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There exists a puzzling disagreement between the results for the neutron lifetime obtained in experiments using the beam technique versus those relying on the bottle method. A possible explanation of this discrepancy postulates the…

High Energy Physics - Phenomenology · Physics 2023-10-18 Bartosz Fornal

The decay of massive neutrinos to final states containing only invisible particles is poorly constrained experimentally. In this letter we describe the constraints that can be put on neutrino mass and lifetime using CMBR measurements. We…

Astrophysics · Physics 2009-10-30 Steen Hannestad

We explore invisible neutrino decay in which a heavy active neutrino state decays into a light sterile neutrino state and present a comparative analysis of two baseline options, $540~$km and $360~$km, for the ESSnuSB experimental setup. Our…

High Energy Physics - Phenomenology · Physics 2021-06-02 Sandhya Choubey , Monojit Ghosh , Daniel Kempe , Tommy Ohlsson

We study the interplay of neutrino oscillation and invisible decay in atmospheric and long-baseline neutrinos experiments. We perform a global analysis of the full atmospheric data from Super-Kamiokande together with long-baseline K2K and…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. C. Gonzalez-Garcia , Michele Maltoni

We present the results of searches for nucleon decays via $p\rightarrow\nu\pi^{+}$ and $n\rightarrow\nu\pi^{0}$ using a 0.484 Mt$\cdot$yr exposure of Super-Kamiokande I-V data covering the entire pure water phase of the experiment. Various…

High Energy Physics - Experiment · Physics 2026-02-03 Kamiokande Collaboration , S. Jung , K. Abe , S. Abe , Y. Asaoka , M. Harada , Y. Hayato , K. Hiraide , K. Hosokawa , K. Ieki , M. Ikeda , J. Kameda , Y. Kanemura , Y. Kataoka , S. Miki , S. Mine , M. Miura , S. Moriyama , M. Nakahata , S. Nakayama , Y. Noguchi , G. Pronost , K. Sato , H. Sekiya , R. Shinoda , M. Shiozawa , Y. Suzuki , A. Takeda , Y. Takemoto , H. Tanaka , T. Yano , T. H. Hung , Y. Itow , T. Kajita , R. Nishijima , K. Okumura , T. Tashiro , T. Tomiya , X. Wang , P. Fernandez , L. Labarga , D. Samudio , B. Zaldivar , C. Yanagisawa , E. Kearns , L. Wan , T. Wester , B. W. Pointon , J. Bian , B. Cortez , N. J. Griskevich , Y. Jiang , M. B. Smy , H. W. Sobel , V. Takhistov , A. Yankelevich , J. Hill , M. C. Jang , S. H. Lee , D. H. Moon , R. G. Park , B. S. Yang , B. Bodur , K. Scholberg , C. W. Walter , A. Beauchêne , O. Drapier , A. Ershova , Th. A. Mueller , A. D. Santos , P. Paganini , C. Quach , R. Rogly , M. Ferey , T. Nakamura , J. S. Jang , R. P. Litchfield , L. N. Machado , F. J. P. Soler , J. G. Learned , K. Choi , S. Cao , L. H. V. Anthony , N. W. Prouse , M. Scott , Y. Uchida , V. Berardi , N. F. Calabria , M. G. Catanesi , N. Ospina , E. Radicioni , A. Langella , G. De Rosa , G. Collazuol , M. Feltre , M. Mattiazzi , L. Ludovici , M. Gonin , L. Périssé , B. Quilain , S. Horiuchi , A. Kawabata , M. Kobayashi , Y. M. Liu , Y. Maekawa , Y. Nishimura , R. Akutsu , M. Friend , T. Hasegawa , Y. Hino , T. Ishida , T. Kobayashi , M. Jakkapu , T. Matsubara , T. Nakadaira , Y. Oyama , A. Portocarrero Yrey , K. Sakashita , T. Sekiguchi , T. Tsukamoto , N. Bhuiyan , G. T. Burton , F. Di Lodovico , J. Gao , T. Katori , R. M. Ramsden , N. Latham , R. Kralik , H. Ito , T. Sone , A. T. Suzuki , Y. Takeuchi , S. Wada , H. Zhong , J. Feng , L. Feng , S. Han , J. Hikida , J. R. Hu , Z. Hu , M. Kawaue , T. Kikawa , T. Nakaya , T. V. Ngoc , R. A. Wendell , S. J. Jenkins , N. McCauley , A. Tarrant , M. Faní , M. J. Wilking , Z. Xie , Y. Fukuda , H. Menjo , Y. Yoshioka , J. Lagoda , M. Mandal , J. Zalipska , M. Mori , J. Jiang , K. Hamaguchi , H. Ishino , Y. Koshio , F. Nakanishi , T. Tada , T. Ishizuka , G. Barr , D. Barrow , L. Cook , S. Samani , D. Wark , A. Holin , F. Nova , J. Yoo , J. E. P. Fannon , L. Kneale , M. Malek , J. M. McElwee , T. Peacock , P. Stowell , M. D. Thiesse , L. F. Thompson , H. Okazawa , S. M. Lakshmi , E. Kwon , M. W. Lee , J. W. Seo , I. Yu , A. K. Ichikawa , K. D. Nakamura , S. Goto , S. Kodama , Y. Mizuno , T. Muro , K. Nakagiri , Y. Nakajima , N. Taniuchi , M. Yokoyama , H. Hayasaki , Y. Masaki , P. de Perio , S. Fujita , C. Jesús-Valls , K. Martens , Ll. Marti , K. M. Tsui , M. R. Vagins , J. Xia , M. Kuze , S. Izumiyama , R. Matsumoto , R. Asaka , M. Ishitsuka , M. Sugo , M. Wako , K. Yamauchi , Y. Nakano , F. Cormier , R. Gaur , M. Hartz , A. Konaka , X. Li , B. R. Smithers , S. Chen , Y. Wu , B. D. Xu , A. Q. Zhang , B. Zhang , M. Girgus , P. Govindaraj , M. Posiadala-Zezula , Y. S. Prabhu , H. Adhikary , S. B. Boyd , R. Edwards , D. Hadley , M. Nicholson , M. O'Flaherty , B. Richards , A. Ali , B. Jamieson , C. Bronner , D. Horiguchi , A. Minamino , Y. Sasaki , R. Shibayama , R. Shimamura

In this note, we analyze various constraints on the ``visible'' decay modes of a massive $\tau $ neutrino, $\nu_\tau\rightarrow\nu^\prime\,\gamma $ and $\nu_\tau\rightarrow\nu^\prime\, e^+ e^-$, where $\nu^\prime$ is a light neutrino. The…

High Energy Physics - Phenomenology · Physics 2008-11-26 K. S. Babu , T. M. Gould , I. Z. Rothstein

As we have pointed out in (arXiv:1806.10107 [hep-ph]), the existence of neutron dark matter decay modes "n -> chi + anything", where "chi" is a dark matter fermion, for the solution of the neutron lifetime problem changes priorities and…

High Energy Physics - Phenomenology · Physics 2018-12-05 A. N. Ivanov , R. Höllwieser , N. I. Troitskaya , M. Wellenzohn , Ya. A. Berdnikov

New decay channels for the neutron into dark matter plus other particles have been suggested for explaining a long-standing discrepancy between the neutron lifetime measured from trapped neutrons versus those decaying in flight. Many such…

High Energy Physics - Phenomenology · Physics 2018-07-16 James M. Cline , Jonathan M. Cornell

The trilepton nucleon decay modes $p \rightarrow e^+ \nu \nu$ and $p \rightarrow \mu^+ \nu \nu$ violate $|\Delta (B - L)|$ by two units. Using data from a 273.4 kiloton year exposure of Super-Kamiokande a search for these decays yields a…

High Energy Physics - Experiment · Physics 2014-09-09 V. Takhistov , K. Abe , Y. Haga , Y. Hayato , M. Ikeda , K. Iyogi , J. Kameda , Y. Kishimoto , M. Miura , S. Moriyama , M. Nakahata , Y. Nakano , S. Nakayama , H. Sekiya , M. Shiozawa , Y. Suzuki , A. Takeda , H. Tanaka , T. Tomura , K. Ueno , R. A. Wendell , T. Yokozawa , T. Irvine , T. Kajita , I. Kametani , K. Kaneyuki , K. P. Lee , T. McLachlan , Y. Nishimura , E. Richard , K. Okumura , L. Labarga , P. Fernandez , S. Berkman , H. A. Tanaka , S. Tobayama , J. Gustafson , E. Kearns , J. L. Raaf , J. L. Stone , L. R. Sulak , M. Goldhaber , G. Carminati , W. R. Kropp , S. Mine , P. Weatherly , A. Renshaw , M. B. Smy , H. W. Sobel , K. S. Ganezer , B. L. Hartfiel , J. Hill , W. E. Keig , N. Hong , J. Y. Kim , I. T. Lim , T. Akiri , A. Himmel , K. Scholberg , C. W. Walter , T. Wongjirad , T. Ishizuka , S. Tasaka , J. S. Jang , J. G. Learned , S. Matsuno , S. N. Smith , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , A. T. Suzuki , Y. Takeuchi , C. Bronner , S. Hirota , K. Huang , K. Ieki , T. Kikawa , A. Minamino , A. Murakami , T. Nakaya , K. Suzuki , S. Takahashi , K. Tateishi , Y. Fukuda , K. Choi , Y. Itow , G. Mitsuka , P. Mijakowski , J. Hignight , J. Imber , C. K. Jung , C. Yanagisawa , H. Ishino , A. Kibayashi , Y. Koshio , T. Mori , M. Sakuda , R. Yamaguchi , T. Yano , Y. Kuno , R. Tacik , S. B. Kim , H. Okazawa , Y. Choi , K. Nishijima , M. Koshiba , Y. Suda , Y. Totsuka , M. Yokoyama , K. Martens , Ll. Marti , M. R. Vagins , J. F. Martin , P. de Perio , A. Konaka , M. J. Wilking , S. Chen , Y. Zhang , K. Connolly , R. J. Wilkes

Neutrinos mix and have mass differences, so decays from one to another must occur. But how fast? The best direct limits on non-radiative decays, based on solar and atmospheric neutrinos, are weak, $\tau \gtrsim 10^{-3}$ s ($m$/eV) or much…

High Energy Astrophysical Phenomena · Physics 2017-03-29 Mauricio Bustamante , John F. Beacom , Kohta Murase

We propose to search for the neutrino radiative decay by fitting a photon energy spectrum of the cosmic infrared background to a sum of the photon energy spectrum from the neutrino radiative decay and a continuum. By comparing the present…

High Energy Physics - Phenomenology · Physics 2012-01-19 Shin-Hong Kim , Ken-ichi Takemasa , Yuji Takeuchi , Shuji Matsuura

An upper limit for the tau-neutrino mass has been determined from the decay tau -> 5pi+- \nu_tau using data collected with the OPAL detector from 1991 to 1995 in e+e- collisions at \sqrt{s} ~ M_Z. A limit of 43.2 MeV at 95% CL is obtained…

High Energy Physics - Experiment · Physics 2008-11-26 The OPAL Collaboration , K. Ackerstaff et al

The large distances travelled by neutrinos emitted from the Sun and core-collapse supernovae together with the characteristic energy of such neutrinos provide ideal conditions to probe their lifetime, when the decay products evade…

High Energy Astrophysical Phenomena · Physics 2024-05-07 Pablo Martínez-Miravé , Irene Tamborra , Mariam Tórtola

We report an improved measurement of the free neutron lifetime $\tau_{n}$ using the UCN$\tau$ apparatus at the Los Alamos Neutron Science Center. We counted a total of approximately $38\times10^{6}$ surviving ultracold neutrons (UCN) after…

We calculate the ground, first intrinsic excited states and density distribution for neutron-rich thorium and uranium isotopes, within the framework of relativistic mean field(RMF) approach using axially deformed basis. The total nucleon…

Nuclear Theory · Physics 2016-03-01 B. Kumar , S. K. Biswal , S. K. Singh , C. Lahiri , S. K. Patra

We study the lifetimes of TeV-scale heavy neutral leptons (Majorana neutrinos) that appear in a model suggested by Okamura et al. [2]. We develop a convenient way to parametrize the neutrino mass texture of the model, and illustrate our…

High Energy Physics - Phenomenology · Physics 2009-09-29 Alexey Pronin , Tatsu Takeuchi

The structure and decay of $^{26}$O are investigated in a three-body $^{24}$O+$n+n$ model suitable for studies of the long-lived (including radioactivity timescale) states. We have found extremely strong effect of the subbarrier…

Nuclear Theory · Physics 2015-06-15 L. V. Grigorenko , I. G. Mukha , M. V. Zhukov

Evidence for Nucleon Decay has yet to be observed. Current results from the observation of a 45 kton-year exposure of Super-Kamiokande and lifetime limits for nucleons to decay via lepton + pion, lepton + eta and lepton + kaon modes are…

High Energy Physics - Experiment · Physics 2007-05-23 Brett Viren

Discrepancies from in-beam and in-bottle type experiments measuring the neutron lifetime are on the 4$\sigma$ standard deviation level. In a recent publication Fornal and Grinstein proposed that the puzzle could be solved if the neutron…

High Energy Physics - Experiment · Physics 2019-06-12 M. Klopf , E. Jericha , B. Märkisch , H. Saul , T. Soldner , H. Abele

The next-generation water Cherenkov Hyper-Kamiokande detector will be able to detect thousands of neutrino events from a galactic Supernova explosion via Inverse Beta Decay processes followed by neutron capture on Gadolinium. This superb…

High Energy Physics - Phenomenology · Physics 2023-10-10 Federica Pompa , Olga Mena