Accès ouvert déclaré 2024 article

Probing the scalar WIMP-pion coupling with the first LUX-ZEPLIN data

J. Aalbers, D. S. Akerib, A. K. Al Musalhi, F. Alder, C. S. Amarasinghe, A. Ames, Tyler Anderson, N. Angelides, H. M. Araújo, J. E. Armstrong, M. Arthurs, Alexander A. Baker, S. Balashov, J. Bang, E. E. Barillier, J. W. Bargemann, K. Beattie, Theophilus Benson, A. Bhatti, A. Biekert, T. P. Biesiadzinski, H. J. Birch, E. Bishop, G. M. Blockinger, B. Boxer, C. A. J. Brew, P. Brás, S. Burdin, M. Buuck, M. C. Carmona-Benitez, M. Carter, A. Chawla, H. Chen, J. J. Cherwinka, Y. T. Chin, N. I. Chott, M. V. Converse, A. Cottle, G. Cox, D. Curran, C. E. Dahl, A. David, John M. DelGaudio, S. Dey, L. de Viveiros, L. Di Felice, C. Ding, J. E. Y. Dobson, E. Druszkiewicz, S. R. Eriksen, A. Fan, N. M. Fearon, N. Fieldhouse, S. Fiorucci, H. Flaecher, E. D. Fraser, T. Fruth, R. J. Gaitskell, A. Geffre, J. Genovesi, C. Ghag, R. Gibbons, S. Gokhale, J. Green, M. G. D. van der Grinten, J. J. Haiston, C. Hall, S. Han, E. Hartigan-O’Connor, S. J. Haselschwardt, S. A. Hertel, G. Heuermann, G. J. Homenides, M. Horn, D. Q. Huang, D. Hunt, E. Jacquet, R. S. James, J. Johnson, A. C. Kaboth, A. Kamaha, M. Kannichankandy, D. Khaitan, A. Khazov, I. Khurana, Y. D. Kim, Jaebak Kim, J. Kingston, R. Kirk, D. Kodroff, L. Korley, E. V. Korolkova, H. Kraus, S. Kravitz, L. Kreczko, V. A. Kudryavtsev, D. S. Leonard, K. T. Lesko, C. Levy, J. Lin, A. Lindote, R. Linehan, W. H. Lippincott, I. Lopes, W. Lorenzon, C. Lu, S. Luitz, P. A. Majewski, A. Manalaysay, R. L. Mannino, C. Maupin, M. E. McCarthy, Gary L. McDowell, D. N. McKinsey, Joseph McLaughlin, R. McMonigle, Eric Haynes Miller, E. Mizrachi, A. Monte, M. E. Monzani, J. D. Morales Mendoza, E. Morrison, B. J. Mount, M. Murdy, A. St. J. Murphy, A. Naylor, H. N. Nelson, F. Neves, A. Nguyen, J. A. Nikoleyczik, I. Olcina, K. C. Oliver-Mallory, J. Orpwood, K. J. Palladino, J. D. Palmer, N. J. Pannifer, N. Parveen, S. J. Patton, G. Pereira, E. Perry, T. Pershing, A. Piepke, Y. Qie, J. Reichenbacher, C. A. Rhyne, Q. Riffard, G. R. C. Rischbieter, H. S. Riyat, R. Rosero, T. Rushton, D. Rynders, D. Santone, A. B. M. R. Sazzad, R. W. Schnee, S. Shaw, T. Shutt, J. J. Silk, C. Silva, G. Sinev, J. Siniscalco, R. Smith, V. N. Solovov, P. Sorensen, J. Soria, I. Stancu, A. Stevens, K. Stifter, B. Suerfu, T. J. Sumner, M. Szydagis, W. C. Taylor, D. R. Tiedt, M. Timalsina, Z. Tong, D. R. Tovey, J. Tranter, M. Trask, M. Tripathi, D. R. Tronstad, A. Vacheret, A. C. Vaitkus, O. Valentino, V. Velan, Andrew Wang, J. J. Wang, Y. Wang, J. R. Watson, R. C. Webb, L. Weeldreyer, T. J. Whitis, M. Williams, W. J. Wisniewski, F. L. H. Wolfs, S. Woodford, David Woodward, Chris J. Wright, Q. Xia, X. Xiang, Jing Xu, M. Yeh, E. A. Zweig

4Citations signalées, ce qui n’est pas une note de qualité

41Institutions déclarées

6Pays d’affiliation déclarés

Rattachement africain : us, gb, ch, pt, au, it. Niveau de preuve : code pays fourni par la source.

Le résumé fourni par la source

Abstract Weakly interacting massive particles (WIMPs) may interact with a virtual pion that is exchanged between nucleons. This interaction channel is important to consider in models where the spin-independent isoscalar channel is suppressed. Using data from the first science run of the LUX-ZEPLIN dark matter experiment, containing 60 live days of data in a 5.5 tonne fiducial mass of liquid xenon, we report the results on a search for WIMP-pion interactions. We observe no significant excess and set an upper limit of 1.5 × 10 −46 cm 2 at a 90% confidence level for a WIMP mass of 33 GeV/c 2 for this interaction.

Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.

Le contrôle bibliographique ouvert

DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.

Titre Crossref: Probing the scalar WIMP-pion coupling with the first LUX-ZEPLIN data
Date Crossref: 31/08/2024
Éditeur: Springer Science and Business Media LLC
Type: journal-article

Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.

Les institutions déclarées

SLAC National Accelerator Laboratory Kavli Institute for Particle Astrophysics and Cosmology Stanford University University College London University of California, Santa Barbara University of Michigan Imperial College London University of Maryland, College Park Rutherford Appleton Laboratory Brown University University of Zurich Lawrence Berkeley National Laboratory University of Wisconsin–Madison University of California, Berkeley Scottish Universities Physics Alliance University of Edinburgh University at Albany, State University of New York University of California, Davis LIP - Laboratory of Instrumentation and Experimental Particle Physics University of Coimbra University of Liverpool Pennsylvania State University Royal Holloway University of London South Dakota School of Mines and Technology University of Rochester South Dakota Science and Technology Authority Northwestern University Fermi National Accelerator Laboratory University of Oxford King's College London University of Bristol The University of Sydney Brookhaven National Laboratory University of Massachusetts Amherst University of Alabama University of Sheffield The University of Texas at Austin Lawrence Livermore National Laboratory Vatican Observatory Black Hills State University Texas A&M University

Une affiliation ne permet pas de déduire la nationalité d’un auteur.

Les sujets associés

Dark Matter and Cosmic PhenomenaParticle physics theoretical and experimental studiesCosmology and Gravitation Theories

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