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Assuming Majorana neutrinos, we infer from oscillation data the expected values of the parameters m_{nu_e} and m_{ee} probed by beta and 0nu2beta-decay experiments. If neutrinos have a `normal hierarchy' we get the 90% CL ranges |m_{ee}| =…

High Energy Physics - Phenomenology · Physics 2009-10-09 Ferruccio Feruglio , Alessandro Strumia , Francesco Vissani

We study a minimal extension of the Standard Model where a scalar field is coupled to the right handed neutrino responsible for the see-saw mechanism for neutrino masses. In the absence of other couplings, below 8 TeV the scalar $A$ has a…

High Energy Physics - Phenomenology · Physics 2015-04-08 Emilian Dudas , Yann Mambrini , Keith Olive

We study the contribution of massive dominantly sterile neutrinos, $N$, to the Lepton Number and Lepton Flavor Violating semileptonic decays of $\tau$ and $B, D, K$-mesons. We focus on special domains of sterile neutrino masses $m_{N}$…

High Energy Physics - Phenomenology · Physics 2013-08-27 Juan Carlos Helo , Sergey Kovalenko , Ivan Schmidt

Neutrino oscillation experiments provide a unique window in exploring several new physics scenarios beyond the standard three flavour. One such scenario is quantum decoherence in neutrino oscillation which tends to destroy the interference…

Determination of the neutrino mass ordering (NMO) is one of the biggest priorities in the intensity frontier of high energy particle physics. To accomplish that goal a lot of efforts are being put together with the atmospheric, solar,…

High Energy Physics - Phenomenology · Physics 2021-01-05 Francesco Capozzi , Sabya Sachi Chatterjee , Antonio Palazzo

The electron would decay into a photon and neutrino if the law of electric charge conservation is not respected. Such a decay would cause vacancy in closed shells of atoms giving rise to emission of x-rays and Auger electrons. Experimental…

High Energy Physics - Theory · Physics 2007-05-23 T. Pradhan

We examine a phenomenon recently predicted by numerical simulations of supernova neutrino flavor evolution: the swapping of supernova $\nu_e$ and $\nu_{\mu,\tau}$ energy spectra below (above) energy $\EC$ for the normal (inverted) neutrino…

Astrophysics · Physics 2008-11-26 Huaiyu Duan , George M. Fuller , J. Carlson , Yong-Zhong Qian

We study a model where the Standard Model is augmented with three sterile neutrinos. By adopting a particular parameterization of a $(6\times6)$ unitary matrix - in this context, light neutrino masses being generated via a type-I seesaw…

High Energy Physics - Phenomenology · Physics 2024-07-17 Debashree Priyadarsini Das , Sasmita Mishra

Recent Super-Kamiokande data have greatly strengthened the hypothesis that the atmospheric neutrino anomaly is mainly due to nearly maximal oscillations between $\nu_{\mu}$ and either $\nu_{\tau}$ or a sterile neutrino $\nu^s_{\mu}$.In this…

Astrophysics · Physics 2007-05-23 D. W. Sciama

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 estimate constraints on the existence of a heavy, mostly sterile neutrino with mass between 10 eV and 1 TeV. We improve upon previous analyses by performing a global combination and expanding the experimental inputs to simultaneously…

High Energy Physics - Phenomenology · Physics 2016-02-17 André de Gouvêa , Andrew Kobach

Present status, and future plans for Double Beta Decay searches are reviewed. Given the recent observations of neutrino oscillations, a possibility to observe $\beta\beta(0\nu)$~ at a neutrino mass scale suggested by present experimental…

High Energy Physics - Experiment · Physics 2011-07-19 Oliviero Cremonesi

Recently the Sudbury Neutrino Observatory (SNO) has measured both the rates as well as the day-night asymmetries in the flux of neutrinos from the Sun in the charged-current (CC), neutral-current (NC) and elastic scattering (ES) channels.…

High Energy Physics - Phenomenology · Physics 2007-05-23 D. Indumathi

The explanation of various observed phenomena such as large angle neutrino oscillations, hierarchies of charged fermion masses and CKM mixings, and apparent baryon number conservation may have a common origin. We show how this could occur…

High Energy Physics - Phenomenology · Physics 2011-05-12 Qaisar Shafi , Zurab Tavartkiladze

We critically examine the ability of future neutrino telescopes, including Baikal-GVD, KM3NeT, P-ONE, TAMBO, and IceCube-Gen2, to determine the flavor composition of high-energy astrophysical neutrinos, ie, the relative number of $\nu_e$,…

High Energy Physics - Phenomenology · Physics 2021-04-28 Ningqiang Song , Shirley Weishi Li , Carlos A. Argüelles , Mauricio Bustamante , Aaron C. Vincent

We calculate constraints on radiatively decaying neutrinos from the recent detection of singly ionized helium in the diffuse intergalactic medium (IGM) at $z \simeq 3.3$. We consider a model in which neutrinos predominantly decay into…

Astrophysics · Physics 2010-11-30 Shiv K. Sethi

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 $\nu_\mu+\overline{\nu}_\mu$ charged-current interactions in the energy range 500--9976 GeV. Our…

High Energy Physics - Experiment · Physics 2024-10-23 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 , S. Jain , 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 , 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 , V. Palusova , 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 , L. Schlickmann , 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

This paper reports results from a search for nucleon decay through 'invisible' modes, where no visible energy is directly deposited during the decay itself, during the initial water phase of SNO+. However, such decays within the oxygen…

High Energy Physics - Experiment · Physics 2019-08-12 SNO+ Collaboration , : , M. Anderson , S. Andringa , E. Arushanova , S. Asahi , M. Askins , D. J. Auty , A. R. Back , Z. Barnard , N. Barros , D. Bartlett , F. Barão , R. Bayes , E. W. Beier , A. Bialek , S. D. Biller , E. Blucher , R. Bonventre , M. Boulay , D. Braid , E. Caden , E. J. Callaghan , J. Caravaca , J. Carvalho , L. Cavalli , D. Chauhan , M. Chen , O. Chkvorets , K. J. Clark , B. Cleveland , C. Connors , I. T. Coulter , D. Cressy , X. Dai , C. Darrach , B. Davis-Purcell , M. M. Depatie , F. Descamps , F. Di Lodovico , N. Duhaime , F. Duncan , J. Dunger , E. Falk , N. Fatemighomi , V. Fischer , E. Fletcher , R. Ford , N. Gagnon , K. Gilje , P. Gorel , K. Graham , C. Grant , J. Grove , S. Grullon , E. Guillian , A. L. Hallin , D. Hallman , S. Hans , J. Hartnell , P. Harvey , M. Hedayatipour , W. J. Heintzelman , J. Heise , R. L. Helmer , J. L. Hernández-Hernández , B. Hreljac , J. Hu , T. Iida , A. S. Inácio , C. M. Jackson , N. A. Jelley , C. J. Jillings , C. Jones , P. G. Jones , K. Kamdin , T. Kaptanoglu , J. Kaspar , K. Keeter , C. Kefelian , P. Khaghani , L. Kippenbrock , J. R. Klein , R. Knapik , J. Kofron , L. L. Kormos , B. Krar , C. Kraus , C. B. Krauss , T. Kroupova , K. Labe , I. Lam , C. Lan , B. J. Land , R. Lane , S. Langrock , A. LaTorre , I. Lawson , L. Lebanowski , G. M. Lefeuvre , E. J. Leming , A. Li , J. Lidgard , B. Liggins , X. Liu , Y. Liu , V. Lozza , M. Luo , S. Maguire , A. Maio , K. Majumdar , S. Manecki , J. Maneira , R. D. Martin , E. Marzec , A. Mastbaum , N. McCauley , A. B. McDonald , J. E. McMillan , P. Mekarski , M. Meyer , C. Miller , M. Mlejnek , E. Mony , I. Morton-Blake , M. J. Mottram , S. Nae , M. Nirkko , V. Novikov , H. M. O'Keeffe , E. O'Sullivan , G. D. Orebi Gann , M. J. Parnell , J. Paton , S. J. M. Peeters , T. Pershing , Z. Petriw , L. Pickard , D. Pracsovics , G. Prior , J. C. Prouty , S. Quirk , A. Reichold , R. Richardson , M. Rigan , A. Robertson , J. Rose , R. Rosero , P. M. Rost , J. Rumleskie , M. A. Schumaker , M. H. Schwendener , D. Scislowski , J. Secrest , M. Seddighin , L. Segui , S. Seibert , I. Semenec , T. Shantz , T. M. Shokair , L. Sibley , J. R. Sinclair , K. Singh , P. Skensved , T. Sonley , R. Stainforth , M. Strait , M. I. Stringer , R. Svoboda , A. Sörensen , B. Tam , J. Tatar , L. Tian , N. Tolich , J. Tseng , H. W. C. Tseung , E. Turner , R. Van Berg , J. G. C. Veinot , C. J. Virtue , B. von Krosigk , E. Vázquez-Jáuregui , J. M. G. Walker , M. Walker , J. Wang , O. Wasalski , J. Waterfield , J. J. Weigand , R. F. White , J. R. Wilson , T. J. Winchester , P. Woosaree , A. Wright , J. P. Yanez , M. Yeh , T. Zhao , K. Zuber , A. Zummo

In this work we present an updated study of the flavor composition suggested by astrophysical neutrinos observed by IceCube. The main novelties compared to previous studies are the following: 1) we use the most recent measurements, namely 8…

High Energy Astrophysical Phenomena · Physics 2020-08-10 Andrea Palladino

Present limits on neutrino masses are briefly reviewed, along with cosmological and astrophysical hints from dark matter, solar and atmospheric neutrino observations that suggest neutrino masses. These would imply many possible new…

High Energy Physics - Phenomenology · Physics 2009-09-25 JosÉ W. F. Valle
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