The first measurements of the top- and antitop-quark differential production cross sections and the top-quark charge asymmetry in the forward region are presented, using proton-proton collision data collected by the LHCb experiment at a center-of-mass energy of 13 TeV corresponding to an integrated luminosity of . The total production cross sections of top and antitop quarks are also determined. Measurements are performed using the final state within a fiducial region defined by -jet and pseudorapidity , with the muon from the -boson decay required to have and . The muon and -jet system must satisfy . The measured integrated production cross sections for the top and antitop quarks are , , where the first uncertainty is statistical, the second systematic, and the third accounts for the luminosity uncertainty. The top-quark charge asymmetry is measured to be , where the first uncertainty is statistical and the second is systematic. These results are consistent with next-to-leading order Standard Model predictions.
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Minamino","affiliations":[{"value":"Department of Physics, Yokohama National University, Yokohama, Kanagawa, 240-8501, Japan","organization":"Department of Physics, Yokohama National University, Yokohama, Kanagawa, 240-8501, Japan","country":{"code":"JP","name":"Japan"}}],"orcid":"0000-0001-6510-7106"},{"first_name":"Y.","last_name":"Sasaki","name":"Y. Sasaki","affiliations":[{"value":"Department of Physics, Yokohama National University, Yokohama, Kanagawa, 240-8501, Japan","organization":"Department of Physics, Yokohama National University, Yokohama, Kanagawa, 240-8501, Japan","country":{"code":"JP","name":"Japan"}}]},{"first_name":"R.","last_name":"Shibayama","name":"R. Shibayama","affiliations":[{"value":"Department of Physics, Yokohama National University, Yokohama, Kanagawa, 240-8501, Japan","organization":"Department of Physics, Yokohama National University, Yokohama, Kanagawa, 240-8501, Japan","country":{"code":"JP","name":"Japan"}}]},{"first_name":"R.","last_name":"Shimamura","name":"R. Shimamura","affiliations":[{"value":"Department of Physics, Yokohama National University, Yokohama, Kanagawa, 240-8501, Japan","organization":"Department of Physics, Yokohama National University, Yokohama, Kanagawa, 240-8501, Japan","country":{"code":"JP","name":"Japan"}}]}],"subtitle":"","related_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1103/yz79-h758/yz79-h758.pdf","created":"2026-06-01T18:00:27.750708+00:00","updated":"2026-06-01T18:00:27.750722+00:00"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1103/yz79-h758/yz79-h758.xml","created":"2026-06-01T18:00:27.754430+00:00","updated":"2026-06-01T18:00:27.754443+00:00"}],"article_identifiers":[{"identifier_type":"DOI","identifier_value":"10.1103/yz79-h758"},{"identifier_type":"arXiv","identifier_value":"2512.19887"}],"first_online_date":null,"publication_date":"2026-06-01","_updated_at":"2026-06-02T00:00:38.274773+00:00","doi":"10.1103/yz79-h758","publication_info":[{"journal_volume":"113","journal_issue":"11","journal_title":"Physical Review D","material":"article","page_start":"","page_end":"","artid":"","volume_year":"2026","journal_issue_date":null,"publisher":"APS"}],"abstract":"Super-Kamiokande (SK) has observed solar neutrino elastic scattering at recoil electron kinetic energies () as low as 3.49 MeV to study neutrino flavor conversion within the Sun. At SK-observable energies, these conversions are dominated by the Mikheyev-Smirnov-Wolfenstein effect. An upturn in the electron neutrino survival probability in which vacuum neutrino oscillations become dominant is predicted to occur at lower energies, but radioactive background increases exponentially with decreasing energy. New machine learning approaches provide substantial background reduction below 3.49 MeV such that statistical extraction of solar neutrino interactions becomes feasible. This article presents an analysis of the solar neutrino interaction rate at with the full SK-IV period, using data from a wideband intelligent trigger when available and with a boosted decision tree for event selection. A solar neutrino signal is observed between with significance and a data to unoscillated Monte Carlo ratio of . These additional low-energy data have a negligible effect on the intervals of the fits to the solar neutrino energy spectrum but have a noticeable effect on the best fit when using the exponential parametrization.
","acceptance_date":null,"reception_date":null,"related_materials":[],"countries":["JP","CN","GB","FR","US","CA","PL","ES","VN","KR","IT"],"id":107656,"title":"Measurement of the solar neutrino interaction rate below 3.49 MeV in Super-Kamiokande-IV","copyright":[{"statement":"Published by the American Physical Society","year":2026,"holder":""}],"_created_at":"2026-06-01T18:00:14.208043+00:00"},{"related_licenses":[{"url":"http://creativecommons.org/licenses/by/4.0/","name":"CC-BY-4.0"}],"article_arxiv_category":[{"category":"hep-ph","primary":true},{"category":"hep-th","primary":false}],"authors":[{"first_name":"Jorge David","last_name":"Castaño-Yepes","name":"Jorge David Castaño-Yepes","affiliations":[{"value":"Departamento de Física, Universidad del Valle, Ciudad Universitaria Meléndez, Santiago de Cali 760032, Colombia","organization":"Departamento de Física, Universidad del Valle, Ciudad Universitaria Meléndez, Santiago de Cali 760032, Colombia","country":{"code":"CO","name":"Colombia"},"ror":"00jb9vg53"}],"orcid":"0000-0002-8654-1304"},{"first_name":"Enrique","last_name":"Muñoz","name":"Enrique Muñoz","affiliations":[{"value":"Facultad de Física, Pontificia Universidad Católica de Chile, Vicuña Mackenna 4860, Santiago, Chile","organization":"Facultad de Física, Pontificia Universidad Católica de Chile, Vicuña Mackenna 4860, Santiago, Chile","country":{"code":"CL","name":"Chile"},"ror":"04teye511"},{"value":"Center for Nanotechnology and Advanced Materials CIEN-UC, Avenida Vicuña Mackenna 4860, Santiago, Chile","organization":"Center for Nanotechnology and Advanced Materials CIEN-UC, Avenida Vicuña Mackenna 4860, Santiago, Chile","country":{"code":"CL","name":"Chile"}}],"orcid":"0000-0003-4457-0817"}],"subtitle":"","related_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1103/fkfs-nlbm/fkfs-nlbm.pdf","created":"2026-06-01T18:00:27.609159+00:00","updated":"2026-06-01T18:00:27.609169+00:00"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1103/fkfs-nlbm/fkfs-nlbm.xml","created":"2026-06-01T18:00:27.612197+00:00","updated":"2026-06-01T18:00:27.612205+00:00"}],"article_identifiers":[{"identifier_type":"DOI","identifier_value":"10.1103/fkfs-nlbm"},{"identifier_type":"arXiv","identifier_value":"2509.18219"}],"first_online_date":null,"publication_date":"2026-06-01","_updated_at":"2026-06-02T00:00:34.600843+00:00","doi":"10.1103/fkfs-nlbm","publication_info":[{"journal_volume":"113","journal_issue":"11","journal_title":"Physical Review D","material":"article","page_start":"","page_end":"","artid":"","volume_year":"2026","journal_issue_date":null,"publisher":"APS"}],"abstract":"We investigate dilepton production in a thermalized quark-gluon plasma subject to global rotation, in the rigid rotating approximation. We consider a generic process involving quark-antiquark annihilation followed by the emission of a highly energetic virtual photon decaying into a dilepton pair. For this process, we compute the dilepton emission rate from the imaginary part of the photon polarization tensor, at finite temperature and vorticity. Our results show that vorticity induces characteristic modifications in the light dilepton channel, namely, production, where the emission spectrum exhibits a suppression at low transverse mass together with a mild shift of the production threshold. This behavior originates from the role of vorticity as an effective spin-dependent chemical potential that alters the available phase-space distribution for the emission process. In contrast, the channel is more weakly affected by the rotational background, thus remaining dominated by its intrinsic mass threshold. The resulting channel dependence highlights a potential phenomenological handle for disentangling rotational effects in heavy-ion collisions: while light dilepton spectra encode the imprints of vorticity in the infrared sector, the muon channel provides a comparatively robust baseline.
","acceptance_date":null,"reception_date":null,"related_materials":[],"countries":["CO","CL"],"id":107655,"title":"Dilepton production in a rotating thermal medium: The rigid rotation approximation","copyright":[{"statement":"Published by the American Physical Society","year":2026,"holder":""}],"_created_at":"2026-06-01T18:00:14.092190+00:00"},{"related_licenses":[{"url":"http://creativecommons.org/licenses/by/4.0/","name":"CC-BY-4.0"}],"article_arxiv_category":[{"category":"hep-ph","primary":true},{"category":"hep-th","primary":false},{"category":"nucl-th","primary":false}],"authors":[{"first_name":"Francesco","last_name":"Giacosa","name":"Francesco Giacosa","affiliations":[{"value":"Institute of Physics, Jan Kochanowski University, ulica Uniwersytecka 7, Kielce, Poland and Institute for Theoretical Physics, J. W. Goethe University, Max-von-Laue-Straße 1, Frankfurt, Germany","organization":"Institute of Physics, Jan Kochanowski University, ulica Uniwersytecka 7, Kielce, Poland and Institute for Theoretical Physics, J. W. Goethe University, Max-von-Laue-Straße 1, Frankfurt, Germany","country":{"code":"DE","name":"Germany"},"ror":"04cvxnb49"}],"orcid":"0000-0002-7290-9366"},{"first_name":"Vanamali","last_name":"Shastry","name":"Vanamali Shastry","affiliations":[{"value":"Center for Exploration of Energy and Matter, Indiana University, Bloomington, Indiana 47403, USA and Department of Physics, Indiana University, Bloomington, Indiana 47405, USA","organization":"Center for Exploration of Energy and Matter, Indiana University, Bloomington, Indiana 47403, USA and Department of Physics, Indiana University, Bloomington, Indiana 47405, USA","country":{"code":"US","name":"United States"},"ror":"02k40bc56"}],"orcid":"0000-0003-1296-8468"}],"subtitle":"","related_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1103/24fy-h8fp/24fy-h8fp.pdf","created":"2026-06-01T18:00:26.543371+00:00","updated":"2026-06-01T18:00:26.543385+00:00"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1103/24fy-h8fp/24fy-h8fp.xml","created":"2026-06-01T18:00:26.547669+00:00","updated":"2026-06-01T18:00:26.547683+00:00"}],"article_identifiers":[{"identifier_type":"DOI","identifier_value":"10.1103/24fy-h8fp"},{"identifier_type":"arXiv","identifier_value":"2507.03145"}],"first_online_date":null,"publication_date":"2026-06-01","_updated_at":"2026-06-02T00:00:34.303506+00:00","doi":"10.1103/24fy-h8fp","publication_info":[{"journal_volume":"113","journal_issue":"11","journal_title":"Physical Review D","material":"article","page_start":"","page_end":"","artid":"","volume_year":"2026","journal_issue_date":null,"publisher":"APS"}],"abstract":"Unstable states that live long enough may appear as in(out)going particles in scattering experiments. Yet, the standard QFT approach strictly applies only to fully stable asymptotic states. This is evident when scattering involving unstable particles develops a -channel singularity at specific angles. We employ a finite-time formalism leading to analytic results without the singularity (even in the infinite-time limit), thus solving the problem at a phenomenological level. In turn, the approach also justifies treating long-lived particles, like weakly decaying pions, as stable during strong interactions.
","acceptance_date":null,"reception_date":null,"related_materials":[],"countries":["DE","US"],"id":107653,"title":"Scattering off unstable states","copyright":[{"statement":"Published by the American Physical Society","year":2026,"holder":""}],"_created_at":"2026-06-01T18:00:14.063289+00:00"},{"related_licenses":[{"url":"http://creativecommons.org/licenses/by/4.0/","name":"CC-BY-4.0"}],"article_arxiv_category":[{"category":"hep-ph","primary":true},{"category":"astro-ph.CO","primary":false},{"category":"hep-th","primary":false}],"authors":[{"first_name":"Sarunas","last_name":"Verner","name":"Sarunas Verner","affiliations":[{"value":"Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, Illinois 60637, USA","organization":"Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, Illinois 60637, USA","country":{"code":"US","name":"United States"},"ror":"024mw5h28"}],"orcid":"0000-0003-4870-0826"}],"subtitle":"","related_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1103/3st2-jhx5/3st2-jhx5.pdf","created":"2026-06-01T18:00:26.526405+00:00","updated":"2026-06-01T18:00:26.526415+00:00"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1103/3st2-jhx5/3st2-jhx5.xml","created":"2026-06-01T18:00:26.529441+00:00","updated":"2026-06-01T18:00:26.529448+00:00"}],"article_identifiers":[{"identifier_type":"DOI","identifier_value":"10.1103/3st2-jhx5"},{"identifier_type":"arXiv","identifier_value":"2512.19041"}],"first_online_date":null,"publication_date":"2026-06-01","_updated_at":"2026-06-02T00:00:32.834462+00:00","doi":"10.1103/3st2-jhx5","publication_info":[{"journal_volume":"113","journal_issue":"12","journal_title":"Physical Review D","material":"article","page_start":"","page_end":"","artid":"","volume_year":"2026","journal_issue_date":null,"publisher":"APS"}],"abstract":"We study the minimal gravitational portal for a massive spin-2 dark matter candidate produced during perturbative reheating. The dark sector couples to the visible sector only via gravity, and we analyze two unavoidable channels: (i) inflaton condensate annihilation, , and (ii) thermal scatterings, , both mediated by graviton exchange. Working in the Fierz-Pauli framework for a free massive spin-2 field of mass , we derive the graviton-mediated amplitudes and perform a full helicity decomposition of the final state. The relic abundance is obtained analytically in terms of and the reheating temperature . In the light mass regime (with the inflaton mass during oscillations), production is overwhelmingly dominated by the longitudinal (helicity-0) mode: the cross section is parametrically enhanced, scaling as , and yields efficient dark matter production despite purely gravitational couplings. Compared to lower-spin cases (spin-0, , 1, and ), massive spin-2 production is substantially more efficient for the same reheating history. Over most of the parameter space the inflaton condensate channel dominates the yield, while the thermal contribution is negligible. Avoiding overproduction typically requires either a relatively low or a spin-2 mass near threshold, . This places the spin-2 portal on similar footing to other higher spins in reheating scenarios, while emphasizing the central role of the helicity-0 mode and the reheating history in setting the dark matter density.
","acceptance_date":null,"reception_date":null,"related_materials":[],"countries":["US"],"id":107652,"title":"Gravitational production of massive spin-2 particles during reheating","copyright":[{"statement":"Published by the American Physical Society","year":2026,"holder":""}],"_created_at":"2026-06-01T18:00:14.358380+00:00"},{"related_licenses":[{"url":"http://creativecommons.org/licenses/by/4.0/","name":"CC-BY-4.0"}],"article_arxiv_category":[{"category":"hep-th","primary":true},{"category":"cond-mat.stat-mech","primary":false}],"authors":[{"first_name":"Runzhe","last_name":"Hu","name":"Runzhe Hu","affiliations":[{"value":"School of Physics, Sun Yat-Sen University, Guangzhou 510275, China","organization":"School of Physics, Sun Yat-Sen University, Guangzhou 510275, China","country":{"code":"CN","name":"China"},"ror":"0064kty71"}],"orcid":"0009-0006-8908-7537"},{"first_name":"Wenliang","last_name":"Li","name":"Wenliang Li","affiliations":[{"value":"School of Physics, Sun Yat-Sen University, Guangzhou 510275, China","organization":"School of Physics, Sun Yat-Sen University, Guangzhou 510275, China","country":{"code":"CN","name":"China"},"ror":"0064kty71"}],"orcid":"0000-0002-0217-5037"}],"subtitle":"","related_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1103/hnd3-636j/hnd3-636j.pdf","created":"2026-06-01T18:00:27.153828+00:00","updated":"2026-06-01T18:00:27.153836+00:00"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1103/hnd3-636j/hnd3-636j.xml","created":"2026-06-01T18:00:27.156191+00:00","updated":"2026-06-01T18:00:27.156198+00:00"}],"article_identifiers":[{"identifier_type":"DOI","identifier_value":"10.1103/hnd3-636j"},{"identifier_type":"arXiv","identifier_value":"2508.20854"}],"first_online_date":null,"publication_date":"2026-06-01","_updated_at":"2026-06-02T00:00:32.579379+00:00","doi":"10.1103/hnd3-636j","publication_info":[{"journal_volume":"136","journal_issue":"22","journal_title":"Physical Review Letters","material":"article","page_start":"","page_end":"","artid":"","volume_year":"2026","journal_issue_date":null,"publisher":"APS"}],"abstract":"The three-dimensional classical model with a boundary has received renewed interest due to the discovery of the extraordinary-log boundary universality class for . The critical value and the exponent of the boundary correlation function are related to certain amplitudes in the normal universality class. To determine their precise values, we revisit the 3D boundary conformal field theory for , 2, 3, 4, 5. After substantially improving the accuracy of the boundary bootstrap, our determinations are in excellent agreement with the Monte Carlo results, resolving the previous discrepancies due to low truncation orders. We also use the recent bulk bootstrap results to deduce highly accurate Ising data. Many bulk and boundary predictions are obtained for the first time. Our results demonstrate the great potential of the minimization method for many unexplored bootstrap problems in which positivity constraints are absent.
","acceptance_date":null,"reception_date":null,"related_materials":[],"countries":["CN"],"id":107654,"title":"Accurate Boundary Bootstrap for the Three-Dimensional Normal Universality Class","copyright":[{"statement":"Published by the American Physical Society","year":2026,"holder":""}],"_created_at":"2026-06-01T18:00:14.152698+00:00"},{"related_licenses":[{"url":"http://creativecommons.org/licenses/by/4.0/","name":"CC-BY-4.0"}],"article_arxiv_category":[],"authors":[{"first_name":"Nurmukhammed","last_name":"Aytimbetov","name":"Nurmukhammed Aytimbetov","affiliations":[{"value":"Namangan, Boburshokh 161, Namangan, 160107, Uzbekistan","organization":"Namangan","country":{"code":"UZ","name":"Uzbekistan"}}],"orcid":"0009-0008-9921-5576"},{"first_name":"Reggie","last_name":"Pantig","name":"Reggie Pantig","affiliations":[{"value":"Physics Department, School of Foundational Studies and Education, Mapúa University, 658 Muralla St., Intramuros, Manila, 1002, Philippines","organization":"Mapúa University","country":{"code":"PH","name":"Philippines"},"ror":"040rd2b57"}],"orcid":"0000-0002-3101-8591"},{"first_name":"Ali","last_name":"Övgün","name":"Ali Övgün","affiliations":[{"value":"Physics Department, Eastern Mediterranean University, Via Mersin 10, Famagusta, North Cyprus, 99628, Turkey","organization":"Eastern Mediterranean University","country":{"code":"TR","name":"Türkiye"},"ror":"00excyz84"}],"orcid":"0000-0002-9889-342X"},{"first_name":"Bobomurat","last_name":"Ahmedov","name":"Bobomurat Ahmedov","affiliations":[{"value":"School of Physics, Harbin Institute of Technology, Harbin, 150001, People’s Republic of China","organization":"Harbin Institute of Technology","country":{"code":"CN","name":"China"},"ror":"01yqg2h08"},{"value":"Institute for Advanced Studies, New Uzbekistan University, Movarounnahr str. 1, Tashkent, 100000, Uzbekistan","organization":"New Uzbekistan University","country":{"code":"UZ","name":"Uzbekistan"},"ror":"035v3tr79"},{"value":"Institute of Theoretical Physics, National University of Uzbekistan, Movarounnahr Str. 1, Tashkent, 100174, Uzbekistan","organization":"Institute of Theoretical Physics, National University of Uzbekistan","country":{"code":"UZ","name":"Uzbekistan"},"ror":"011647w73"}],"orcid":"0000-0002-1232-610X"},{"first_name":"Javlon","last_name":"Rayimbaev","name":"Javlon Rayimbaev","affiliations":[{"value":"Kimyo International University in Tashkent, Shota Rustaveli Street 156, Tashkent, 100121, Uzbekistan","organization":"Kimyo International University in Tashkent","country":{"code":"UZ","name":"Uzbekistan"},"ror":"05jfh7098"},{"value":"University of Tashkent for Applied Sciences, Gavhar Str. 1, Tashkent, 700127, Uzbekistan","organization":"University of Tashkent for Applied Sciences","country":{"code":"UZ","name":"Uzbekistan"},"ror":"02erf0j28"}],"orcid":"0000-0001-9293-1838"}],"subtitle":"","related_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1140/epjc/s10052-026-15805-x/10052_2026_Article_15805.xml.Meta.xml","created":"2026-06-01T18:55:36.126067+00:00","updated":"2026-06-01T18:55:36.126076+00:00"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1140/epjc/s10052-026-15805-x/10052_2026_Article_15805_a.pdf","created":"2026-06-01T18:55:36.129074+00:00","updated":"2026-06-01T18:55:36.129082+00:00"}],"article_identifiers":[{"identifier_type":"DOI","identifier_value":"10.1140/epjc/s10052-026-15805-x"}],"first_online_date":null,"publication_date":"2026-06-01","_updated_at":"2026-06-01T18:55:36.311612+00:00","doi":"10.1140/epjc/s10052-026-15805-x","publication_info":[{"journal_volume":"86","journal_issue":"6","journal_title":"European Physical Journal C","material":"article","page_start":"1","page_end":"14","artid":"s10052-026-15805-x","volume_year":"2026","journal_issue_date":null,"publisher":"Springer"}],"abstract":"We investigate Josephson phenomena in a slowly rotating, stationary spacetime, emphasizing the distinct roles of gravitational redshift and rotational frame-dragging, motivated by [ ]. Using a covariant formulation based on gauge-invariant phase dynamics and conserved currents within a $$3+1$$ decomposition, we analyze both AC and DC Josephson effects and interferometric configurations. Restricting attention to linear order in the rotation parameter $\\textit{a}$, and working in the Eulerian/ZAMO frame, we show that in the slow-rotation slicing adopted here the lapse function agrees with its static (Schwarzschild-type) form up to $$\\mathcal {O}(a^2)$$ , while rotational effects enter through the shift vector. Consequently, redshift effects on Josephson frequencies and DC critical currents remain unchanged relative to the non-rotating case at $$\\mathcal {O}(a)$$ . The AC Josephson relation retains its redshifted structure when expressed in terms of proper voltages and reduces to the standard flat-spacetime form when formulated in terms of asymptotic (Killing-time) observables. Likewise, the DC critical current measured at infinity scales with a single power of the lapse function and is unaffected by rotation at linear order in the absence of azimuthal condensate momentum. Rotational effects become relevant only in configurations that are sensitive to spatial phase transport or to synchronization with the global time coordinate. In particular, RF-driven interferometric setups can acquire Sagnac-type phase offsets associated with frame dragging, whereas the DC fluxoid constraint remains unshifted at linear order in the present approximation. Our results provide a clean separation between lapse-driven redshift effects and shift-driven rotational contributions in Josephson physics and furnish a consistent framework for superconducting circuits in stationary spacetimes.","acceptance_date":null,"reception_date":null,"related_materials":[],"countries":["PH","CN","UZ","TR"],"id":107660,"title":"Josephson effects in slowly rotating spacetimes","copyright":[{"statement":"","year":2026,"holder":"The Author(s)"}],"_created_at":"2026-06-01T18:55:31.409583"},{"related_licenses":[{"url":"http://creativecommons.org/licenses/by/4.0/","name":"CC-BY-4.0"}],"article_arxiv_category":[],"authors":[{"first_name":"F.","last_name":"Minotti","name":"F. Minotti","affiliations":[{"value":"Departamento de Física, Universidad de Buenos Aires, Facultad de Ciencias Exactas y Naturales, Buenos Aires, Argentina","organization":"Universidad de Buenos Aires, Facultad de Ciencias Exactas y Naturales","country":{"code":"AR","name":"Argentina"},"ror":"0081fs513"},{"value":"Instituto de Física Interdisciplinaria y Aplicada (INFINA), CONICET-Universidad de Buenos Aires, Buenos Aires, Argentina","organization":"CONICET-Universidad de Buenos Aires","country":{"code":"AR","name":"Argentina"},"ror":"0081fs513"}],"orcid":"0000-0003-0577-9589"},{"first_name":"G.","last_name":"Modanese","name":"G. Modanese","affiliations":[{"value":"Free University of Bozen-Bolzano, Faculty of Engineering, Bolzano, 39100, Italy","organization":"Free University of Bozen-Bolzano, Faculty of Engineering","country":{"code":"IT","name":"Italy"},"ror":"012ajp527"}],"orcid":"0000-0003-4302-2966"}],"subtitle":"","related_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1140/epjc/s10052-026-15825-7/10052_2026_Article_15825.xml.Meta.xml","created":"2026-06-01T18:55:36.219965+00:00","updated":"2026-06-01T18:55:36.219974+00:00"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1140/epjc/s10052-026-15825-7/10052_2026_Article_15825_a.pdf","created":"2026-06-01T18:55:36.223108+00:00","updated":"2026-06-01T18:55:36.223117+00:00"}],"article_identifiers":[{"identifier_type":"DOI","identifier_value":"10.1140/epjc/s10052-026-15825-7"}],"first_online_date":null,"publication_date":"2026-06-01","_updated_at":"2026-06-01T18:55:36.285189+00:00","doi":"10.1140/epjc/s10052-026-15825-7","publication_info":[{"journal_volume":"86","journal_issue":"6","journal_title":"European Physical Journal C","material":"article","page_start":"1","page_end":"17","artid":"s10052-026-15825-7","volume_year":"2026","journal_issue_date":null,"publisher":"Springer"}],"abstract":"We study a scalar–tensor extension of gravity with two scalar fields coupled to the Aharonov–Bohm extension of electrodynamics, where the scalar mode $$S\\equiv \\partial _\\mu A^\\mu $$ is dynamical. In this framework the trace of the electromagnetic energy–momentum tensor is nonvanishing and the scalar $\\textit{S}$ induces an electro-gravitational coupling that can be enhanced by the vacuum expectation value of the second gravitational scalar. For bosonic matter described by a macroscopic wavefunction (as in superconductors), the coupling to the electromagnetic potential generates $\\textit{S}$ already at the semiclassical level, implying sizable junction-induced discontinuities. Including the scalar–tensor sector yields a nonlinear system for $\\textit{S}$ and a gravitational scalar combination $$\\beta $$ that admits a bulk saturation solution $$S_\\textrm{sat}^2=(\\Lambda \\lambda _L^2)^{-1}$$ and a corresponding threshold condition for macroscopic effects. We apply these results to pulsed discharges across normal-superconducting junctions and obtain scaling relations for the onset of anomalous gravitational signals in terms of current density, pulse duration, and superconducting volume, consistent with reported threshold behavior in two independent experimental configurations for a single microscopic parameter. We also present time-dependent propagating solutions in the weak-field regime and derive a class of one-dimensional traveling exact solutions of the nonlinear vacuum Einstein equations.","acceptance_date":null,"reception_date":null,"related_materials":[],"countries":["AR","IT"],"id":107661,"title":"Scalar–tensor gravity and Aharonov–Bohm electrodynamics with bosons: applications to superconductors","copyright":[{"statement":"","year":2026,"holder":"The Author(s)"}],"_created_at":"2026-06-01T18:55:31.390068"},{"related_licenses":[{"url":"http://creativecommons.org/licenses/by/4.0/","name":"CC-BY-4.0"}],"article_arxiv_category":[{"category":"hep-ph","primary":true}],"authors":[{"first_name":"Swarup","last_name":"Sangiri","name":"Swarup Sangiri","affiliations":[{"value":"Physics Department, Indian Institute of Technology Kharagpur, Kharagpur, 721302, India","organization":"Indian Institute of Technology Kharagpur","country":{"code":"IN","name":"India"},"ror":"03w5sq511"}],"orcid":"0000-0002-2656-1012"}],"subtitle":"","related_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1140/epjc/s10052-026-15853-3/10052_2026_Article_15853.xml.Meta.xml","created":"2026-06-01T18:55:36.012023+00:00","updated":"2026-06-01T18:55:36.012038+00:00"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1140/epjc/s10052-026-15853-3/10052_2026_Article_15853_a.pdf","created":"2026-06-01T18:55:36.016176+00:00","updated":"2026-06-01T18:55:36.016190+00:00"}],"article_identifiers":[{"identifier_type":"DOI","identifier_value":"10.1140/epjc/s10052-026-15853-3"},{"identifier_type":"arXiv","identifier_value":"2603.29976"}],"first_online_date":null,"publication_date":"2026-06-01","_updated_at":"2026-06-01T18:55:36.072538+00:00","doi":"10.1140/epjc/s10052-026-15853-3","publication_info":[{"journal_volume":"86","journal_issue":"6","journal_title":"European Physical Journal C","material":"article","page_start":"1","page_end":"12","artid":"s10052-026-15853-3","volume_year":"2026","journal_issue_date":null,"publisher":"Springer"}],"abstract":"Bargmann invariants provide a rephasing-invariant description of phase relations among quantum states and offer a geometric perspective on interference phenomena. In this work, we investigate their role in neutral meson systems by constructing cyclic products involving the heavy and light mass eigenstates together with decay-projected states arising from correlated meson decays. Explicit expressions for third-order and fourth-order invariants are obtained in terms of mixing parameters and decay amplitudes. The analysis shows that the associated geometric phases encode $$\\mathcal CP$$ -sensitive interference effects between meson–antimeson mixing and decay amplitudes and become trivial in the $$\\mathcal CP$$ -conserving limit. Expressing the decay amplitudes in terms of CKM matrix elements reveals quartic combinations with analogous rephasing-invariant weak-phase structure to that of the Jarlskog invariant. We further introduce a rephasing-invariant ratio constructed from third- and fourth-order Bargmann invariants, which isolates correlated $$\\mathcal CP$$ -violating structures that cannot, in general, be factorized into independent decay-channel contributions and can enhance sensitivity to small deviations from $$\\mathcal CP$$ symmetry. The invariants can also be related to parameters governing time-dependent $$\\mathcal CP$$ asymmetries in neutral meson decays, thereby providing a geometric interpretation of observable $$\\mathcal CP$$ -violating interference effects.","acceptance_date":null,"reception_date":null,"related_materials":[],"countries":["IN"],"id":107659,"title":"Bargmann invariants and correlated geometric $$\\mathcal CP$$ -violating structures in neutral meson systems","copyright":[{"statement":"","year":2026,"holder":"The Author(s)"}],"_created_at":"2026-06-01T18:55:31.386668"},{"related_licenses":[{"url":"http://creativecommons.org/licenses/by/4.0/","name":"CC-BY-4.0"}],"article_arxiv_category":[{"category":"gr-qc","primary":true}],"authors":[{"first_name":"Jie","last_name":"Zhu","name":"Jie Zhu","affiliations":[{"value":"Department of Physics, Chongqing Key Laboratory for Strongly Coupled Physics, Chongqing University, Chongqing, 401331, People’s Republic of China","organization":"Chongqing University","country":{"code":"CN","name":"China"},"ror":"023rhb549"}],"orcid":"0000-0002-9733-2460"},{"first_name":"Hao","last_name":"Li","name":"Hao Li","affiliations":[{"value":"Department of Physics, Chongqing Key Laboratory for Strongly Coupled Physics, Chongqing University, Chongqing, 401331, People’s Republic of China","organization":"Chongqing University","country":{"code":"CN","name":"China"},"ror":"023rhb549"}],"orcid":"0000-0002-2971-4539"}],"subtitle":"","related_files":[{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1140/epjc/s10052-026-15793-y/10052_2026_Article_15793.xml.Meta.xml","created":"2026-06-01T18:55:35.925112+00:00","updated":"2026-06-01T18:55:35.925128+00:00"},{"file":"https://scoap3-prod-backend.s3.cern.ch/media/harvested_files/10.1140/epjc/s10052-026-15793-y/10052_2026_Article_15793_a.pdf","created":"2026-06-01T18:55:35.939101+00:00","updated":"2026-06-01T18:55:35.939121+00:00"}],"article_identifiers":[{"identifier_type":"DOI","identifier_value":"10.1140/epjc/s10052-026-15793-y"},{"identifier_type":"arXiv","identifier_value":"2601.05750"}],"first_online_date":null,"publication_date":"2026-06-01","_updated_at":"2026-06-01T18:55:36.011539+00:00","doi":"10.1140/epjc/s10052-026-15793-y","publication_info":[{"journal_volume":"86","journal_issue":"6","journal_title":"European Physical Journal C","material":"article","page_start":"1","page_end":"19","artid":"s10052-026-15793-y","volume_year":"2026","journal_issue_date":null,"publisher":"Springer"}],"abstract":"This work systematically investigates the post-Newtonian behavior of general quadratic gravity in the weak-field regime. By extending the Einstein–Hilbert action to include quadratic curvature terms as $$\\mathcal {L}\\propto R-\\lambda C^2+\\mu R^2$$ , the theory introduces two massive modes: a scalar mode and a ghost tensor mode. Using the post-Newtonian expansion method, we derive the explicit expressions for the metric for a general source up to 1.5PN order. Furthermore, for a point-mass source, we extend the solution to 2PN order and evaluate the effective parameterized post-Newtonian parameters $$\\gamma (r)$$ and $$\\beta (r)$$ . The results show that deviations from General Relativity are exponentially suppressed. The theory has the feature $$\\gamma (r)\\equiv 1$$ when $$m_R=m_W$$ , and to ensure that gravity remains attractive, we have $$m_W>m_R/4$$ . At short distance scales, the Newtonian potential no longer exhibits a 1/$\\textit{r}$ behavior, but instead displays a polynomial dependence on $\\textit{r}$. The leading correction to $$\\beta (r)$$ exhibiting a characteristic $$\\mathcal {O}(r \\ln (r)e^{-mr})$$ dependence. Based on the Solar System experiments, we derive preliminary constraints on the theory’s parameters: $$m_R,m_W\\gtrsim 23\\mathrm {~AU}^{-1}$$ , corresponding to $$\\lambda \\lesssim 2.1\\times 10^{19}\\mathrm {~m}^2$$ and $$\\mu \\lesssim 7.1\\times 10^{18}\\mathrm {~m}^2$$ . This study provides a theoretical foundation for future tests of quadratic gravity using pulsar timing arrays, gravitational-wave observations, and laboratory-scale short-range gravity experiments.","acceptance_date":null,"reception_date":null,"related_materials":[],"countries":["CN"],"id":107658,"title":"Parameterized post-Newtonian analysis of quadratic gravity and solar system constraints","copyright":[{"statement":"","year":2026,"holder":"The Author(s)"}],"_created_at":"2026-06-01T18:55:31.725430"}]}