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New measurements of the coherent elastic neutrino-nucleus scattering (CEvNS) are expected to be achieved in the near future by using two neutrino production channels with different energy distributions: the very low energy electron…

High Energy Physics - Phenomenology · Physics 2020-02-19 B. C. Canas , E. A. Garces , O. G. Miranda , A. Parada , G. Sanchez Garcia

Neutrino oscillation experiments are known to be sensitive to Non-Standard Interactions (NSIs). We extend the NSI formalism to include one-loop effects. We discuss universal effects induced by corrections to the tree level W exchange, as…

High Energy Physics - Phenomenology · Physics 2015-05-20 Brando Bellazzini , Yuval Grossman , Itay Nachshon , Paride Paradisi

We analyze the possibility of probing non-standard neutrino interactions (NSI, for short) through the detection of neutrinos produced in a future galactic supernova (SN).We consider the effect of NSI on the neutrino propagation through the…

High Energy Physics - Phenomenology · Physics 2008-11-26 A. Esteban-Pretel , R. Tomàs , J. W. F. Valle

Models of radiative Majorana neutrino masses require new scalars and/or fermions to induce lepton number violating interactions. We show that these new particles also generate observable neutrino nonstandard interactions (NSI) with matter.…

High Energy Physics - Phenomenology · Physics 2020-03-06 K. S. Babu , P. S. Bhupal Dev , Sudip Jana , Anil Thapa

We explore the effects of non-standard neutrino interactions (NSI) and how they modify neutrino propagation in the Deep Underground Neutrino Experiment (DUNE). We find that NSI can significantly modify the data to be collected by the DUNE…

High Energy Physics - Phenomenology · Physics 2016-06-22 André de Gouvêa , Kevin J. Kelly

Non-standard interactions (NSI) between neutrinos and electrons can significantly modify the decoupling of neutrinos from the plasma. These interactions have two effects on the overall picture: (i) they alter neutrino oscillations though…

High Energy Physics - Phenomenology · Physics 2022-03-02 Pablo Martínez-Miravé

We analyze the energy and zenith angle distributions of the latest 2-year IceCube dataset of upward going atmospheric neutrinos to constrain sterile neutrinos at the eV scale in the 3+1 scenario. We find that the parameters favored by a…

High Energy Physics - Phenomenology · Physics 2016-08-17 Jiajun Liao , Danny Marfatia

We provide updated bounds on non-standard neutrino interactions based on data from the Planck satellite as well as auxiliary cosmological measurements. Two types of models are studied - A Fermi-like 4-point interaction and an interaction…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-17 Maria Archidiacono , Steen Hannestad

We consider the impact of non-standard interactions of neutrinos (NSI) on the determination of neutrino mixing parameters at a neutrino factory using $\pnu{e}\to\pnu{\mu}$ ``golden channels'' for the measurement of $\theta_{13}$. We show…

High Energy Physics - Phenomenology · Physics 2009-09-17 P. Huber , T. Schwetz , J. W. F. Valle

Compared to other neutrino sources, the huge anti-neutrino fluxes at nuclear reactor based experiments empower us to derive stronger bounds on non-standard interactions of neutrinos with electrons mediated by light scalar/vector mediators.…

High Energy Physics - Phenomenology · Physics 2023-04-12 Bhaskar Dutta , Sumit Ghosh , Tianjun Li , Adrian Thompson , Ankur Verma

The discovery of neutrino oscillations implies that neutrinos are massive and mixed, necessitating an extension of the Standard Model, which may require the introduction of non-standard neutrino interactions (NSI). We investigate the…

High Energy Physics - Phenomenology · Physics 2023-08-16 Sudip Jana , Sophie Klett

We investigate non-standard neutrino interactions (NSIs) in the Zee--Babu model. The size of NSIs predicted by this model is obtained from a full scan over the parameter space, taking into account constraints from low-energy experiments…

High Energy Physics - Phenomenology · Physics 2009-11-18 Tommy Ohlsson , Thomas Schwetz , He Zhang

Non-standard interactions in the propagation of neutrinos in matter can lead to significant deviations from expectations within the standard neutrino oscillation framework and atmospheric neutrino detectors have been considered to set…

High Energy Physics - Phenomenology · Physics 2017-03-08 Jordi Salvado , Olga Mena , Sergio Palomares-Ruiz , Nuria Rius

Non-standard interactions (NSI) of neutrinos with matter mediated by a scalar field would induce medium-dependent neutrino masses which can modify oscillation probabilities. Generating observable effects requires an ultra-light scalar…

High Energy Physics - Phenomenology · Physics 2020-06-03 K. S. Babu , Garv Chauhan , P. S. Bhupal Dev

Scalar non-standard neutrino interactions (sNSI) is a scenario where neutrinos can develop a medium dependent contribution to their mass due to a new scalar mediator. This scenario differs from the commonly discussed vector mediator case in…

High Energy Physics - Phenomenology · Physics 2025-02-05 Peter B. Denton , Alessio Giarnetti , Davide Meloni

This Letter reports a search for charge-parity ($CP$) symmetry violating nonstandard interactions (NSI) of neutrinos with matter using the NOvA Experiment, and examines their effects on the determination of the standard oscillation…

High Energy Physics - Experiment · Physics 2024-11-28 NOvA Collaboration , M. A. Acero , B. Acharya , P. Adamson , L. Aliaga , N. Anfimov , A. Antoshkin , E. Arrieta-Diaz , L. Asquith , A. Aurisano , A. Back , N. Balashov , P. Baldi , B. A. Bambah , A. Bat , K. Bays , R. Bernstein , T. J. C. Bezerra , V. Bhatnagar , D. Bhattarai , B. Bhuyan , J. Bian , A. C. Booth , R. Bowles , B. Brahma , C. Bromberg , N. Buchanan , A. Butkevich , S. Calvez , T. J. Carroll , E. Catano-Mur , J. P. Cesar , A. Chatla , S. Chaudhary , R. Chirco , B. C. Choudhary , A. Christensen , M. F. Cicala , T. E. Coan , A. Cooleybeck , C. Cortes-Parra , D. Coveyou , L. Cremonesi , G. S. Davies , P. F. Derwent , Z. Djurcic , M. Dolce , D. Doyle , D. Dueñas Tonguino , E. C. Dukes , A. Dye , R. Ehrlich , E. Ewart , P. Filip , J. Franc , M. J. Frank , H. R. Gallagher , F. Gao , A. Giri , R. A. Gomes , M. C. Goodman , M. Groh , R. Group , A. Habig , F. Hakl , J. Hartnell , R. Hatcher , M. He , K. Heller , V Hewes , A. Himmel , Y. Ivaneev , A. Ivanova , B. Jargowsky , J. Jarosz , C. Johnson , M. Judah , I. Kakorin , D. M. Kaplan , A. Kalitkina , J. Kleykamp , O. Klimov , L. W. Koerner , L. Kolupaeva , R. Kralik , A. Kumar , C. D. Kuruppu , V. Kus , T. Lackey , K. Lang , J. Lesmeister , A. Lister , J. Liu , J. A. Lock , M. Lokajicek , M. MacMahon , S. Magill , W. A. Mann , M. T. Manoharan , M. Manrique Plata , M. L. Marshak , M. Martinez-Casales , V. Matveev , B. Mehta , M. D. Messier , H. Meyer , T. Miao , V. Mikola , W. H. Miller , S. Mishra , S. R. Mishra , A. Mislivec , R. Mohanta , A. Moren , A. Morozova , W. Mu , L. Mualem , M. Muether , K. Mulder , D. Myers , D. Naples , A. Nath , S. Nelleri , J. K. Nelson , R. Nichol , E. Niner , A. Norman , A. Norrick , T. Nosek , H. Oh , A. Olshevskiy , T. Olson , M. Ozkaynak , A. Pal , J. Paley , L. Panda , R. B. Patterson , G. Pawloski , O. Petrova , R. Petti , L. R. Prais , A. Rafique , V. Raj , M. Rajaoalisoa , B. Ramson , M. Ravelhofer , B. Rebel , P. Roy , O. Samoylov , M. C. Sanchez , S. Sánchez Falero , P. Shanahan , P. Sharma , A. Shmakov , A. Sheshukov , S. Shukla , D. K. Singha , W. Shorrock , I. Singh , P. Singh , V. Singh , E. Smith , J. Smolik , P. Snopok , N. Solomey , A. Sousa , K. Soustruznik , M. Strait , L. Suter , A. Sutton , K. Sutton , S. Swain , C. Sweeney , A. Sztuc , B. Tapia Oregui , P. Tas , T. Thakore , J. Thomas , E. Tiras , Y. Torun , J. Tripathi , J. Trokan-Tenorio , J. Urheim , P. Vahle , Z. Vallari , J. Vasel , J. D. Villamil , K. J. Vockerodt , T. Vrba , M. Wallbank , M. Wetstein , D. Whittington , D. A. Wickremasinghe , T. Wieber , J. Wolcott , M. Wrobel , S. Wu , W. Wu , Y. Xiao , B. Yaeggy , A. Yahaya , A. Yankelevich , K. Yonehara , Y. Yu , S. Zadorozhnyy , J. Zalesak , R. Zwaska

We revisit the constraints on the properties of right handed neutrinos from the requirement to explain the observed light neutrino oscillation data in the type-I seesaw model. We use well-known relations to show that there is in general no…

High Energy Physics - Phenomenology · Physics 2019-05-03 Marco Drewes

In the standard interaction scenario, a direct measurement of absolute neutrino masses via neutrino oscillations is not feasible, as the oscillations depend only on the mass-squared differences. However, scalar non-standard interactions…

High Energy Physics - Phenomenology · Physics 2025-06-23 Abinash Medhi , Arnab Sarker , Moon Moon Devi

Neutrino experiments, in the next years, aim to determine with precision all the six parameters of the three-neutrino standard paradigm. The complete success of the experimental program is, nevertheless, attached to the non-existence (or at…

High Energy Physics - Phenomenology · Physics 2024-03-06 Adriano Cherchiglia , Jose Santiago

Many scenarios of new physics predict the existence of neutrino Non-Standard Interactions, new vector contact interactions between neutrinos and first generation fermions beyond the Standard Model. We obtain model-independent constraints on…

High Energy Physics - Phenomenology · Physics 2020-05-20 Jorge Terol-Calvo , Mariam Tórtola , Avelino Vicente
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