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Second-order combinatorial algebraic time-delay interferometry

dc.contributor.authorQian, Wei-Liang [UNESP]
dc.contributor.authorWang, Pan-Pan
dc.contributor.authorWu, Zhang-Qi
dc.contributor.authorShao, Cheng-Gang
dc.contributor.authorWang, Bin
dc.contributor.authorYue, Rui-Hong
dc.contributor.institutionYangzhou University
dc.contributor.institutionUniversidade de São Paulo (USP)
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.contributor.institutionHuazhong University of Science and Technology
dc.contributor.institutionShanghai Jiao Tong University
dc.date.accessioned2025-04-29T18:06:13Z
dc.date.issued2023-07-15
dc.description.abstractInspired by the combinatorial algebraic approach proposed by Dhurandhar et al., we propose two novel classes of second-generation time-delay interferometry (TDI) solutions and their further generalization. The primary strategy of the algorithm is to enumerate specific types of residual laser frequency noise associated with second-order commutators in products of time-displacement operators. The derivations are based on analyzing the delay time residual when expanded in time derivatives of the armlengths order-by-order. It is observed that the solutions obtained by such a scheme are primarily captured by the geometric TDI approach and therefore possess an intuitive interpretation. Nonetheless, the fully symmetric Sagnac and Sagnac-inspired combinations inherit the properties from the original algebraic approach, and subsequently lie outside of the scope of geometric TDI. We explicitly show that novel solutions, distinct from existing ones in terms of both algebraic structure and sensitivity curve, are encountered. Moreover, at its lowest order, the solution is furnished by commutators of relatively compact form. Besides the original Michelson-type solution, we elaborate on other types of solutions such as the Monitor, Beacon, Relay, Sagnac, fully symmetric Sagnac, and Sagnac-inspired ones. The average response functions, residual noise power spectral density, and sensitivity curves are evaluated for the obtained solutions. Also, the relations between the present scheme and other existing algorithms are discussed.en
dc.description.affiliationCenter for Gravitation and Cosmology College of Physical Science and Technology Yangzhou University
dc.description.affiliationEscola de Engenharia de Lorena Universidade de São Paulo, Lorena
dc.description.affiliationFaculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista, Guaratinguetá
dc.description.affiliationMOE Key Laboratory of Fundamental Physical Quantities Measurement Hubei Key Laboratory of Gravitation and Quantum Physics PGMF School of Physics Huazhong University of Science and Technology
dc.description.affiliationSchool of Aeronautics and Astronautics Shanghai Jiao Tong University
dc.description.affiliationUnespFaculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista, Guaratinguetá
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.108.022002
dc.identifier.citationPhysical Review D, v. 108, n. 2, 2023.
dc.identifier.doi10.1103/PhysRevD.108.022002
dc.identifier.issn2470-0029
dc.identifier.issn2470-0010
dc.identifier.scopus2-s2.0-85164969530
dc.identifier.urihttps://hdl.handle.net/11449/297318
dc.language.isoeng
dc.relation.ispartofPhysical Review D
dc.sourceScopus
dc.titleSecond-order combinatorial algebraic time-delay interferometryen
dc.typeArtigopt
dspace.entity.typePublication
relation.isOrgUnitOfPublicationa4071986-4355-47c3-a5a3-bd4d1a966e4f
relation.isOrgUnitOfPublication.latestForDiscoverya4071986-4355-47c3-a5a3-bd4d1a966e4f
unesp.author.orcid0000-0002-3450-1984 0000-0002-3450-1984 0000-0002-3450-1984[1]
unesp.author.orcid0000-0003-3433-3818[2]
unesp.author.orcid0000-0001-5017-9385[3]
unesp.author.orcid0000-0003-0343-3250[4]
unesp.campusUniversidade Estadual Paulista (UNESP), Faculdade de Engenharia e Ciências, Guaratinguetápt

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