Raman response of the charge density wave in cuprate superconductors

dc.creatorMoallison Ferreira Cavalcante
dc.creatorSoumen Kumar Bag
dc.creatorIndranil Paul
dc.creatorAlain Sacuto
dc.creatorMaria Carolina de Oliveira Aguiar
dc.creatorMarcello Civelli
dc.date.accessioned2025-02-04T19:06:51Z
dc.date.accessioned2025-09-08T22:49:25Z
dc.date.available2025-02-04T19:06:51Z
dc.date.issued2023-10-10
dc.identifier.doi10.1103/physrevb.108.165111
dc.identifier.issn2469-9969
dc.identifier.urihttps://hdl.handle.net/1843/79656
dc.languageeng
dc.publisherUniversidade Federal de Minas Gerais
dc.relation.ispartofPhysical Review B
dc.rightsAcesso Aberto
dc.subjectOndas (Física)
dc.subject.otherCharge density waves
dc.subject.otherElectronic structure
dc.subject.otherHigh-temperature superconductors
dc.subject.otherSuperconductivity
dc.subject.otherPath integrals
dc.titleRaman response of the charge density wave in cuprate superconductors
dc.typeArtigo de periódico
local.citation.epage13
local.citation.issue16
local.citation.spage01
local.citation.volume108
local.description.resumoWe study the Raman response, for B1g and B2g light-polarization symmetries, of the charge density wave phase appearing in the underdoped region of cuprate superconductors. We show that the B2g response provides a distinctive signature of the charge order, independently of the details of the electronic structure and from the concomitant presence of a pseudogap, in sharp contrast with the behavior of the B1g response. This well accounts for the Raman experimental results. We then clearly identify a charge density wave energy scale, and show that its doping dependence is eventually driven by the monotonic behavior of the pseudogap. This has also been pointed out in Raman experiments, and it is suggestive of a pseudogap ruling the multiple energy scales of the exotic phases appearing in the cuprate phase diagram.
local.publisher.countryBrasil
local.publisher.departmentICX - DEPARTAMENTO DE FÍSICA
local.publisher.initialsUFMG
local.url.externahttps://journals.aps.org/prb/pdf/10.1103/PhysRevB.108.165111

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