcHzEVt4yGFuqOilTHQCj2izmaVSTHnhO52NALqmJGaM1LHjFTNqDpezI4bHKOrn2MweOsCgAWQAYDVDmRVi_9XL33RxcewrAmWaoXZmvfHuDH9WeBfs_0A8amyIg</recordid><startdate>20201201</startdate><enddate>20201201</enddate><creator>Cho, Minjae</creator><creator>Collier, Scott</creator><creator>Yin, Xi</creator><general>Springer Berlin Heidelberg</general><general>Springer Nature</general><general>Springer Nature B.V</general><general>SpringerOpen</general><scope>C6C</scope><scope>AOWDO</scope><scope>BLEPL</scope><scope>DTL</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>OIOZB</scope><scope>OTOTI</scope><scope>DOA</scope><orcidid>https://orcid.org/0000-0002-8647-6653</orcidid></search><sort><creationdate>20201201</creationdate><title>Strings in Ramond-Ramond backgrounds from the Neveu-Schwarz-Ramond formalism</title><author>Cho, Minjae ; Collier, Scott ; Yin, Xi</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c510t-5d55d537c7963f5eea898ff1571fb3f81d70223d70819e75e5126b9c24bde77d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Classical and Quantum Gravitation</topic><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>Elementary Particles</topic><topic>Field theory</topic><topic>Fluxes</topic><topic>Formalism</topic><topic>High energy physics</topic><topic>Physical Sciences</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Physics, Particles & Fields</topic><topic>Quantum Field Theories</topic><topic>Quantum Field Theory</topic><topic>Quantum Physics</topic><topic>Regular Article - Theoretical Physics</topic><topic>Relativity Theory</topic><topic>Science & Technology</topic><topic>String Field Theory</topic><topic>String Theory</topic><topic>Superstrings and Heterotic Strings</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Cho, Minjae</creatorcontrib><creatorcontrib>Collier, Scott</creatorcontrib><creatorcontrib>Yin, Xi</creatorcontrib><creatorcontrib>Harvard Univ., Cambridge, MA (United States)</creatorcontrib><collection>Springer Nature OA Free Journals</collection><collection>Web of Science - Science Citation Index Expanded - 2020</collection><collection>Web of Science Core Collection</collection><collection>Science Citation Index Expanded</collection><collection>CrossRef</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</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>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Access via ProQuest (Open Access)</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>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><collection>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>Cho, Minjae</au><au>Collier, Scott</au><au>Yin, Xi</au><aucorp>Harvard Univ., Cambridge, MA (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Strings in Ramond-Ramond backgrounds from the Neveu-Schwarz-Ramond formalism</atitle><jtitle>The journal of high energy physics</jtitle><stitle>J. High Energ. Phys</stitle><stitle>J HIGH ENERGY PHYS</stitle><date>2020-12-01</date><risdate>2020</risdate><volume>2020</volume><issue>12</issue><spage>1</spage><epage>44</epage><pages>1-44</pages><artnum>123</artnum><issn>1029-8479</issn><eissn>1029-8479</eissn><abstract>A
bstract
We treat RR flux backgrounds of type II string theory in the framework of closed superstring field theory based on the NSR formalism, focusing on two examples: (1) the pp-wave background supported by 5-form flux, and (2) AdS
3
×
S
3
×
M
4
supported by mixed 3-form fluxes. In both cases, we analyze the classical string field solution perturbatively, and compute the correction to the dispersion relation of string states to quadratic order in the RR flux. In the first example, our result is in a delicate way consistent with that obtained from lightcone quantization of the Green-Schwarz string. In the second example, we will obtain numerically the mass corrections to pulsating type IIB strings in AdS
3
×
S
3
×
M
4
. Our results, valid at finite AdS radius, agree with previously known answers in the semiclassical limit and in the BMN limit respectively.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1007/JHEP12(2020)123</doi><tpages>44</tpages><orcidid>https://orcid.org/0000-0002-8647-6653</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Classical and Quantum Gravitation CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS Elementary Particles Field theory Fluxes Formalism High energy physics Physical Sciences Physics Physics and Astronomy Physics, Particles & Fields Quantum Field Theories Quantum Field Theory Quantum Physics Regular Article - Theoretical Physics Relativity Theory Science & Technology String Field Theory String Theory Superstrings and Heterotic Strings |
title | Strings in Ramond-Ramond backgrounds from the Neveu-Schwarz-Ramond formalism |
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