{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1363951795367285376.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1016/0370-2693(83)90638-x"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:037026938390638X?httpAccept=text/xml"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:037026938390638X?httpAccept=text/plain"}}],"dc:title":[{"@value":"A cosmological bound on the invisible axion"}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004053896932106","@type":"Researcher","foaf:name":[{"@value":"L.F. Abbott"}]},{"@id":"https://cir.nii.ac.jp/crid/1383951795367285376","@type":"Researcher","foaf:name":[{"@value":"P. Sikivie"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"03702693"},{"@type":"PISSN","@value":"http://id.crossref.org/issn/03702693"},{"@type":"PISSN","@value":"https://id.crossref.org/issn/03702693"}],"prism:publicationName":[{"@value":"Physics Letters B"}],"dc:publisher":[{"@value":"Elsevier BV"}],"prism:publicationDate":"1983-01","prism:volume":"120","prism:number":"1-3","prism:startingPage":"133","prism:endingPage":"136"},"reviewed":"false","dc:rights":["https://www.elsevier.com/tdm/userlicense/1.0/"],"url":[{"@id":"https://api.elsevier.com/content/article/PII:037026938390638X?httpAccept=text/xml"},{"@id":"https://api.elsevier.com/content/article/PII:037026938390638X?httpAccept=text/plain"}],"createdAt":"2002-11-12","modifiedAt":"2019-04-02","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050001202619904640","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Topological susceptibility in finite temperature (2+1)-flavor QCD using gradient flow"},{"@value":"Topological susceptibility in finite temperature (\n<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mrow><mml:mn>2</mml:mn><mml:mo>+</mml:mo><mml:mn>1</mml:mn></mml:mrow></mml:math>\n)-flavor QCD using gradient flow"}]},{"@id":"https://cir.nii.ac.jp/crid/1050003824938231680","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"High scale validity of the DFSZ axion model with precision"}]},{"@id":"https://cir.nii.ac.jp/crid/1050013397240321536","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Axion cloud evaporation during inspiral of black hole binaries: The effects of backreaction and radiation"}]},{"@id":"https://cir.nii.ac.jp/crid/1050013397240382464","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Adiabatic evolution of the self-interacting axion field around rotating black holes"}]},{"@id":"https://cir.nii.ac.jp/crid/1050015897173949568","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Evolution of binary systems accompanying axion clouds in extreme mass ratio inspirals"}]},{"@id":"https://cir.nii.ac.jp/crid/1050020519547949184","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Circularly polarized gravitational waves in Chern-Simons gravity originating from an axion domain wall"}]},{"@id":"https://cir.nii.ac.jp/crid/1050023627021060608","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Revisiting the stochastic QCD axion window: departure from equilibrium during inflation"}]},{"@id":"https://cir.nii.ac.jp/crid/1050305101997724672","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Exploring the spin of ultralight dark matter with gravitational wave detectors"}]},{"@id":"https://cir.nii.ac.jp/crid/1050564285717966976","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Axion cosmology with long-lived domain walls"}]},{"@id":"https://cir.nii.ac.jp/crid/1050568617148931840","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Search for Axionlike Particles Produced in e⁺e⁻ Collisions at Belle II"},{"@value":"Search for Axionlike Particles Produced in \n<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:msup><mml:mi>e</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>e</mml:mi><mml:mo>−</mml:mo></mml:msup></mml:math>\n Collisions at Belle II"}]},{"@id":"https://cir.nii.ac.jp/crid/1050568937753949184","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Adiabatic suppression of the axion abundance and isocurvature due to coupling to hidden monopoles"}]},{"@id":"https://cir.nii.ac.jp/crid/1050575520345942528","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"ja","@value":"Stability of axion dark matter-photon conversion"}]},{"@id":"https://cir.nii.ac.jp/crid/1050580007680198016","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Ma-xion: Majoron as QCD axion in a radiative seesaw model"}]},{"@id":"https://cir.nii.ac.jp/crid/1050585803064650240","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Nuclear spin metrology with nitrogen vacancy center in diamond for axion dark matter detection"}]},{"@id":"https://cir.nii.ac.jp/crid/1050850412730657408","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Unified origin of axion and monopole dark matter, and solution to the domain-wall problem"}]},{"@id":"https://cir.nii.ac.jp/crid/1050856995323719936","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Electromagnetic waves propagating in the string axiverse"}]},{"@id":"https://cir.nii.ac.jp/crid/1050859758014229888","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Observing axions through photon ring dimming of black holes"}]},{"@id":"https://cir.nii.ac.jp/crid/1050862776837660544","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Quantum algorithm for the Vlasov simulation of the large-scale structure formation with massive neutrinos"}]},{"@id":"https://cir.nii.ac.jp/crid/1050863705678995968","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Squeezed quantum states of graviton and axion in the universe"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002215249509888","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Weighing the light gravitino mass with weak lensing surveys"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002216121103744","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Suppressing the QCD axion abundance by hidden monopoles"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004231122971648","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"On longevity of I-ball/oscillon"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004232441336192","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cosmologically safe QCD axion as a present from extra dimension"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004234433377664","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cosmological perturbations of axion with a dynamical decay constant"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004235015942656","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Affleck-Dine baryogenesis with<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mrow><mml:mi>R</mml:mi></mml:mrow></mml:math>-parity violation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004235017954816","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Observable dark radiation from a cosmologically safe QCD axion"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004235019955456","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"High-scale SUSY from an<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mi>R</mml:mi></mml:math>-invariant new inflation in the landscape"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004235026743808","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion isocurvature perturbations in low-scale models of hybrid inflation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004235045875968","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cosmologically Safe QCD Axion without Fine-Tuning"}]},{"@id":"https://cir.nii.ac.jp/crid/1360009142458279424","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A new method for detecting axion with cylindrical superconductor"}]},{"@id":"https://cir.nii.ac.jp/crid/1360009142481060352","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Stellar cooling anomalies and variant axion models"}]},{"@id":"https://cir.nii.ac.jp/crid/1360009142529519232","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Low scale leptogenesis in a model with promising CP structure"}]},{"@id":"https://cir.nii.ac.jp/crid/1360009142766063488","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Nano-Hz Gravitational-Wave Signature from Axion Dark Matter"}]},{"@id":"https://cir.nii.ac.jp/crid/1360009142766791040","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"What if ALP dark matter for the XENON1T excess is the inflaton"}]},{"@id":"https://cir.nii.ac.jp/crid/1360009142863592448","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Excess electronic recoil events in XENON1T"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013168719286656","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cosmic axion background"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013168768708224","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Probing relativistic axions from transient astrophysical sources"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013168772973568","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Analytic study of dark photon and gravitational wave production from axion"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013168868665344","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Heavy QCD axion in \n<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mi>b</mml:mi><mml:mo stretchy=\"false\">→</mml:mo><mml:mi>s</mml:mi></mml:math>\n transition: Enhanced limits and projections"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013276122714880","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Harvesting quantum coherence from axion dark matter"}]},{"@id":"https://cir.nii.ac.jp/crid/1360017279824598016","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Search for lepton flavor violating decay at FASER"}]},{"@id":"https://cir.nii.ac.jp/crid/1360017279824687232","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Anomaly-free axion dark matter in three Higgs doublet model and its phenomenological implications"}]},{"@id":"https://cir.nii.ac.jp/crid/1360017279881906816","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Pilot Search for Axion-Like Particles by a Three-Beam Stimulated Resonant Photon Collider with Short Pulse Lasers"}]},{"@id":"https://cir.nii.ac.jp/crid/1360017282193108480","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Implications of the cosmic birefringence measurement for the axion dark matter search"}]},{"@id":"https://cir.nii.ac.jp/crid/1360017282195344384","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Shining ALP dark radiation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360017282446535552","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A next-generation liquid xenon observatory for dark matter and neutrino physics"}]},{"@id":"https://cir.nii.ac.jp/crid/1360017282459032064","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Possible evidence of axion stars in HSC and OGLE microlensing events"}]},{"@id":"https://cir.nii.ac.jp/crid/1360021389803405824","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Implications of multi-axion dark matter on structure formation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360021390745635072","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"QCD axion hybrid inflation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360021390746954752","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Neutrino astronomy as a probe of physics beyond the Standard Model: Decay of sub-MeV \n<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mrow><mml:mi>B</mml:mi><mml:mtext>−</mml:mtext><mml:mi>L</mml:mi></mml:mrow></mml:math>\n gauge boson dark matter"}]},{"@id":"https://cir.nii.ac.jp/crid/1360021390747001600","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"QCD axion: A unique player in the axiverse with mixings"}]},{"@id":"https://cir.nii.ac.jp/crid/1360021391875099520","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Ultraviolet sensitivity of Peccei-Quinn inflation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360025430624795264","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion detection via superfluid 3He ferromagnetic phase and quantum measurement techniques"}]},{"@id":"https://cir.nii.ac.jp/crid/1360025430626904448","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Induced domain walls of QCD axion, and gravitational waves"}]},{"@id":"https://cir.nii.ac.jp/crid/1360025430645279104","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Primordial black holes"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283690224937856","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Flaxion: a minimal extension to solve puzzles in the standard model"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283692429948544","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Domain wall and isocurvature perturbation problems in axion models"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283692803673984","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Production of dark matter axions from collapse of string-wall systems"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283692804221184","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Peccei-Quinn symmetry from a gauged discrete<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mi>R</mml:mi></mml:math>symmetry"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283692804804608","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion dark matter from topological defects"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283692805296640","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion dark matter in the post-inflationary Peccei-Quinn symmetry breaking scenario"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285706108155904","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Topological susceptibility at high temperature on the lattice"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285707418618496","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cosmological problems of the string axion alleviated by high scale SUSY of m3/2≃ 10–100 TeV"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285707421554048","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Detecting axion stars with radio telescopes"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285707421610880","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cosmological abundance of the QCD axion coupled to hidden photons"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285707421625856","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"QCD axion dark matter from long-lived domain walls during matter domination"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285707421630080","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cosmologically allowed regions for the axion decay constant F"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285709409874304","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dynamics of Peccei-Quinn breaking field after inflation and axion isocurvature perturbations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285709990413440","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Evolution and thermalization of dark matter axions in the condensed regime"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285710000865280","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Current status of top-specific variant axion model"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285711151808384","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"AXIVERSE AND BLACK HOLE"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285714435870976","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Bosonic coherent motions in the Universe"}]},{"@id":"https://cir.nii.ac.jp/crid/1360286991764117120","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Ghost-free non-local <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\" id=\"d1e106\" altimg=\"si17.svg\"><mml:mrow><mml:mi>F</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity cosmology"}]},{"@id":"https://cir.nii.ac.jp/crid/1360286994330818432","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Efficient self-resonance instability from axions"}]},{"@id":"https://cir.nii.ac.jp/crid/1360286994945241984","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dynamical solution to the axion domain wall problem"}]},{"@id":"https://cir.nii.ac.jp/crid/1360290617480850688","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Probing axionlike particles via cosmic microwave background polarization"}]},{"@id":"https://cir.nii.ac.jp/crid/1360290617480866688","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Green Bank and Effelsberg Radio Telescope Searches for Axion Dark Matter Conversion in Neutron Star Magnetospheres"}]},{"@id":"https://cir.nii.ac.jp/crid/1360290617488774784","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Stochastic axion dark matter in axion landscape"}]},{"@id":"https://cir.nii.ac.jp/crid/1360290617488909440","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"XENON1T Excess from Anomaly-Free Axionlike Dark Matter and Its Implications for Stellar Cooling Anomaly"}]},{"@id":"https://cir.nii.ac.jp/crid/1360290617759385856","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Particle production from oscillating scalar field and consistency of Boltzmann equation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360290617760525184","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"21 cm forest probes on axion dark matter in postinflationary Peccei-Quinn symmetry breaking scenarios"}]},{"@id":"https://cir.nii.ac.jp/crid/1360290617879265152","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"QCD axions and CMB anisotropy"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643706445824","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Hidden dark matter from Starobinsky inflation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643707740416","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cosmic axion force"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643715217152","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Can primordial black holes as all dark matter explain fast radio bursts?"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643724708608","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Electron beam dump constraints on light bosons with lepton flavor violating couplings"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643773635840","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Semi-secretly interacting Axion-like particle as an explanation of Fermilab muon g − 2 measurement"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643847550848","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Search for sub-eV axion-like resonance states via stimulated quasi-parallel laser collisions with the parameterization including fully asymmetric collisional geometry"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643864254464","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Presupernova ultralight axionlike particles"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298339718417792","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Phenomenology of CP-even ALP"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298755610293120","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 data"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298755610963712","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Observational constraint on axion dark matter with gravitational waves"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298757403129472","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Probing massive scalar and vector fields with binary pulsars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298757421279232","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Resonant axion radiation conversion in solar spicules"}]},{"@id":"https://cir.nii.ac.jp/crid/1360302864771032448","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Role of QCD in moduli stabilization during inflation and axion dark matter"}]},{"@id":"https://cir.nii.ac.jp/crid/1360302864792957440","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Resonant production of dark photons from axions without a large coupling"}]},{"@id":"https://cir.nii.ac.jp/crid/1360302866839255296","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Can baryon asymmetry be explained by a large initial value before inflation?"}]},{"@id":"https://cir.nii.ac.jp/crid/1360302866839401728","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Hadrophobic axion from a GUT"}]},{"@id":"https://cir.nii.ac.jp/crid/1360302866848989824","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A generic formation mechanism of ultralight dark matter solar halos"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306904390308352","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Bubble misalignment mechanism for axions"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306904393057024","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"First Result for Dark Matter Search by WINERED"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306904404915200","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Self-interacting axion clouds around rotating black holes in binary systems"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306905149613696","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Remote sensing of backward reflection from stimulated axion decay"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306905625811200","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Experimental Search for Invisible Dark Matter Axions around \n<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mrow><mml:mn>22</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi mathvariant=\"normal\">μ</mml:mi><mml:mi>eV</mml:mi></mml:mrow></mml:math>"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306905625901696","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Extensive Search for Axion Dark Matter over 1 GHz with CAPP’S Main Axion Experiment"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306906074280576","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"More is different: multi-axion dynamics changes topological defect evolution"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306906076180480","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Opening a meV mass window for axionlike particles with a microwave-laser-mixed stimulated resonant photon collider"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306906076236416","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Undulators are ALP factories"}]},{"@id":"https://cir.nii.ac.jp/crid/1360565165203458432","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Topological defects and nano-Hz gravitational waves in aligned axion models"}]},{"@id":"https://cir.nii.ac.jp/crid/1360565165204278400","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion models with high scale inflation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360565166074826496","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Enhanced axion–photon coupling in GUT with hidden photon"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567181074498304","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Affleck-Dine leptogenesis with varying Peccei-Quinn scale"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567181088184320","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Peccei-Quinn extended gauge-mediation model with vector-like matter and 125 GeV Higgs"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567182396878848","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dark matter in axion landscape"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567184385876608","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cosmological constraints on spontaneous R-symmetry breaking models"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567184386550272","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Strongly broken Peccei-Quinn symmetry in the early Universe"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567184387273216","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Enhanced photon coupling of ALP dark matter adiabatically converted from the QCD axion"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567184387397888","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The Simons Observatory: science goals and forecasts"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567184977092480","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Possible roles of Peccei-Quinn symmetry in an effective low energy model"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567184980944640","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Affleck-Dine baryogenesis in the SUSY Dine-Fischler-Srednicki-Zhitnitsky axion model without<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mi>R</mml:mi></mml:math>parity"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567186092113280","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dark matter stability and one-loop neutrino mass generation based on Peccei–Quinn symmetry"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567186093520256","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"An extension of the SM based on effective Peccei–Quinn Symmetry"}]},{"@id":"https://cir.nii.ac.jp/crid/1360568465695105664","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Relaxing the cosmological moduli problem by low-scale inflation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360568469922187264","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Note on a solution to domain wall problem with the Lazarides-Shafi mechanism in axion dark matter models"}]},{"@id":"https://cir.nii.ac.jp/crid/1360568471112647680","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Proton decay and axion dark matter in SO(10) grand unification via minimal left–right symmetry"}]},{"@id":"https://cir.nii.ac.jp/crid/1360572092411677312","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion-radiation conversion by super and normal conductors"}]},{"@id":"https://cir.nii.ac.jp/crid/1360572092635689472","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Characterization of a flux-driven Josephson parametric amplifier with near quantum-limited added noise for axion search experiments"}]},{"@id":"https://cir.nii.ac.jp/crid/1360572092721253888","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Primordial black holes from QCD axion bubbles"}]},{"@id":"https://cir.nii.ac.jp/crid/1360572092784937088","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Probing axion dark matter with 21 cm fluctuations from minihalos"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118670665344","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion strings are superconducting"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118677636224","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Topological axion electrodynamics and 4-group symmetry"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118683512320","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A natural and simple UV completion of the QCD axion model"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118684481664","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cosmic Birefringence Triggered by Dark Matter Domination"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118700523904","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion cloud decay due to the axion–photon conversion with background magnetic fields"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118712301184","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion/hidden-photon dark matter conversion into condensed matter axion"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118726399360","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Strong CP problem and axion dark matter with small instantons"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118820562560","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Composite neutrinos and the QCD axion: Baryogenesis, dark matter, small Dirac neutrino masses, and vanishing neutron electric dipole moment"}]},{"@id":"https://cir.nii.ac.jp/crid/1360579814655892480","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cosmological effects of Peccei-Quinn symmetry breaking on QCD axion dark matter"}]},{"@id":"https://cir.nii.ac.jp/crid/1360579814655947264","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dark matter Axion search with riNg Cavity Experiment DANCE: Design and development of auxiliary cavity for simultaneous resonance of linear polarizations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580230589531648","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Searching for eV-mass axionlike particles with cross correlations between line intensity and weak lensing maps"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580230589742592","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Early dark energy by a dark Higgs field and axion-induced nonthermal trapping"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580232151564672","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Radiation burst by axion star collision with star in the Andromeda Galaxy"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584339752707712","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A way of determination of axion mass with quantum Hall effect"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584339778224128","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Gravitational wave production from axion rotations right after a transition to kination"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584340510970368","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Impact of multiple modes on the evolution of self-interacting axion condensate around rotating black holes"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584340510989440","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Quantum decay of scalar and vector boson stars and oscillons into gravitons"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584340512191872","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"First results of axion dark matter search with DANCE"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584343261516672","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Observational constraint on axion dark matter in a realistic halo profile with gravitational waves"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588379359563520","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Wormhole-induced ALP dark matter"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588379368371456","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Deci-Hz gravitational waves from the self-interacting axion cloud around a rotating stellar mass black hole"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588379387164544","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Thermal production of astrophobic axions"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588380160814976","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Probing long-lived axions at the KOTO experiment"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588380590637440","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion Detection with Quantum Hall Effect"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588381068274176","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Parameter Optimization of Josephson Parametric Amplifiers Using a Heuristic Search Algorithm for Axion Haloscope Search"}]},{"@id":"https://cir.nii.ac.jp/crid/1360846640179704192","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Quality of the Peccei-Quinn symmetry in the aligned QCD axion and cosmological implications"}]},{"@id":"https://cir.nii.ac.jp/crid/1360846642757925632","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cosmological solutions to the lithium problem: Big-bang nucleosynthesis with photon cooling, \n<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mi>X</mml:mi></mml:math>\n-particle decay and a primordial magnetic field"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848656054913024","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Supersymmetric flaxion"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848656063733376","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Topology in QCD and the axion abundance"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848656065312000","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Flavor-changing neutral-current decays in top-specific variant axion model"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848657371067392","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Flavor violating <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" altimg=\"si1.gif\" overflow=\"scroll\"><mml:msup><mml:mrow><mml:mi>Z</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math> from <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" altimg=\"si2.gif\" overflow=\"scroll\"><mml:mrow><mml:mi mathvariant=\"italic\">SO</mml:mi></mml:mrow><mml:mo stretchy=\"false\">(</mml:mo><mml:mn>10</mml:mn><mml:mo stretchy=\"false\">)</mml:mo></mml:math> SUSY GUT in High-Scale SUSY"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848657374739072","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion production from Landau quantization in the strong magnetic field of magnetars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848659362856064","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"More on cosmological constraints on spontaneous R-symmetry breaking models"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848659940035712","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Inflation from a supersymmetric axion model"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848659945340672","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Effective gravitational interactions of dark matter axions"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848659948849024","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Peccei-Quinn symmetry from dynamical supersymmetry breaking"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848659955822592","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"QCD axion window and low-scale inflation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848659957005952","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Muon \n<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mi>g</mml:mi><mml:mo>−</mml:mo><mml:mn>2</mml:mn></mml:math>\n and rare top decays in up-type specific variant axion models"}]},{"@id":"https://cir.nii.ac.jp/crid/1360849944284282496","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Vector coherent oscillation dark matter"}]},{"@id":"https://cir.nii.ac.jp/crid/1360853567413968896","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion star nucleation in dark minihalos around primordial black holes"}]},{"@id":"https://cir.nii.ac.jp/crid/1360853567413982848","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"New approach to neutrino masses and leptogenesis with Occam’s razor"}]},{"@id":"https://cir.nii.ac.jp/crid/1360853567441227904","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"QCD axion window and false vacuum Higgs inflation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360853567517783680","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Classification of discrete modular symmetries in type IIB flux vacua"}]},{"@id":"https://cir.nii.ac.jp/crid/1360853567712306432","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Detecting light boson dark matter through conversion into a magnon"}]},{"@id":"https://cir.nii.ac.jp/crid/1360853567712810112","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Light dark matter from inflaton decay"}]},{"@id":"https://cir.nii.ac.jp/crid/1360853567791787264","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Constraining the gravitational coupling of axion dark matter at LIGO"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593649431680","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cosmological perturbations for ultralight axionlike particles in a state of Bose-Einstein condensate"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593652690048","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion-CMB scenario in a supercooled universe"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593659878656","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Hidden photon and axion dark matter from symmetry breaking"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593660904704","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Trapping effect for QCD axion dark matter"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593661153152","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion dark matter search using arm cavity transmitted beams of gravitational wave detectors"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593689777920","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Inflation connected to the origin of \n<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:math>\n violation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593727848320","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Spectral-temporal features of repeating and one-off fast radio bursts and axion star"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593771928832","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Microlensing constraints on axion stars including finite lens and source size effects"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593817223808","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Electric current on surface of a metal/superconductor in axion/hidden-photon background"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857596726609408","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Radio signatures from encounters between neutron stars and QCD-axion minihalos around primordial black holes"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857758718225920","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"New scenario of QCD axion clump formation. Part I. Linear analysis"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861705566365568","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Formation of a chiral soliton lattice"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861705596160256","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Radio bounds on the mixed dark matter scenarios of primordial black holes and WIMPs"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861707123832960","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Detection of QCD axion dark matter by coherent scattering"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861707355793408","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion dark matter from first-order phase transition, and very high energy photons from GRB 221009A"}]},{"@id":"https://cir.nii.ac.jp/crid/1360865814728582784","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dynamics of superconformal axion: Quality and scalegenesis"}]},{"@id":"https://cir.nii.ac.jp/crid/1360865814733815552","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dissipation of axion energy via the Schwinger and Witten effects"}]},{"@id":"https://cir.nii.ac.jp/crid/1360865815503913984","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Design and Construction of a Variable-Angle Three-Beam Stimulated Resonant Photon Collider toward eV-Scale ALP Search"}]},{"@id":"https://cir.nii.ac.jp/crid/1360865815698141184","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Spin-2 dark matter from an anisotropic universe in bigravity"}]},{"@id":"https://cir.nii.ac.jp/crid/1360869854345549056","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Constraining ultralight ALP dark matter in light of cosmic birefringence"}]},{"@id":"https://cir.nii.ac.jp/crid/1360869854360610688","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Majoron-driven leptogenesis in gauged \n<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mi>U</mml:mi><mml:mo stretchy=\"false\">(</mml:mo><mml:mn>1</mml:mn><mml:msub><mml:mo stretchy=\"false\">)</mml:mo><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi>μ</mml:mi></mml:msub><mml:mo>−</mml:mo><mml:msub><mml:mi>L</mml:mi><mml:mi>τ</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math>\n model"}]},{"@id":"https://cir.nii.ac.jp/crid/1360869855564900480","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Axion cogenesis without isocurvature perturbations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360869855564910720","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cosmic stability of dark matter from Pauli blocking"}]},{"@id":"https://cir.nii.ac.jp/crid/1361131415656731264","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"QCD axion on hilltop by a phase shift of π."}]},{"@id":"https://cir.nii.ac.jp/crid/1361412894851598592","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Pati-Salam unification with a spontaneous \n<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:math>\n violation"}]},{"@id":"https://cir.nii.ac.jp/crid/2051151842044118912","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dark matter in the SO(5) × U(1) gauge-Higgs unification"}]},{"@id":"https://cir.nii.ac.jp/crid/2051151842060146304","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Detectable electric current induced by the dark matter axion in a conductor"}]},{"@id":"https://cir.nii.ac.jp/crid/2051151842060155904","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Global 4-group symmetry and 't Hooft anomalies in topological axion electrodynamics"}]},{"@id":"https://cir.nii.ac.jp/crid/2051996266988209920","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Classifying topological charge in SU(3) Yang–Mills theory with machine learning"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1016/0370-2693(83)90638-x"},{"@type":"CROSSREF","@value":"10.1007/jhep06(2014)162_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep01(2018)053_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep03(2017)122_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2016/08/056_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1093/ptep/ptu146_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.90.045001_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.91.125018_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.93.055022_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.98.075003_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevlett.116.051801_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2020.135861_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2020/03/007_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1093/ptep/ptaa138_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1140/epjc/s10052-021-09109-5_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevlett.126.121301_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep01(2021)152_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.102.072004_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.103.115004_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevlett.125.161806_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2021.136858_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep05(2021)043_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.104.055036_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1142/s0217732322500286_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1093/ptep/ptac058_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1093/ptep/ptab170_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep01(2023)145_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep07(2022)124_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.3390/universe9030123_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2022/09/062_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.105.115003_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1361-6471/ac841a_references_DOI_KBzUqTlwndjJW9EUgQixNpAqydT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2023.137891_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2023/06/049_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.107.123505_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2023/12/039_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.106.075011_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.108.036020_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.108.083525_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.108.063530_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.109.095012_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep09(2024)191_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2024/10/038_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/b978-0-32-395636-9.00012-8_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep01(2017)096_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2013/11/030_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.85.105020_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.88.075022_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.91.065014_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.93.085031_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep09(2016)021_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2015/11/003_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.87.085010_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.95.054502_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.97.035015_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1142/s2010194512004199_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.3389/fphy.2014.00060_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.dark.2020.100541_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2019/06/055_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.101.035029_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep10(2019)120_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.103.063508_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevlett.125.171301_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2020/05/004_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevlett.125.161801_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep03(2021)296_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.102.023522_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.102.103513_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1093/ptep/ptab150_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep09(2021)179_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.104.095010_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.104.123033_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep11(2021)082_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2021.136529_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep12(2021)108_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.105.023020_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep04(2022)113_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2021/09/004_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.105.102001_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.106.l081301_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.102.104003_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1142/s0217732323500165_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep11(2023)103_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevresearch.6.013200_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.107.123518_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.108.083518_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.109.035024_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2023/12/021_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2024/05/122_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevlett.134.051004_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.110.104038_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2024/05/085_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep09(2024)034_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevlett.133.051802_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevx.14.031023_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2025/04/002_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.110.092017_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.111.036020_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.107.103516_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep08(2016)044_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep11(2014)151_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.96.075039_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep02(2017)017_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep11(2012)158_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2013/04/043_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2015/10/010_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2018/10/042_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2019/02/056_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.96.115004_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.99.055035_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1140/epjc/s10052-018-5519-4_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1140/epjc/s10052-018-6370-3_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.101.075026_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1140/epjc/s10052-020-7922-x_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2018.03.070_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2018.03.039_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.nuclphysb.2020.115298_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1361-6668/abf23b_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2020/11/060_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.103.023521_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep06(2021)052_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2021.136762_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2021.136267_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevlett.127.181103_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1093/pasj/psab110_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep08(2021)074_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep07(2021)078_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.105.015024_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2022/03/026_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1742-6596/2156/1/012182_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.103.103014_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.107.063016_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1142/s0218271822500985_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2022.137089_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2023.138242_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.108.l081303_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2023/06/016_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2023/08/058_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.108.072005_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.107.103020_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep02(2025)183_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.110.044002_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep09(2024)136_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.108.055007_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1093/ptep/ptae076_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.3390/electronics13112127_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep06(2016)150_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2013/01/001_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.90.023001_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep04(2018)094_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep10(2015)136_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep11(2015)057_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2014/01/024_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1093/ptep/pty029_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.82.123531_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.89.065012_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.92.075003_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.98.015042_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.98.043535_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.98.095020_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep03(2020)011_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2018.04.056_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2019/10/019_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2015.12.075_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2016.12.034_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2015.08.043_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2018.05.014_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep04(2019)149_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.102.023013_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.102.055021_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep05(2020)154_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.101.106017_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.101.096013_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep03(2021)301_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.102.055013_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.103.123533_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.104.063525_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1007/jhep10(2021)026_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2021/05/062_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.104.062008_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.104.075034_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.104.043022_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.104.123012_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2022.136950_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2022/03/039_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1093/ptep/ptac044_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.106.096022_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1088/1475-7516/2022/08/004_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.105.095030_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2023.137824_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2024.138447_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.109.015014_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.3390/universe9080355_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.107.104007_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.110.103525_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.110.103510_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.111.075028_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.110.055009_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.110.075038_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.100.055019_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1103/physrevd.101.043505_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2015.12.043_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2018.01.084_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2015.04.020_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"},{"@type":"CROSSREF","@value":"10.1016/j.physletb.2018.04.024_references_DOI_IIoAP9BHOv3TocJpNBmLVAm2EtT"}]}