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The final result extends already known findings in the literature in several ways. First, it is an analytical function of both the space-like boundary coordinates; in other words, we keep track of what happens both along and transversely to the inter-quark axis. Then, we take into account the finiteness of the inter-quark distance and the first correction in the strong coupling expansion. To the same order, we also confirm the relation between the mass of the lightest glueball in the spectrum and the intrinsic width of the flux tube profile. We conclude by trying to gain some insights about the quantum fluctuations. Intriguingly, our proposal is in agreement with widespread expectations in the literature. En passant, we also derive a semi-analytical formula that gives the first correction to the scalar glueball masses in the strong coupling expansion."}],"arxiv_eprints":[{"categories":["hep-th","hep-lat"],"value":["10.1007/JHEP04(2026)002","2510.02442"]}],"authors":[{"affiliations":[{"country":"Italy","organization":"Università di Torino","value":"Dipartimento di Fisica, Università di Torino, Via Pietro Giuria 1, Torino, 10125, Italy"},{"country":"Italy","organization":"Istituto Nazionale di Fisica Nucleare, Sezione di Torino","value":"Istituto Nazionale di Fisica Nucleare, Sezione di Torino, Via Pietro Giuria 1, Torino, 10125, Italy"}],"email":null,"full_name":null,"given_names":"Tommaso","surname":"Canneti"}],"collections":[{"primary":"Journal of High Energy Physics"}],"control_number":106095,"copyright":[{"statement":"","holder":"The Author(s)","year":2026}],"dois":[{"value":"10.1007/JHEP04(2026)002"},{"value":"2510.02442"}],"imprints":[{"date":null,"publisher":"Springer"}],"license":[{"license":"CC-BY-4.0","url":"http://creativecommons.org/licenses/by/4.0/"}],"page_nr":[55],"publication_info":[{"artid":"JHEP04(2026)002","journal_issue":"4","journal_title":"Journal of High Energy Physics","journal_volume":"2026","page_end":"55","page_start":"1","year":"2026"}],"record_creation_date":"2026-04-02T18:56:19.994033","titles":[{"source":"Springer","title":"Flux tube profile from holography: finite size and strong coupling corrections"}]},"updated":"2026-04-02T18:56:25.738607+00:00","id":106095,"created":"2026-04-02T18:56:19.994033"},{"metadata":{"_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1007/JHEP04(2026)013/13130_2026_Article_28585.xml.scoap.xml","key":"13130_2026_Article_28585.xml.scoap","filetype":"xml"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1007/JHEP04(2026)013/13130_2026_Article_28585_a.pdf","key":"13130_2026_Article_28585_a","filetype":"pdf"}],"abstracts":[{"source":"Springer","value":"A line of first-order phase transitions is conjectured in the phase diagram of Quantum Chromodynamics at non-zero baryon density. If this is the case, numerical simulations of neutron star mergers suggest that various regions of the stars may cross this line multiple times. This results in the nucleation of bubbles of the preferred phase, which subsequently expand and collide. The resulting gravitational wave spectrum is highly sensitive to the velocity of the bubble walls. We use holography to perform the first microscopic simulation of bubble dynamics in a theory that qualitatively mirrors the expected phase diagram of Quantum Chromodynamics. We determine the wall velocity in the metastable regions and we compare it to theoretical estimates. 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Meanwhile, the type-I seesaw mechanism offers an elegant explanation for the lightness of the observed neutrino masses; however, its extremely heavy Majorana states place it far beyond experimental reach. Low-scale alternatives such as the inverse seesaw improve testability but typically lack a strong theoretical motivation. In this paper we bridge this gap by showing that gauging the discrete symmetry $\\textit{ℤ}$ × $\\textit{ℤ}$ — motivated by the internal structure of the Standard Model — naturally yields a QCD axion with a high-quality Peccei-Quinn symmetry solving the strong CP problem, while simultaneously enforcing the field content and hierarchy required for a natural inverse seesaw. The resulting model is highly predictive and has the potential to be fully tested by future experiments. Beyond addressing the strong CP problem and the origin of neutrino masses, our scenario also contains a viable dark-matter candidate and offers potential mechanisms for generating the baryon asymmetry of the Universe."}],"arxiv_eprints":[{"categories":["hep-ph"],"value":["10.1007/JHEP04(2026)004","2512.13158"]}],"authors":[{"affiliations":[{"country":"Japan","organization":"Kavli IPMU (WPI), UTIAS, University of Tokyo","value":"Kavli IPMU (WPI), UTIAS, University of Tokyo, Kashiwa, 277-8583, Japan"}],"email":null,"full_name":null,"given_names":"Yannis","surname":"Georis"},{"affiliations":[{"country":"Japan","organization":"Kavli IPMU (WPI), UTIAS, University of Tokyo","value":"Kavli IPMU (WPI), UTIAS, University of Tokyo, Kashiwa, 277-8583, Japan"}],"email":null,"full_name":null,"given_names":"Jie","surname":"Sheng"},{"affiliations":[{"country":"France","organization":"Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (UMR 9012), CNRS/IN2P3","value":"Pôle Théorie, Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (UMR 9012), CNRS/IN2P3, 15 Rue Georges Clemenceau, Orsay, 91400, France"}],"email":null,"full_name":null,"given_names":"Salvador","surname":"Urrea"},{"affiliations":[{"country":"China","organization":"Shanghai Jiao Tong University","value":"Tsung-Dao Lee Institute, Shanghai Jiao Tong University, Shanghai, 201210, China"},{"country":"Japan","organization":"Kavli IPMU (WPI), UTIAS, University of Tokyo","value":"Kavli IPMU (WPI), UTIAS, University of Tokyo, Kashiwa, 277-8583, Japan"}],"email":null,"full_name":null,"given_names":"Tsutomu","surname":"Yanagida"}],"collections":[{"primary":"Journal of High Energy Physics"}],"control_number":106091,"copyright":[{"statement":"","holder":"The Author(s)","year":2026}],"dois":[{"value":"10.1007/JHEP04(2026)004"},{"value":"2512.13158"}],"imprints":[{"date":null,"publisher":"Springer"}],"license":[{"license":"CC-BY-4.0","url":"http://creativecommons.org/licenses/by/4.0/"}],"page_nr":[16],"publication_info":[{"artid":"JHEP04(2026)004","journal_issue":"4","journal_title":"Journal of High Energy Physics","journal_volume":"2026","page_end":"16","page_start":"1","year":"2026"}],"record_creation_date":"2026-04-02T18:56:09.679061","titles":[{"source":"Springer","title":"Testable inverse seesaw motivated from a high quality QCD axion"}]},"updated":"2026-04-02T18:56:14.589344+00:00","id":106091,"created":"2026-04-02T18:56:09.679061"},{"metadata":{"_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1007/JHEP04(2026)014/13130_2026_Article_28586.xml.scoap.xml","key":"13130_2026_Article_28586.xml.scoap","filetype":"xml"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1007/JHEP04(2026)014/13130_2026_Article_28586_a.pdf","key":"13130_2026_Article_28586_a","filetype":"pdf"}],"abstracts":[{"source":"Springer","value":"In the context of entanglement in relativistic 2 → 2 scattering described by a perturbative $\\textit{S}$-matrix, we derive analytically the concurrence for a mixed final state of two qubits corresponding to a discrete quantum number of the scattered particles. The qubit density matrix is obtained by tracing the momentum degrees of freedom out of the full density matrix of the scattered system. Given an initial product state, the derived concurrence depends at the leading order on the real part of the inelastic forward amplitude and the initial state only. We also point out that the real part of the forward amplitude provides a subleading correction to the linearized entropy, reducing it by an amount that, for a computational-basis state, is equivalent to the relative entropy of coherence. We illustrate our findings with two examples of phenomenological interest: high-energy scattering of two scalar fields in the two-Higgs doublet model, and high-energy electron-positron annihilation."}],"arxiv_eprints":[{"categories":["hep-ph","hep-th","quant-ph"],"value":["10.1007/JHEP04(2026)014","2510.04200"]}],"authors":[{"affiliations":[{"country":"Poland","organization":"National Centre for Nuclear Research","value":"National Centre for Nuclear Research, Pasteura 7, Warsaw, 02-093, Poland"}],"email":null,"full_name":null,"given_names":"Kamila","surname":"Kowalska"},{"affiliations":[{"country":"Poland","organization":"National Centre for Nuclear Research","value":"National Centre for Nuclear Research, Pasteura 7, Warsaw, 02-093, Poland"}],"email":null,"full_name":null,"given_names":"Enrico","surname":"Sessolo"}],"collections":[{"primary":"Journal of High Energy Physics"}],"control_number":106086,"copyright":[{"statement":"","holder":"The Author(s)","year":2026}],"dois":[{"value":"10.1007/JHEP04(2026)014"},{"value":"2510.04200"}],"imprints":[{"date":null,"publisher":"Springer"}],"license":[{"license":"CC-BY-4.0","url":"http://creativecommons.org/licenses/by/4.0/"}],"page_nr":[27],"publication_info":[{"artid":"JHEP04(2026)014","journal_issue":"4","journal_title":"Journal of High Energy Physics","journal_volume":"2026","page_end":"27","page_start":"1","year":"2026"}],"record_creation_date":"2026-04-02T18:56:09.106893","titles":[{"source":"Springer","title":"Qubit entanglement from forward scattering"}]},"updated":"2026-04-02T18:56:12.682940+00:00","id":106086,"created":"2026-04-02T18:56:09.106893"},{"metadata":{"_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1007/JHEP04(2026)005/13130_2026_Article_28577.xml.scoap.xml","key":"13130_2026_Article_28577.xml.scoap","filetype":"xml"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1007/JHEP04(2026)005/13130_2026_Article_28577_a.pdf","key":"13130_2026_Article_28577_a","filetype":"pdf"}],"abstracts":[{"source":"Springer","value":"The associated production of a photon and a top-antitop quark pair $$ \\left(t\\overline{t}\\gamma \\right) $$ is important for measuring the top-quark charge and probing the top-photon interaction, and it requires improved theoretical predictions. We focus on the calculation of two-loop amplitudes for $$ t\\overline{t}\\gamma $$ production at hadron colliders. The infrared singularities with full top-quark mass dependence are derived from universal anomalous dimensions combined with one-loop massive amplitudes expanded to higher orders in the dimensional regulator $\\textit{ϵ}$. The finite remainders are approximated in the high-energy boosted limit using the mass-factorization formula. To validate our approach, we compare approximate one-loop amplitudes up to $$ \\mathcal{O}\\left({\\epsilon}^2\\right) $$ , as well as the two-loop infrared poles, against our exact results. The results in this paper serve as an important step toward next-to-next-to-leading order predictions for $$ t\\overline{t}\\gamma $$ production."}],"arxiv_eprints":[{"categories":["hep-ph"],"value":["10.1007/JHEP04(2026)005","2510.01774"]}],"authors":[{"affiliations":[{"country":"France","organization":"UMR 7589, Sorbonne Université et CNRS","value":"Laboratoire de Physique Théorique et Hautes Energies (LPTHE), UMR 7589, Sorbonne Université et CNRS, 4 place Jussieu, Paris Cedex 05, 75252, France"}],"email":null,"full_name":null,"given_names":"Guoxing","surname":"Wang"},{"affiliations":[{"country":"China","organization":"School of Physics, Zhejiang University","value":"Zhejiang Institute of Modern Physics, School of Physics, Zhejiang University, Hangzhou, 310027, China"}],"email":null,"full_name":null,"given_names":"Li","surname":"Yang"}],"collections":[{"primary":"Journal of High Energy Physics"}],"control_number":106094,"copyright":[{"statement":"","holder":"The Author(s)","year":2026}],"dois":[{"value":"10.1007/JHEP04(2026)005"},{"value":"2510.01774"}],"imprints":[{"date":null,"publisher":"Springer"}],"license":[{"license":"CC-BY-4.0","url":"http://creativecommons.org/licenses/by/4.0/"}],"page_nr":[31],"publication_info":[{"artid":"JHEP04(2026)005","journal_issue":"4","journal_title":"Journal of High Energy Physics","journal_volume":"2026","page_end":"31","page_start":"1","year":"2026"}],"record_creation_date":"2026-04-02T18:56:20.214889","titles":[{"source":"Springer","title":"Two-loop QCD amplitudes for $$ t\\overline{t}\\gamma $$ production at hadron colliders"}]},"updated":"2026-04-02T18:56:25.593800+00:00","id":106094,"created":"2026-04-02T18:56:20.214889"},{"metadata":{"_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1016/j.physletb.2026.140384/main.pdf","key":"main","filetype":"pdf"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1016/j.physletb.2026.140384/main.xml","key":"main","filetype":"xml"}],"abstracts":[{"source":"Elsevier","value":"The <italic>R</italic> <sup>2</sup> and the single-field-like regime of <italic>R</italic> <sup>2</sup>-Higgs inflation are disfavored by the observed high spectral index <italic>n<inf>s</inf></italic> from the combined cosmic microwave background (CMB) and baryon acoustic oscillation (BAO) measurements at the &#8239;&#8764;&#8239;2 <italic>&#963;</italic> level. The addition of a dimension-six <italic>R</italic> <sup>3</sup> term in the action helps alleviate this tension. We show that the parameter space accounting for the observed high <italic>n<inf>s</inf></italic> also induces rapid Goldstone and Higgs preheating. The preheating, especially from Goldstone modes, helps match the CMB and inflationary scales, which in turn supports the observed <italic>n<inf>s</inf></italic>."}],"arxiv_eprints":[{"categories":[],"value":["10.1016/j.physletb.2026.140384"]}],"authors":[{"affiliations":[{"country":"India","organization":"Department of Physical Sciences","value":"Department of Physical Sciences, Indian Institute of Science Education and Research Berhampur, Berhampur, 760003, India"}],"email":null,"full_name":null,"given_names":"Tanmoy","surname":"Modak"}],"collections":[{"primary":"Physics Letters B"}],"control_number":106115,"copyright":[{"statement":"The Authors","holder":"The Authors","year":2026}],"dois":[{"value":"10.1016/j.physletb.2026.140384"}],"imprints":[{"date":null,"publisher":"Elsevier"}],"license":[{"license":"CC-BY-3.0","url":"http://creativecommons.org/licenses/by/3.0/"}],"page_nr":[],"publication_info":[{"artid":"140384","journal_issue":"","journal_title":"Physics Letters B","journal_volume":"876 C","page_end":"","page_start":"","year":"2026"}],"record_creation_date":"2026-04-04T00:07:44.866263+00:00","titles":[{"source":"Elsevier","title":"Echoes of <italic>R</italic> <sup>3</sup> modification and Goldstone preheating in the CMB-BAO landscape"}]},"updated":"2026-04-04T12:26:55.299605+00:00","id":106115,"created":"2026-04-04T00:07:44.866263+00:00"},{"metadata":{"_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1140/epjc/s10052-026-15567-6/10052_2026_Article_15567.xml.Meta.xml","key":"10052_2026_Article_15567.xml.Meta","filetype":"xml"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1140/epjc/s10052-026-15567-6/10052_2026_Article_15567_a.pdf","key":"10052_2026_Article_15567_a","filetype":"pdf"}],"abstracts":[{"source":"Springer","value":"Relations between the kinematical tensors (the expansion, the shear, and the vorticity) and the polarization modes of gravitational waves are studied within the context of metric theories of gravity by considering freely falling test particles. After analyzing exact relations, we consider slowly moving particles under the influence of a weak gravitational field. Linearized plane waves of theories representative of those determined by a general second-order Lagrangian, including General Relativity, are shown to exemplify the following interconnections: between the transverse components of the shear and the transverse tensor polarization mode; between the expansion, and both the transverse scalar and the longitudinal polarization modes; and between the longitudinal-transverse components of both the shear and the vorticity, and the vector polarization mode. These relations, from the theoretical point of view, offer a novel insight into the interpretation of the polarization modes in terms of the kinematical tensors. 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For vacuum regions, we discuss the constancy of the nonmetricity scalar $\\textit{Q}$ and derive general vacuum solutions, which correspond effectively to Taub-(anti) de Sitter spacetimes with a cosmological constant determined by the specific $\\textit{f}$($\\textit{Q}$) model. By matching a singular thin shell source to the vacuum solutions, we relate the shell’s energy density and pressure to the integration constants of the exterior geometry. We also examine a finite-thickness slab as another matter source supporting the vacuum solution. Through numerical analysis of a quadratic model $$f(Q)=Q+\\alpha Q^2$$ with isotropic matter, we show that the maximum pressure inside the slab generally does not coincide with the geometric center. Moreover, a negative $$\\alpha $$ with larger magnitude leads to higher internal pressure and a thicker slab, while models with positive $$\\alpha $$ are incompatible with a self-gravitating slab of positive pressure."}],"arxiv_eprints":[{"categories":[],"value":["10.1140/epjc/s10052-026-15516-3"]}],"authors":[{"affiliations":[{"country":"China","organization":"Shanghai Normal University","value":"Division of Mathematics and Theoretical Physics, Shanghai Normal University, 100 Guilin Road, Shanghai, 200234, China"}],"email":null,"full_name":null,"given_names":"Jun-Qin","surname":"Long"},{"affiliations":[{"country":"China","organization":"Shanghai Normal University","value":"Division of Mathematics and Theoretical Physics, Shanghai Normal University, 100 Guilin Road, Shanghai, 200234, China"}],"email":null,"full_name":null,"given_names":"Rui-Hui","surname":"Lin"},{"affiliations":[{"country":"China","organization":"Shanghai Normal University","value":"Division of Mathematics and Theoretical Physics, Shanghai Normal University, 100 Guilin Road, Shanghai, 200234, China"}],"email":null,"full_name":null,"given_names":"Xiang-Hua","surname":"Zhai"}],"collections":[{"primary":"European Physical Journal C"}],"control_number":106028,"copyright":[{"statement":"","holder":"The Author(s)","year":2026}],"dois":[{"value":"10.1140/epjc/s10052-026-15516-3"}],"imprints":[{"date":null,"publisher":"Springer"}],"license":[{"license":"CC-BY-4.0","url":"http://creativecommons.org/licenses/by/4.0/"}],"page_nr":[10],"publication_info":[{"artid":"s10052-026-15516-3","journal_issue":"3","journal_title":"European Physical Journal C","journal_volume":"86","page_end":"10","page_start":"1","year":"2026"}],"record_creation_date":"2026-03-31T18:55:44.382056","titles":[{"source":"Springer","title":"Static plane symmetric solutions in $\\textit{f}$($\\textit{Q}$) gravity"}]},"updated":"2026-03-31T18:55:50.419935+00:00","id":106028,"created":"2026-03-31T18:55:44.382056"},{"metadata":{"_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1140/epjc/s10052-026-15519-0/10052_2026_Article_15519.xml.Meta.xml","key":"10052_2026_Article_15519.xml.Meta","filetype":"xml"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1140/epjc/s10052-026-15519-0/10052_2026_Article_15519_a.pdf","key":"10052_2026_Article_15519_a","filetype":"pdf"}],"abstracts":[{"source":"Springer","value":"Utilizing an emergent metric developed from deep learning techniques, we determine the complex potential associated with static quarkonium. This study explores the disintegration process of quarkonium by analyzing the real component of this potential, which is crucial for understanding its stability in various conditions. We show that the dissociation length, the critical distance at which a quark and antiquark pair disintegrate, decreases as the temperature increases. Furthermore, our assessment of the imaginary component of the potential indicates an increase in the magnitude of the imaginary potential for quarkonium as temperatures rise. This enhancement contributes to the quarkonium’s suppression within the quark-gluon plasma, mirroring the anticipated outcomes from QCD. Our findings not only confirm the theoretical predictions but also demonstrate the efficacy of deep learning methods in advancing our understanding of high-energy particle physics."}],"arxiv_eprints":[{"categories":[],"value":["10.1140/epjc/s10052-026-15519-0"]}],"authors":[{"affiliations":[{"country":"Iran","organization":"Shahrood University of Technology","value":"Faculty of Physics, Shahrood University of Technology, Shahrood, Iran"}],"email":null,"full_name":null,"given_names":"Mahdi","surname":"Mansouri"},{"affiliations":[{"country":"Iran","organization":"Shahrood University of Technology","value":"Faculty of Physics, Shahrood University of Technology, Shahrood, Iran"}],"email":null,"full_name":null,"given_names":"Kazem","surname":"Bitaghsir Fadafan"},{"affiliations":[{"country":"China","organization":"University of South China","value":"School of Nuclear Science and Technology, University of South China, Hengyang, 421001, China"}],"email":null,"full_name":null,"given_names":"Xun","surname":"Chen"}],"collections":[{"primary":"European Physical Journal C"}],"control_number":106026,"copyright":[{"statement":"","holder":"The Author(s)","year":2026}],"dois":[{"value":"10.1140/epjc/s10052-026-15519-0"}],"imprints":[{"date":null,"publisher":"Springer"}],"license":[{"license":"CC-BY-4.0","url":"http://creativecommons.org/licenses/by/4.0/"}],"page_nr":[11],"publication_info":[{"artid":"s10052-026-15519-0","journal_issue":"3","journal_title":"European Physical Journal C","journal_volume":"86","page_end":"11","page_start":"1","year":"2026"}],"record_creation_date":"2026-03-31T18:55:44.143484","titles":[{"source":"Springer","title":"Holographic complex potential of a quarkonium from deep learning"}]},"updated":"2026-03-31T18:55:50.425890+00:00","id":106026,"created":"2026-03-31T18:55:44.143484"},{"metadata":{"_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1140/epjc/s10052-026-15388-7/10052_2026_Article_15388.xml.Meta.xml","key":"10052_2026_Article_15388.xml.Meta","filetype":"xml"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1140/epjc/s10052-026-15388-7/10052_2026_Article_15388_a.pdf","key":"10052_2026_Article_15388_a","filetype":"pdf"}],"abstracts":[{"source":"Springer","value":"It is well known that torsion waves in teleparallel Einstein gravity may induce gravitational waves (GWs). In this paper we show that a modification to Holst gravity induces low-frequency torsion waves of torsional frequency $$\\sim {10^{12}Hz}= 1THz$$ as GWs sourced from astrophysical black holes. Of course, since here we use the almost Riemann-flat manifold approximation, there are no Riemannian GWs as in teleparallel spacetime but only torsionful gravitational waves. This result in Holst gravity allows us to determine an upper bound for the Barbero–Immirzi (BI) parameter as $$\\gamma<<<10^{-58}$$ , which agrees with the BI bound obtained by Aliberti and Lambiase by considering matter–anti-matter asymmetry in Holst gravity. Unfortunately, this very interesting result suffers from the usual torsion ambiguity. To remedy this situation, we proceed with the BI parameter promoted to a field ore BI scalarization. Again we find a BI parameter with a bound of $$10^{-58}$$ from a terahertz-frequency torsion wave. The BI parameter is promoted to a field, and with specific approximation one obtains a BI wave equation with a plane wave solution, similar to those obtained by Taveras and Yunes. From this wave equation constant the BI parameter implies zero torsion, and consequently general relativity (GR), but the converse is not true. Higgs field variation is regarded as responsible for massive torsion. This comes from an analogy between the Higgs field and BI scalar."}],"arxiv_eprints":[{"categories":[],"value":["10.1140/epjc/s10052-026-15388-7"]}],"authors":[{"affiliations":[{"country":"Brazil","organization":"IF-UERJ","value":"Departamento de Física Teórica, IF-UERJ, Rua São Francisco Xavier 524, Maracanã, Rio de Janeiro, RJ, 20550, Brazil"},{"country":"Croatia","organization":"Institute of Cosmology and Philosophy of Nature","value":"Institute of Cosmology and Philosophy of Nature, Krizževci, Croatia"},{"country":"China","organization":"Radioastronomy and technology LAB of Tianjin observary","value":"Radioastronomy and technology LAB of Tianjin observary, street of science 1 #150, urumqi city, People’s Republic of China"}],"email":null,"full_name":null,"given_names":"L.","surname":"Andrade"},{"affiliations":[{"country":"China","organization":"Astronomical Observatory of Chinese Academy of Sciences","value":"Astronomical Observatory of Chinese Academy of Sciences, Chaoyang, 100107, China"}],"email":null,"full_name":null,"given_names":"Zhi-fu","surname":"Gao"}],"collections":[{"primary":"European Physical Journal C"}],"control_number":106029,"copyright":[{"statement":"","holder":"The Author(s)","year":2026}],"dois":[{"value":"10.1140/epjc/s10052-026-15388-7"}],"imprints":[{"date":null,"publisher":"Springer"}],"license":[{"license":"CC-BY-4.0","url":"http://creativecommons.org/licenses/by/4.0/"}],"page_nr":[8],"publication_info":[{"artid":"s10052-026-15388-7","journal_issue":"3","journal_title":"European Physical Journal C","journal_volume":"86","page_end":"8","page_start":"1","year":"2026"}],"record_creation_date":"2026-03-31T18:55:44.336152","titles":[{"source":"Springer","title":"Torsion mass generation induced by Einstein–Cartan gravity with a Barbero–Immirzi Higgs field analogue"}]},"updated":"2026-03-31T18:55:50.469503+00:00","id":106029,"created":"2026-03-31T18:55:44.336152"}]}}