{"title":"Celestial string integrands & their expansions","authors":"Daniel Bockisch","doi":"10.1016/j.nuclphysb.2025.116792","DOIUrl":null,"url":null,"abstract":"<div><div>We transform the one-loop four-point type I open superstring gluon amplitude to correlation functions on the celestial sphere including both the (non-)orientable planar and non-planar sector. This requires a Mellin transform with respect to the energies of the scattered strings, as well as to integrate over the open-string worldsheet moduli space. After accomplishing the former we obtain celestial string integrands with remaining worldsheet integrals <span><math><mi>Ψ</mi><mrow><mo>(</mo><mi>β</mi><mo>)</mo></mrow></math></span>, where <em>β</em> is related to the conformal scaling dimensions of the conformal primary operators under consideration. Employing an alternative approach of performing an <span><math><msup><mrow><mi>α</mi></mrow><mrow><mo>′</mo></mrow></msup></math></span>-expansion of the open superstring amplitude first and Mellin transforming afterwards, we obtain a fully integrated expression, capturing the pole structure in the <em>β</em>-plane. The same analysis is performed at tree-level yielding similar results. We conclude by solving <span><math><mi>Ψ</mi><mrow><mo>(</mo><mi>β</mi><mo>)</mo></mrow></math></span> for specific values of <em>β</em>, consistently reproducing the results of the <span><math><msup><mrow><mi>α</mi></mrow><mrow><mo>′</mo></mrow></msup></math></span>-expansion ansatz. In all approaches we find that the dependence on <span><math><msup><mrow><mi>α</mi></mrow><mrow><mo>′</mo></mrow></msup></math></span> reduces to that of a simple overall factor of <span><math><msup><mrow><mo>(</mo><msup><mrow><mi>α</mi></mrow><mrow><mo>′</mo></mrow></msup><mo>)</mo></mrow><mrow><mi>β</mi><mo>−</mo><mn>3</mn></mrow></msup></math></span> at loop and <span><math><msup><mrow><mo>(</mo><msup><mrow><mi>α</mi></mrow><mrow><mo>′</mo></mrow></msup><mo>)</mo></mrow><mrow><mi>β</mi></mrow></msup></math></span> at tree level, consistent with previous literature.</div></div>","PeriodicalId":54712,"journal":{"name":"Nuclear Physics B","volume":"1011 ","pages":"Article 116792"},"PeriodicalIF":2.5000,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Nuclear Physics B","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0550321325000021","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"PHYSICS, PARTICLES & FIELDS","Score":null,"Total":0}
引用次数: 0
Abstract
We transform the one-loop four-point type I open superstring gluon amplitude to correlation functions on the celestial sphere including both the (non-)orientable planar and non-planar sector. This requires a Mellin transform with respect to the energies of the scattered strings, as well as to integrate over the open-string worldsheet moduli space. After accomplishing the former we obtain celestial string integrands with remaining worldsheet integrals , where β is related to the conformal scaling dimensions of the conformal primary operators under consideration. Employing an alternative approach of performing an -expansion of the open superstring amplitude first and Mellin transforming afterwards, we obtain a fully integrated expression, capturing the pole structure in the β-plane. The same analysis is performed at tree-level yielding similar results. We conclude by solving for specific values of β, consistently reproducing the results of the -expansion ansatz. In all approaches we find that the dependence on reduces to that of a simple overall factor of at loop and at tree level, consistent with previous literature.
期刊介绍:
Nuclear Physics B focuses on the domain of high energy physics, quantum field theory, statistical systems, and mathematical physics, and includes four main sections: high energy physics - phenomenology, high energy physics - theory, high energy physics - experiment, and quantum field theory, statistical systems, and mathematical physics. The emphasis is on original research papers (Frontiers Articles or Full Length Articles), but Review Articles are also welcome.