{"title":"Unitarization of the one-loop graviton-graviton scattering amplitudes and study of the graviball","authors":"J.A. Oller , Marcela Peláez","doi":"10.1016/j.physletb.2025.139275","DOIUrl":null,"url":null,"abstract":"<div><div>From the graviton-graviton scattering amplitudes calculated perturbatively in quantum gravity to the one-loop order, we develop further a formalism that allows one to calculate infrared-finite partial-wave amplitudes fulfilling perturbative unitarity. As a result of this process a parameter dubbed <span><math><mi>ln</mi><mo></mo><mi>a</mi></math></span> emerges that separate between infrared and typical external momenta. The resulting partial-wave amplitudes are next unitarized by employing the Inverse Amplitude Method and the algebraic-<span><math><mi>N</mi><mo>/</mo><mi>D</mi></math></span> method. Then, the graviball resonance, with a similar pole position, is confirmed in the <em>S</em>-wave partial-wave amplitude for all unitarization methods, also with respect to the unitarization of only the leading-order amplitude. Although the spectrum of the theory is independent of the specific value of <span><math><mi>ln</mi><mo></mo><mi>a</mi></math></span>, the requirement for a well-behaved unitarized effective field theory of gravity identifies the optimal range of <span><math><mi>ln</mi><mo></mo><mi>a</mi></math></span> for our next-to-leading-order calculations as <span><math><mn>0.5</mn><mo>≲</mo><mi>ln</mi><mo></mo><mi>a</mi><mo>≲</mo><mn>1.7</mn></math></span>. Briefly, we discuss the <em>D</em>-wave scattering that is weaker than the <em>S</em>-wave scattering, repulsive and non-resonant for <span><math><mi>ln</mi><mo></mo><mi>a</mi><mo>≈</mo><mn>1</mn></math></span>.</div></div>","PeriodicalId":20162,"journal":{"name":"Physics Letters B","volume":"861 ","pages":"Article 139275"},"PeriodicalIF":4.3000,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physics Letters B","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0370269325000358","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
From the graviton-graviton scattering amplitudes calculated perturbatively in quantum gravity to the one-loop order, we develop further a formalism that allows one to calculate infrared-finite partial-wave amplitudes fulfilling perturbative unitarity. As a result of this process a parameter dubbed emerges that separate between infrared and typical external momenta. The resulting partial-wave amplitudes are next unitarized by employing the Inverse Amplitude Method and the algebraic- method. Then, the graviball resonance, with a similar pole position, is confirmed in the S-wave partial-wave amplitude for all unitarization methods, also with respect to the unitarization of only the leading-order amplitude. Although the spectrum of the theory is independent of the specific value of , the requirement for a well-behaved unitarized effective field theory of gravity identifies the optimal range of for our next-to-leading-order calculations as . Briefly, we discuss the D-wave scattering that is weaker than the S-wave scattering, repulsive and non-resonant for .
期刊介绍:
Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.