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Exploration of mass splitting and muon/tau mixing parameters for an eV-scale sterile neutrino with IceCube
Physics Letters B ( IF 4.3 ) Pub Date : 2024-10-17 , DOI: 10.1016/j.physletb.2024.139077
IceCube Collaboration, R. Abbasi, M. Ackermann, J. Adams, S.K. Agarwalla, J.A. Aguilar, M. Ahlers, J.M. Alameddine, N.M. Amin, K. Andeen, C. Argüelles, Y. Ashida, S. Athanasiadou, L. Ausborm, S.N. Axani, X. Bai, A. Balagopal V, M. Baricevic, S.W. Barwick, S. Bash, V. Basu, R. Bay, J.J. Beatty, J. Becker Tjus, J. Beise, C. Bellenghi, C. Benning, S. BenZvi, D. Berley, E. Bernardini, D.Z. Besson, E. Blaufuss, L. Bloom, S. Blot, F. Bontempo, J.Y. Book Motzkin, C. Boscolo Meneguolo, S. Böser, O. Botner, J. Böttcher, J. Braun, B. Brinson, J. Brostean-Kaiser, L. Brusa, R.T. Burley, D. Butterfield, M.A. Campana, I. Caracas, K. Carloni, J. Carpio, S. Chattopadhyay, N. Chau, Z. Chen, D. Chirkin, S. Choi, B.A. Clark, A. Coleman, G.H. Collin, A. Connolly, J.M. Conrad, P. Coppin, R. Corley, P. Correa, D.F. Cowen, P. Dave, C. De Clercq, J.J. DeLaunay, D. Delgado, S. Deng, A. Desai, P. Desiati, K.D. de Vries, G. de Wasseige, T. DeYoung, A. Diaz, J.C. Díaz-Vélez, P. Dierichs, M. Dittmer, A. Domi, L. Draper, H. Dujmovic, K. Dutta, M.A. DuVernois, T. Ehrhardt, L. Eidenschink, A. Eimer, P. Eller, E. Ellinger, S. El Mentawi, D. Elsässer, R. Engel, H. Erpenbeck, J. Evans, P.A. Evenson, K.L. Fan, K. Fang, K. Farrag, A.R. Fazely, A. Fedynitch, N. Feigl, S. Fiedlschuster, C. Finley, L. Fischer, D. Fox, A. Franckowiak, S. Fukami, P. Fürst, J. Gallagher, E. Ganster, A. Garcia, M. Garcia, G. Garg, E. Genton, L. Gerhardt, A. Ghadimi, C. Girard-Carillo, C. Glaser, T. Glüsenkamp, J.G. Gonzalez, S. Goswami, A. Granados, D. Grant, S.J. Gray, O. Gries, S. Griffin, S. Griswold, K.M. Groth, C. Günther, P. Gutjahr, C. Ha, C. Haack, A. Hallgren, L. Halve, F. Halzen, H. Hamdaoui, M. Ha Minh, M. Handt, K. Hanson, J. Hardin, A.A. Harnisch, P. Hatch, A. Haungs, J. Häußler, K. Helbing, J. Hellrung, J. Hermannsgabner, L. Heuermann, N. Heyer, S. Hickford, A. Hidvegi, C. Hill, G.C. Hill, K.D. Hoffman, S. Hori, K. Hoshina, M. Hostert, W. Hou, T. Huber, K. Hultqvist, M. Hünnefeld, R. Hussain, K. Hymon, A. Ishihara, W. Iwakiri, M. Jacquart, O. Janik, M. Jansson, G.S. Japaridze, M. Jeong, M. Jin, B.J.P. Jones, N. Kamp, D. Kang, W. Kang, X. Kang, A. Kappes, D. Kappesser, L. Kardum, T. Karg, M. Karl, A. Karle, A. Katil, U. Katz, M. Kauer, J.L. Kelley, M. Khanal, A. Khatee Zathul, A. Kheirandish, J. Kiryluk, S.R. Klein, A. Kochocki, R. Koirala, H. Kolanoski, T. Kontrimas, L. Köpke, C. Kopper, D.J. Koskinen, P. Koundal, M. Kovacevich, M. Kowalski, T. Kozynets, J. Krishnamoorthi, K. Kruiswijk, E. Krupczak, A. Kumar, E. Kun, N. Kurahashi, N. Lad, C. Lagunas Gualda, M. Lamoureux, M.J. Larson, S. Latseva, F. Lauber, J.P. Lazar, J.W. Lee, K. Leonard DeHolton, A. Leszczyńska, J. Liao, M. Lincetto, Y.T. Liu, M. Liubarska, E. Lohfink, C. Love, C.J. Lozano Mariscal, L. Lu, F. Lucarelli, W. Luszczak, Y. Lyu, J. Madsen, E. Magnus, K.B.M. Mahn, Y. Makino, E. Manao, S. Mancina, W. Marie Sainte, I.C. Mariş, S. Marka, Z. Marka, M. Marsee, I. Martinez-Soler, R. Maruyama, F. Mayhew, F. McNally, J.V. Mead, K. Meagher, S. Mechbal, A. Medina, M. Meier, Y. Merckx, L. Merten, J. Micallef, J. Mitchell, T. Montaruli, R.W. Moore, Y. Morii, R. Morse, M. Moulai, T. Mukherjee, R. Naab, R. Nagai, M. Nakos, U. Naumann, J. Necker, A. Negi, L. Neste, M. Neumann, H. Niederhausen, M.U. Nisa, K. Noda, A. Noell, A. Novikov, A. Obertacke Pollmann, V. O'Dell, B. Oeyen, A. Olivas, R. Orsoe, J. Osborn, E. O'Sullivan, H. Pandya, N. Park, G.K. Parker, E.N. Paudel, L. Paul, C. Pérez de los Heros, T. Pernice, J. Peterson, S. Philippen, A. Pizzuto, M. Plum, A. Pontén, Y. Popovych, M. Prado Rodriguez, B. Pries, R. Procter-Murphy, G.T. Przybylski, C. Raab, J. Rack-Helleis, M. Ravn, K. Rawlins, Z. Rechav, A. Rehman, P. Reichherzer, E. Resconi, S. Reusch, W. Rhode, B. Riedel, A. Rifaie, E.J. Roberts, S. Robertson, S. Rodan, G. Roellinghoff, M. Rongen, A. Rosted, C. Rott, T. Ruhe, L. Ruohan, D. Ryckbosch, I. Safa, J. Saffer, D. Salazar-Gallegos, P. Sampathkumar, A. Sandrock, M. Santander, S. Sarkar, S. Sarkar, J. Savelberg, P. Savina, P. Schaile, M. Schaufel, H. Schieler, S. Schindler, B. Schlüter, F. Schlüter, N. Schmeisser, T. Schmidt, J. Schneider, F.G. Schröder, L. Schumacher, S. Sclafani, D. Seckel, M. Seikh, M. Seo, S. Seunarine, P. Sevle Myhr, R. Shah, S. Shefali, N. Shimizu, M. Silva, B. Skrzypek, B. Smithers, R. Snihur, J. Soedingrekso, A. Søgaard, D. Soldin, P. Soldin, G. Sommani, C. Spannfellner, G.M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, T. Stezelberger, T. Stürwald, T. Stuttard, G.W. Sullivan, I. Taboada, S. Ter-Antonyan, A. Terliuk, M. Thiesmeyer, W.G. Thompson, J. Thwaites, S. Tilav, K. Tollefson, C. Tönnis, S. Toscano, D. Tosi, A. Trettin, R. Turcotte, J.P. Twagirayezu, M.A. Unland Elorrieta, A.K. Upadhyay, K. Upshaw, A. Vaidyanathan, N. Valtonen-Mattila, J. Vandenbroucke, N. van Eijndhoven, D. Vannerom, J. van Santen, J. Vara, F. Varsi, J. Veitch-Michaelis, M. Venugopal, M. Vereecken, S. Verpoest, D. Veske, A. Vijai, C. Walck, A. Wang, C. Weaver, P. Weigel, A. Weindl, J. Weldert, A.Y. Wen, C. Wendt, J. Werthebach, M. Weyrauch, N. Whitehorn, C.H. Wiebusch, D.R. Williams, L. Witthaus, A. Wolf, M. Wolf, G. Wrede, X.W. Xu, J.P. Yanez, E. Yildizci, S. Yoshida, R. Young, S. Yu, T. Yuan, Z. Zhang, P. Zhelnin, P. Zilberman, M. Zimmerman

We present the first three-parameter fit to a 3+1 sterile neutrino model using 7.634 years of data from the IceCube Neutrino Observatory on νμ+νμ charged-current interactions in the energy range 500–9976 GeV. Our analysis is sensitive to the mass-squared splitting between the heaviest and lightest mass state (Δm412), the mixing matrix element connecting muon flavor to the fourth mass state (|Uμ4|2), and the element connecting tau flavor to the fourth mass state (|Uτ4|2). Predicted propagation effects in matter enhance the signature through a resonance as atmospheric neutrinos from the Northern Hemisphere traverse the Earth to the IceCube detector at the South Pole. The remaining sterile neutrino matrix elements are left fixed, with |Ue4|2=0 and δ14=0, as they have a negligible effect, and δ24=π is set to give the most conservative limits. The result is consistent with the no-sterile neutrino hypothesis with a probability of 4.3%. Profiling the likelihood of each parameter yields the 90% confidence levels: 2.4eV2<Δm412<9.6eV2, 0.0081<|Uμ4|2<0.10, and |Uτ4|2<0.035, which narrows the allowed parameter-space for |Uτ4|2. However, the primary result of this analysis is the first map of the 3+1 parameter space exploring the interdependence of Δm412, |Uμ4|2, and |Uτ4|2.

中文翻译:


使用 IceCube 探索 eV 级无菌中微子的质量分裂和 μ 子/tau 混合参数



我们使用 IceCube 中微子天文台 7.634 年关于 500–9976 GeV 能量范围内 νμ+ν ̅ μ 带电相互作用的数据,提出了对 3+1 无菌中微子模型的第一个三参数拟合。我们的分析对最重和最轻质量态 (Δm412) 之间的质量平方分裂很敏感,混合基质元素将 μ 子风味与第四质量态 (|Uμ4|2) 和将 tau 风味与第四质量态联系起来的元素 (|Uτ4|2)。当来自北半球的大气中微子穿过地球到达南极的 IceCube 探测器时,预测的物质传播效应通过共振增强特征。剩余的无菌中微子基质元件保持固定,使用 |Ue4|2=0 和 δ14=0,因为它们的影响可以忽略不计,而 δ24=π 设置为给出最保守的限制。结果与非无菌中微子假说一致,概率为 4.3%。分析每个参数的可能性得到 90% 的置信水平:2.4eV2<Δm412<9.6eV2, 0.0081<|Uμ4|2<0.10 和 |Uτ4|2<0.035,这缩小了 |Uτ4|2.然而,该分析的主要结果是 3+1 参数空间的第一张映射,探索了 Δm412 的相互依赖性,|Uμ4|2 和 |Uτ4|2.
更新日期:2024-10-17
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