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  • image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
    Authors: Pierre Heidmann; Anthony Houppe;

    We construct large families of supergravity solutions that are asymptotic to AdS$_2$ and terminate with a cap that is singular in two dimensions but smooth in higher dimensions. These solutions break supersymmetry and conformal invariance. We list arguments suggesting that they correspond to finite-energy excitations in empty AdS$_2$ that back-react on the geometry by inducing non-trivial bubbling topology. They are constructed from the novel technique associated with the Ernst formalism for AdS$_D\times\mathcal{C}$ solitons in supergravity \cite{Bah:2022pdn}. The technique is applied to $D=2$ in M-theory with $\mathcal{C}=\,$S$^3\times$T$^6$. The directions of $\mathcal{C}$ degenerate smoothly as a chain of bolts which ends the spacetime in the IR and generates non-supersymmetric bubbles supported by M2-brane flux. Some specific solutions have ``flat'' directions where the sizes of their bubbles are totally unconstrained and can be arbitrarily tuned while the asymptotics remains fixed. The solitons should correspond to regular non-supersymmetric states of a holographically dual CFT$_1$. Comment: 46 pages, 15 figures, 3 appendices. v2 published version: minor corrections + section about energy of the solutions. arXiv admin note: text overlap with arXiv:2210.06483

    image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ arXiv.org e-Print Ar...arrow_drop_down
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    image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
    Journal of High Energy Physics
    Article . 2023 . Peer-reviewed
    License: CC BY
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    https://doi.org/10.48550/arxiv...
    Article . 2022
    License: arXiv Non-Exclusive Distribution
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    Article . 2023
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      image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ arXiv.org e-Print Ar...arrow_drop_down
      image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
      image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
      Journal of High Energy Physics
      Article . 2023 . Peer-reviewed
      License: CC BY
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      https://doi.org/10.48550/arxiv...
      Article . 2022
      License: arXiv Non-Exclusive Distribution
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  • image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
    Authors: Kuzucuoğlu, Catherine; Leroy, Suzanne;

    This article aims at presenting water level changes within the Caspian Sea watershed since the Last Glacial Maximum, with some chronological references to Late Pleistocene highstands and lowstands. The drivers of water level changes may be related to a climatic context, or other triggering factors. After introducing the physical geography of the Caspian Sea, (submarine basins and sills, geological structure, surrounding reliefs), the climate components connected to changes in water level are presented. Caspian Sea level changes are discussed separately for the Late Pleistocene and the Holocene, as different time periods require different methods, and because Caspian Sea levels respond to a wide range of different drivers. For this purpose, based on an updated synthesis of publications, and after a brief review of methodological limitations, a discussion of the role of climate change versus other factors is provided. The other factors comprise insolation, changes in the extension of the drainage area of the Caspian Sea, especially north up to the Arctic sphere and to the Tien-Shan-Pamir, the wide-ranging latitudes of the regions concerned, as well as local factors related to relief and (past or present) river connections, tectonics, water mass dynamics and other geographical and geomorphological specificities of the watershed. Cet article a pour objectif de présenter l’état des connaissances sur les changements de niveau de la mer Caspienne dans le cadre de son bassin versant, et de présenter des données-références de la chronologie des hauts et bas niveaux. Les facteurs contrôlant ces changements de niveaux sont exposés, qu’il s’agisse de contrôles par le contexte climatique, ou de tout autre contrôle. Après une introduction présentant le cadre physique de la mer Caspienne (bassins et seuils, structure géologique et reliefs environnants), les composantes climatiques influençant les changements de niveau dans les bassins sont présentées. Les changements de niveau sont discutés séparément pour la fin du Pléistocène et pour l’Holocène, car l’étude de chaque période requiert des méthodes différentes, et aussi parce qu’un large éventail de facteurs influence le niveau de la mer Caspienne. C’est pourquoi, après une synthèse des publications sur le sujet, et après un bref rappel des limitations méthodologiques, l’article propose une discussion sur le rôle du climat versus les autres facteurs de contrôle de changements de niveaux. Ces autres facteurs sont l’insolation, les changements d’extension du bassin versant de la mer Caspienne, spécifiquement vers le nord en direction de la zone Arctique et vers le sud-est jusqu’au Pamir, la grande extension latitudinale de la zone considérée, et aussi des facteurs locaux dépendant du relief et des connections hydrographiques (passées ou présentes), de la tectonique, de la dynamique des masses d’eau, et d’autres particularités géographiques et géomorphologiques dans le bassin versant.

    image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ OpenEditionarrow_drop_down
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    Article . 2023 . Peer-reviewed
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  • image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
    Authors: Castellano Mora, Alberto; Herráez Escudero, Alvaro; Ibañez Santiago, Luis Enrique;

    In the Emergence Proposal in QG it is conjectured that all light-particle kinetic terms are absent in the fundamental UV theory and are generated by quantum corrections in the IR. It has been argued that this may provide for some microscopic understanding of the WGC and SDC. In the present paper we take the first steps towards a systematic study of Emergence in the context of string theory. We emphasize the crucial role of the species scale in any EFT coupled to gravity, and discuss its computation in string theory and general systems with light towers of states. We then introduce the notion of Emergence and show how kinetic terms for moduli, gauge bosons and fermions may be generated. One-loop computations play an important role in Emergence, so we present detailed calculations in $d$ spacetime dimensions for the wave-function renormalization of scalars, vectors and fermions. We extend and check the Emergence Proposal in a number string vacua, including 4d $\mathcal{N}=2$ theories arising from type IIA on a CY$_3$, where the towers at strong coupling are comprised by D0 and (wrapped) D2-branes, and also elaborate on how instanton corrections would fit within the emergence picture. Higher dimensional examples are also discussed, including 6d and 7d models arising from F-/M-theory on an elliptic CY$_3$ or a $K3$ surface. We also consider 10d string theories and study in some detail the emergence mechanism in type IIA. We show as well how the flux potential in 4d may be obtained from the emergence prescription, by analyzing the corresponding decompactification limits to M-theory. We find that the required kinetic terms for the dual 3-form fields can arise upon integrating out towers of massive gravitini (and bosonic superpartners). Our analysis renders support to the Emergence Proposal, and to the idea that infinite distance singularities may arise in QG as an intrinsic IR phenomenon. Comment: v2: minor changes and typos corrected. 79 pages + Appendices, 11 figures, 8 tables

    image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ Recolector de Cienci...arrow_drop_down
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    image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
    image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
    Biblos-e Archivo
    Other literature type . 2023
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    image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
    Journal of High Energy Physics
    Article . 2023 . Peer-reviewed
    License: CC BY
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    DOAJ
    Article . 2023
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    https://doi.org/10.48550/arxiv...
    Article . 2022
    License: arXiv Non-Exclusive Distribution
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      image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ Recolector de Cienci...arrow_drop_down
      image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
      image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
      image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
      Biblos-e Archivo
      Other literature type . 2023
      Data sources: Biblos-e Archivo
      image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
      Journal of High Energy Physics
      Article . 2023 . Peer-reviewed
      License: CC BY
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      DOAJ
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      https://doi.org/10.48550/arxiv...
      Article . 2022
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  • image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
    Authors: A. Albert; S. Alves; M. André; M. Ardid; +150 Authors

    Interactions of cosmic ray protons, atomic nuclei, and electrons in the interstellar medium in the inner part of the Milky Way produce a γ-ray flux from the Galactic Ridge. If the γ-ray emission is dominated by proton and nuclei interactions, a neutrino flux comparable to the γ-ray flux is expected from the same sky region. Data collected by the ANTARES neutrino telescope are used to constrain the neutrino flux from the Galactic Ridge in the 1-100 TeV energy range. Neutrino events reconstructed both as tracks and showers are considered in the analysis and the selection is optimized for the search of an excess in the region |l| <30◦, |b| <2◦. The expected background in the search region is estimated using an off-zone region with similar sky coverage. Neutrino signal originating from a power-law spectrum with spectral index ranging from ν=1to 4is simulated in both channels. The observed energy distributions are fitted to constrain the neutrino emission from the Ridge. The energy distributions in the signal region are inconsistent with the background expectation at ∼96%confidence level. The mild excess over the background is consistent with a neutrino flux with a power law with a spectral index 2.45+0.22−0.34and a flux normalization dNνdEν=4.0+2.7−2.0×10−16GeV−1cm−2s−1sr−1at 40 TeV reference energy. Such flux is consistent with the expected neutrino signal if the bulk of the observed γ-ray flux from the Galactic Ridge originates from interactions of cosmic ray protons and nuclei with a power-law spectrum extending well into the PeV energy range Consiliul National al Cercetarii Stiintifice (CNCS) Unitatea Executiva pentru Finantarea Invatamantului Superior, a Cercetarii, Dezvoltarii si Inovarii (UEFISCDI) ANR-10-LABX-0023 ANR-18-IDEX-0001 Arab Fund for Economic and Social Development ASFAE/2022/023 ASFAE/2022/014 PROMETEO/2020/019 GENT/2018/034 GENT/2019/043 GENT/2020/049 GENT/2021/23 P18-FR-5057 101025085 Ministry of Higher Education, Scientific Research and Training, Morocco PID2021-124591NB-C41 PID2021-124591NB-C42 PID2021-124591NB-C43 Programa Maria Zambrano (Spanish Ministry of Universities by the European Union, NextGenerationEU), Spain "European Union NextGenerationEU/PRTR", Programa de Planes Complementarios I+D+I Netherlands Organization for Scientific Research (NWO) Netherlands Government Centre National de la Recherche Scientifique (CNRS) Federal Ministry of Education & Research (BMBF) Istituto Nazionale di Fisica Nucleare (INFN) Marie Curie Actions European Union (EU) GenT of the Generalitat Valenciana Region Provence-Alpes-Cpte d'Azur Region Provence-Alpes-Cote d'Azur French Atomic Energy Commission ERDF A way of making Europe Junta de Andalucia 754496 European Union (EU) Programa Prometeo Region Grand-Est Labex UnivEarthS EU: MSC program MCIN/AEI

    image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ Archivio istituziona...arrow_drop_down
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    Other literature type . 2023 . Peer-reviewed
    License: CC BY
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    Physics Letters B
    Article . 2023 . Peer-reviewed
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    https://doi.org/10.48550/arxiv...
    Article . 2022
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    Article . 2023
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  • image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
    Authors: Bonetti, Federico; Minasian, Ruben; Camell, Valentí Vall; Weck, Peter;

    Abstract In this paper, we present a unified perspective on sphere consistent truncations based on the classical geometric properties of sphere bundles. The backbone of our approach is the global angular form for the sphere. A universal formula for the Kaluza-Klein ansatz of the flux threading the n-sphere captures the full nonabelian isometry group SO(n + 1) and scalar deformations associated to the coset SL(n + 1, ℝ)/SO(n + 1). In all cases, the scalars enter the ansatz in a shift by an exact form. We find that the latter can be completely fixed by imposing mild conditions, motivated by supersymmetry, on the scalar potential arising from dimensional reduction of the higher dimensional theory. We comment on the role of the global angular form in the derivation of the topological couplings of the lower-dimensional theory, and on how this perspective could provide inroads into the study of consistent truncations with less supersymmetry.

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    https://doi.org/10.48550/arxiv...
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    Authors: The Pierre Auger Collaboration; Halim, A. Abdul; Abreu, P.; Aglietta, M.; +202 Authors

    Spain – Ministerio de Economía, Industria y Competitividad (FPA2017-85114-P and PID2019-104676GB-C32) RENATA Red Nacional Temática de Astropartículas (FPA2015-68783-REDT) Junta de Andalucía (SOMM17/6104/UGR, P18-FR-4314) Feder Funds María de Maeztu Unit of Excellence (MDM-2016-0692) Xunta de Galicia (ED431C 2017/07)

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    https://doi.org/10.5445/ir/100...
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    https://doi.org/10.48550/arxiv...
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    Authors: Shyam Balaji; Maura E. Ramirez-Quezada; Joseph Silk; Yongchao Zhang;

    Recent astrophysical transient Swift J1913.1+1946 may be associated with the $\gamma$-ray burst GRB 221009A. The redshift of this event is $z\simeq 0.151$. Very high-energy $\gamma$-rays (up to 18 TeV) followed the transient and were observed by LHAASO, additionally Carpet-2 detected a photon-like air shower of 251 TeV. Photons of such high energy are expected to readily annihilate with the diffuse extragalactic background light (EBL) before reaching Earth. If the $\gamma$-ray identification and redshift measurements are correct, new physics could be necessary to explain these measurements. This letter provides the first CP-even scalar explanation of the most energetic 18 TeV event reported by LHAASO. In this minimal scenario, the light scalar singlet $S$ mixes with the Standard Model (SM) Higgs boson $h$. The highly boosted $S$ particles are produced in the GRB and then undergo the radiative decay di-photon $S\rightarrow \gamma\gamma$ while propagating to Earth. The resulting photons may thus be produced at a remote region without being nullified by the EBL. Hence, the usual exponential reduction of $\gamma$-rays is lifted due to an attenuation that is inverse in the optical depth, which becomes much larger due to the scalar carriers. Comment: 6 pages, 2 figures

    image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ arXiv.org e-Print Ar...arrow_drop_down
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    https://doi.org/10.1103/physre...
    Article . 2023 . Peer-reviewed
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      https://doi.org/10.1103/physre...
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    Authors: S. Gwon; P. Granger; G. Yang; S. Bolognesi; +46 Authors

    Neutrino oscillation experiments require a precise measurement of the neutrino energy. However, the kinematic detection of the final-state neutron in the neutrino interaction is missing in current neutrino oscillation experiments. The missing neutron kinematic detection results in a smaller detected neutrino energy than the true neutrino energy. A novel 3D-projection scintillator tracker, which consists of roughly ten million active cubes covered with an optical reflector, is capable of measuring the neutron kinetic energy and direction on an event-by-event basis using the time-of-flight technique thanks to the fast timing, fine granularity, and high light yield. The ν¯μ interactions tend to produce neutrons in the final state. By measuring the neutron kinetic energy, the ν¯μ energy can be reconstructed better, allowing a tighter incoming neutrino flux constraint. This article shows the detector’s ability to reconstruct neutron kinetic energy and the ν¯μ flux constraint achieved by selecting the charged-current interactions without mesons or protons in the final state. Neutrino oscillation experiments require a precise measurement of the neutrino energy. However, the kinematic detection of the final-state neutron in the neutrino interaction is missing in current neutrino oscillation experiments. The missing neutron kinematic detection results in a feed-down of the detected neutrino energy compared to the true neutrino energy. A novel 3D\textcolor{black}{-}projection scintillator tracker, which consists of roughly ten million active cubes covered with an optical reflector, is capable of measuring the neutron kinetic energy and direction on an event-by-event basis using the time-of-flight technique thanks to the fast timing, fine granularity, and high light yield. The $\bar{\nu}_{\mu}$ interactions tend to produce neutrons in the final state. By inferring the neutron kinetic energy, the $\bar{\nu}_{\mu}$ energy can be reconstructed better, allowing a tighter incoming neutrino flux constraint. This paper shows the detector's ability to reconstruct neutron kinetic energy and the $\bar{\nu}_{\mu}$ flux constraint achieved by selecting the charged-current interactions without mesons or protons in the final state.

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    https://doi.org/10.1103/physre...
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    Authors: Pierre Auger Collaboration; Abdul Halim, A.; Abreu, P.; Aglietta, M.; +337 Authors

    Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET) Spanish Government FPA2017-85114-P PID2019-104676GB-C32 European Particle Physics Latin American Network Junta de Andalucia SOMM17/6104/UGR P18-FR-4314 Xunta de Galicia ED431C 2017/07 ANPCyT Spanish Government Marie Curie-IRSES/EPLANET Spanish Government

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    https://doi.org/10.5445/ir/100...
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    https://doi.org/10.5445/ir/100...
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    The Astrophysical Journal Supplement Series
    Article . 2023 . Peer-reviewed
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    Authors: Dieminger, T.; Dolan, S.; Sgalaberna, D.; Nikolakopoulos, A.; +4 Authors

    The potential for mis-modeling of $\nu_{\mu}$/$\nu_{e}$, $\bar{\nu}_{\mu}$/$\bar{\nu}_{e}$ and $\nu_{e}$/$\bar{\nu}_{e}$ cross section ratios due to nuclear effects is quantified by considering model spread within the full kinematic phase space for CCQE interactions. Its impact is then propagated to simulated experimental configurations based on the Hyper-K and ESS$\nu$SB experiments. Although significant discrepancies between theoretical models is confirmed, it is found that these largely lie in regions of phase space that contribute only a very small portion of the flux integrated cross sections. Overall, a systematic uncertainty on the oscillated flux-averaged $\nu_{e}$/$\bar{\nu}_{e}$ cross-section ratio is found to be $\sim$2\% and $\sim$4\% for Hyper-K and ESS$\nu$SB respectively. Comment: 5 pages, 4 figures. A letter-style version of the original arXiv submission

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  • image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
    Authors: Pierre Heidmann; Anthony Houppe;

    We construct large families of supergravity solutions that are asymptotic to AdS$_2$ and terminate with a cap that is singular in two dimensions but smooth in higher dimensions. These solutions break supersymmetry and conformal invariance. We list arguments suggesting that they correspond to finite-energy excitations in empty AdS$_2$ that back-react on the geometry by inducing non-trivial bubbling topology. They are constructed from the novel technique associated with the Ernst formalism for AdS$_D\times\mathcal{C}$ solitons in supergravity \cite{Bah:2022pdn}. The technique is applied to $D=2$ in M-theory with $\mathcal{C}=\,$S$^3\times$T$^6$. The directions of $\mathcal{C}$ degenerate smoothly as a chain of bolts which ends the spacetime in the IR and generates non-supersymmetric bubbles supported by M2-brane flux. Some specific solutions have ``flat'' directions where the sizes of their bubbles are totally unconstrained and can be arbitrarily tuned while the asymptotics remains fixed. The solitons should correspond to regular non-supersymmetric states of a holographically dual CFT$_1$. Comment: 46 pages, 15 figures, 3 appendices. v2 published version: minor corrections + section about energy of the solutions. arXiv admin note: text overlap with arXiv:2210.06483

    image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ arXiv.org e-Print Ar...arrow_drop_down
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    Journal of High Energy Physics
    Article . 2023 . Peer-reviewed
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    https://doi.org/10.48550/arxiv...
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      Journal of High Energy Physics
      Article . 2023 . Peer-reviewed
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  • image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
    Authors: Kuzucuoğlu, Catherine; Leroy, Suzanne;

    This article aims at presenting water level changes within the Caspian Sea watershed since the Last Glacial Maximum, with some chronological references to Late Pleistocene highstands and lowstands. The drivers of water level changes may be related to a climatic context, or other triggering factors. After introducing the physical geography of the Caspian Sea, (submarine basins and sills, geological structure, surrounding reliefs), the climate components connected to changes in water level are presented. Caspian Sea level changes are discussed separately for the Late Pleistocene and the Holocene, as different time periods require different methods, and because Caspian Sea levels respond to a wide range of different drivers. For this purpose, based on an updated synthesis of publications, and after a brief review of methodological limitations, a discussion of the role of climate change versus other factors is provided. The other factors comprise insolation, changes in the extension of the drainage area of the Caspian Sea, especially north up to the Arctic sphere and to the Tien-Shan-Pamir, the wide-ranging latitudes of the regions concerned, as well as local factors related to relief and (past or present) river connections, tectonics, water mass dynamics and other geographical and geomorphological specificities of the watershed. Cet article a pour objectif de présenter l’état des connaissances sur les changements de niveau de la mer Caspienne dans le cadre de son bassin versant, et de présenter des données-références de la chronologie des hauts et bas niveaux. Les facteurs contrôlant ces changements de niveaux sont exposés, qu’il s’agisse de contrôles par le contexte climatique, ou de tout autre contrôle. Après une introduction présentant le cadre physique de la mer Caspienne (bassins et seuils, structure géologique et reliefs environnants), les composantes climatiques influençant les changements de niveau dans les bassins sont présentées. Les changements de niveau sont discutés séparément pour la fin du Pléistocène et pour l’Holocène, car l’étude de chaque période requiert des méthodes différentes, et aussi parce qu’un large éventail de facteurs influence le niveau de la mer Caspienne. C’est pourquoi, après une synthèse des publications sur le sujet, et après un bref rappel des limitations méthodologiques, l’article propose une discussion sur le rôle du climat versus les autres facteurs de contrôle de changements de niveaux. Ces autres facteurs sont l’insolation, les changements d’extension du bassin versant de la mer Caspienne, spécifiquement vers le nord en direction de la zone Arctique et vers le sud-est jusqu’au Pamir, la grande extension latitudinale de la zone considérée, et aussi des facteurs locaux dépendant du relief et des connections hydrographiques (passées ou présentes), de la tectonique, de la dynamique des masses d’eau, et d’autres particularités géographiques et géomorphologiques dans le bassin versant.

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  • image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
    Authors: Castellano Mora, Alberto; Herráez Escudero, Alvaro; Ibañez Santiago, Luis Enrique;

    In the Emergence Proposal in QG it is conjectured that all light-particle kinetic terms are absent in the fundamental UV theory and are generated by quantum corrections in the IR. It has been argued that this may provide for some microscopic understanding of the WGC and SDC. In the present paper we take the first steps towards a systematic study of Emergence in the context of string theory. We emphasize the crucial role of the species scale in any EFT coupled to gravity, and discuss its computation in string theory and general systems with light towers of states. We then introduce the notion of Emergence and show how kinetic terms for moduli, gauge bosons and fermions may be generated. One-loop computations play an important role in Emergence, so we present detailed calculations in $d$ spacetime dimensions for the wave-function renormalization of scalars, vectors and fermions. We extend and check the Emergence Proposal in a number string vacua, including 4d $\mathcal{N}=2$ theories arising from type IIA on a CY$_3$, where the towers at strong coupling are comprised by D0 and (wrapped) D2-branes, and also elaborate on how instanton corrections would fit within the emergence picture. Higher dimensional examples are also discussed, including 6d and 7d models arising from F-/M-theory on an elliptic CY$_3$ or a $K3$ surface. We also consider 10d string theories and study in some detail the emergence mechanism in type IIA. We show as well how the flux potential in 4d may be obtained from the emergence prescription, by analyzing the corresponding decompactification limits to M-theory. We find that the required kinetic terms for the dual 3-form fields can arise upon integrating out towers of massive gravitini (and bosonic superpartners). Our analysis renders support to the Emergence Proposal, and to the idea that infinite distance singularities may arise in QG as an intrinsic IR phenomenon. Comment: v2: minor changes and typos corrected. 79 pages + Appendices, 11 figures, 8 tables

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    Journal of High Energy Physics
    Article . 2023 . Peer-reviewed
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      Journal of High Energy Physics
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    Authors: A. Albert; S. Alves; M. André; M. Ardid; +150 Authors

    Interactions of cosmic ray protons, atomic nuclei, and electrons in the interstellar medium in the inner part of the Milky Way produce a γ-ray flux from the Galactic Ridge. If the γ-ray emission is dominated by proton and nuclei interactions, a neutrino flux comparable to the γ-ray flux is expected from the same sky region. Data collected by the ANTARES neutrino telescope are used to constrain the neutrino flux from the Galactic Ridge in the 1-100 TeV energy range. Neutrino events reconstructed both as tracks and showers are considered in the analysis and the selection is optimized for the search of an excess in the region |l| <30◦, |b| <2◦. The expected background in the search region is estimated using an off-zone region with similar sky coverage. Neutrino signal originating from a power-law spectrum with spectral index ranging from ν=1to 4is simulated in both channels. The observed energy distributions are fitted to constrain the neutrino emission from the Ridge. The energy distributions in the signal region are inconsistent with the background expectation at ∼96%confidence level. The mild excess over the background is consistent with a neutrino flux with a power law with a spectral index 2.45+0.22−0.34and a flux normalization dNνdEν=4.0+2.7−2.0×10−16GeV−1cm−2s−1sr−1at 40 TeV reference energy. Such flux is consistent with the expected neutrino signal if the bulk of the observed γ-ray flux from the Galactic Ridge originates from interactions of cosmic ray protons and nuclei with a power-law spectrum extending well into the PeV energy range Consiliul National al Cercetarii Stiintifice (CNCS) Unitatea Executiva pentru Finantarea Invatamantului Superior, a Cercetarii, Dezvoltarii si Inovarii (UEFISCDI) ANR-10-LABX-0023 ANR-18-IDEX-0001 Arab Fund for Economic and Social Development ASFAE/2022/023 ASFAE/2022/014 PROMETEO/2020/019 GENT/2018/034 GENT/2019/043 GENT/2020/049 GENT/2021/23 P18-FR-5057 101025085 Ministry of Higher Education, Scientific Research and Training, Morocco PID2021-124591NB-C41 PID2021-124591NB-C42 PID2021-124591NB-C43 Programa Maria Zambrano (Spanish Ministry of Universities by the European Union, NextGenerationEU), Spain "European Union NextGenerationEU/PRTR", Programa de Planes Complementarios I+D+I Netherlands Organization for Scientific Research (NWO) Netherlands Government Centre National de la Recherche Scientifique (CNRS) Federal Ministry of Education & Research (BMBF) Istituto Nazionale di Fisica Nucleare (INFN) Marie Curie Actions European Union (EU) GenT of the Generalitat Valenciana Region Provence-Alpes-Cpte d'Azur Region Provence-Alpes-Cote d'Azur French Atomic Energy Commission ERDF A way of making Europe Junta de Andalucia 754496 European Union (EU) Programa Prometeo Region Grand-Est Labex UnivEarthS EU: MSC program MCIN/AEI

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    Physics Letters B
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    https://doi.org/10.48550/arxiv...
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    Authors: Bonetti, Federico; Minasian, Ruben; Camell, Valentí Vall; Weck, Peter;

    Abstract In this paper, we present a unified perspective on sphere consistent truncations based on the classical geometric properties of sphere bundles. The backbone of our approach is the global angular form for the sphere. A universal formula for the Kaluza-Klein ansatz of the flux threading the n-sphere captures the full nonabelian isometry group SO(n + 1) and scalar deformations associated to the coset SL(n + 1, ℝ)/SO(n + 1). In all cases, the scalars enter the ansatz in a shift by an exact form. We find that the latter can be completely fixed by imposing mild conditions, motivated by supersymmetry, on the scalar potential arising from dimensional reduction of the higher dimensional theory. We comment on the role of the global angular form in the derivation of the topological couplings of the lower-dimensional theory, and on how this perspective could provide inroads into the study of consistent truncations with less supersymmetry.

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    Authors: The Pierre Auger Collaboration; Halim, A. Abdul; Abreu, P.; Aglietta, M.; +202 Authors

    Spain – Ministerio de Economía, Industria y Competitividad (FPA2017-85114-P and PID2019-104676GB-C32) RENATA Red Nacional Temática de Astropartículas (FPA2015-68783-REDT) Junta de Andalucía (SOMM17/6104/UGR, P18-FR-4314) Feder Funds María de Maeztu Unit of Excellence (MDM-2016-0692) Xunta de Galicia (ED431C 2017/07)

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    Authors: Shyam Balaji; Maura E. Ramirez-Quezada; Joseph Silk; Yongchao Zhang;

    Recent astrophysical transient Swift J1913.1+1946 may be associated with the $\gamma$-ray burst GRB 221009A. The redshift of this event is $z\simeq 0.151$. Very high-energy $\gamma$-rays (up to 18 TeV) followed the transient and were observed by LHAASO, additionally Carpet-2 detected a photon-like air shower of 251 TeV. Photons of such high energy are expected to readily annihilate with the diffuse extragalactic background light (EBL) before reaching Earth. If the $\gamma$-ray identification and redshift measurements are correct, new physics could be necessary to explain these measurements. This letter provides the first CP-even scalar explanation of the most energetic 18 TeV event reported by LHAASO. In this minimal scenario, the light scalar singlet $S$ mixes with the Standard Model (SM) Higgs boson $h$. The highly boosted $S$ particles are produced in the GRB and then undergo the radiative decay di-photon $S\rightarrow \gamma\gamma$ while propagating to Earth. The resulting photons may thus be produced at a remote region without being nullified by the EBL. Hence, the usual exponential reduction of $\gamma$-rays is lifted due to an attenuation that is inverse in the optical depth, which becomes much larger due to the scalar carriers. Comment: 6 pages, 2 figures

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    https://doi.org/10.1103/physre...
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    Authors: S. Gwon; P. Granger; G. Yang; S. Bolognesi; +46 Authors

    Neutrino oscillation experiments require a precise measurement of the neutrino energy. However, the kinematic detection of the final-state neutron in the neutrino interaction is missing in current neutrino oscillation experiments. The missing neutron kinematic detection results in a smaller detected neutrino energy than the true neutrino energy. A novel 3D-projection scintillator tracker, which consists of roughly ten million active cubes covered with an optical reflector, is capable of measuring the neutron kinetic energy and direction on an event-by-event basis using the time-of-flight technique thanks to the fast timing, fine granularity, and high light yield. The ν¯μ interactions tend to produce neutrons in the final state. By measuring the neutron kinetic energy, the ν¯μ energy can be reconstructed better, allowing a tighter incoming neutrino flux constraint. This article shows the detector’s ability to reconstruct neutron kinetic energy and the ν¯μ flux constraint achieved by selecting the charged-current interactions without mesons or protons in the final state. Neutrino oscillation experiments require a precise measurement of the neutrino energy. However, the kinematic detection of the final-state neutron in the neutrino interaction is missing in current neutrino oscillation experiments. The missing neutron kinematic detection results in a feed-down of the detected neutrino energy compared to the true neutrino energy. A novel 3D\textcolor{black}{-}projection scintillator tracker, which consists of roughly ten million active cubes covered with an optical reflector, is capable of measuring the neutron kinetic energy and direction on an event-by-event basis using the time-of-flight technique thanks to the fast timing, fine granularity, and high light yield. The $\bar{\nu}_{\mu}$ interactions tend to produce neutrons in the final state. By inferring the neutron kinetic energy, the $\bar{\nu}_{\mu}$ energy can be reconstructed better, allowing a tighter incoming neutrino flux constraint. This paper shows the detector's ability to reconstruct neutron kinetic energy and the $\bar{\nu}_{\mu}$ flux constraint achieved by selecting the charged-current interactions without mesons or protons in the final state.

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      https://doi.org/10.1103/physre...
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    Authors: Pierre Auger Collaboration; Abdul Halim, A.; Abreu, P.; Aglietta, M.; +337 Authors

    Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET) Spanish Government FPA2017-85114-P PID2019-104676GB-C32 European Particle Physics Latin American Network Junta de Andalucia SOMM17/6104/UGR P18-FR-4314 Xunta de Galicia ED431C 2017/07 ANPCyT Spanish Government Marie Curie-IRSES/EPLANET Spanish Government

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    The Astrophysical Journal Supplement Series
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    Authors: Dieminger, T.; Dolan, S.; Sgalaberna, D.; Nikolakopoulos, A.; +4 Authors

    The potential for mis-modeling of $\nu_{\mu}$/$\nu_{e}$, $\bar{\nu}_{\mu}$/$\bar{\nu}_{e}$ and $\nu_{e}$/$\bar{\nu}_{e}$ cross section ratios due to nuclear effects is quantified by considering model spread within the full kinematic phase space for CCQE interactions. Its impact is then propagated to simulated experimental configurations based on the Hyper-K and ESS$\nu$SB experiments. Although significant discrepancies between theoretical models is confirmed, it is found that these largely lie in regions of phase space that contribute only a very small portion of the flux integrated cross sections. Overall, a systematic uncertainty on the oscillated flux-averaged $\nu_{e}$/$\bar{\nu}_{e}$ cross-section ratio is found to be $\sim$2\% and $\sim$4\% for Hyper-K and ESS$\nu$SB respectively. Comment: 5 pages, 4 figures. A letter-style version of the original arXiv submission

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