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Related papers: Loop-induced Neutrino Non-Standard Interactions

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In neutrino interactions with nucleons and nuclei, Shallow Inelastic Scattering (SIS) refers to processes, dominated by non-resonant contributions, in the kinematic region where $Q^2$ is small and the invariant mass of the hadronic system,…

We explore the role of matter effect in the evolution of neutrino oscillation parameters in the presence of lepton-flavor-conserving and lepton-flavor-violating neutral-current non-standard interactions (NSI) of the neutrino. We derive…

High Energy Physics - Phenomenology · Physics 2021-12-01 Sanjib Kumar Agarwalla , Sudipta Das , Mehedi Masud , Pragyanprasu Swain

Many new physics scenarios predict the existence of the extra charged gauge boson $ W'$, which can induce the charged-current (CC) non-standard neutrino interactions (NSI). We investigate the constraints on the CC NSI in model-independent…

High Energy Physics - Phenomenology · Physics 2021-02-03 ChongXing Yue , XueJia Cheng

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

Understanding the pion generation and the consequences of final-state interactions (FSI) are critical for the data processing in all neutrino experiments. The energy utilized in modern neutrino research of the resonance (RES) generation…

High Energy Physics - Phenomenology · Physics 2022-09-01 Ritu Devi , Baba Potukuchi

We have reconsidered the atmospheric neutrino anomaly in light of the laetst data from Super-Kamiokande contained events and from Super-Kamiokande and MACRO up-going muons. We have reanalysed the proposed solution to the atmospheric…

High Energy Physics - Phenomenology · Physics 2010-05-28 N. Fornengo , M. Maltoni , R. Tomas , J. W. F. Valle

The detection of coherent neutrino-nucleus scattering by the COHERENT collaboration has set on quantitative grounds the existence of an irreducible neutrino background in direct detection searches of Weakly Interacting Massive Dark Matter…

High Energy Physics - Phenomenology · Physics 2018-07-06 M. C. Gonzalez-Garcia , Michele Maltoni , Yuber F. Perez-Gonzalez , Renata Zukanovich Funchal

We formulate an alternative approach based on unitarity triangles to describe neutrino oscillations in presence of non-standard interactions (NSI). Using perturbation theory, we derive the expression for the oscillation probability in case…

High Energy Physics - Phenomenology · Physics 2023-01-11 Mehedi Masud , Poonam Mehta , Christoph A. Ternes , Mariam Tortola

We report new constraints on flavor-changing non-standard neutrino interactions from the MINOS long-baseline experiment using $\nu_{e}$ and $\bar{\nu}_{e}$ appearance candidate events from predominantly $\nu_{\mu}$ and $\bar{\nu}_{\mu}$…

High Energy Physics - Experiment · Physics 2017-01-18 P. Adamson , I. Anghel , A. Aurisano , G. Barr , M. Bishai , A. Blake , G. J. Bock , D. Bogert , S. V. Cao , T. J. Carroll , C. M. Castromonte , R. Chen , S. Childress , J. A. B. Coelho , L. Corwin , D. Cronin-Hennessy , J. K. de Jong , S. de Rijck , A. V. Devan , N. E. Devenish , M. V. Diwan , C. O. Escobar , J. J. Evans , E. Falk , G. J. Feldman , W. Flanagan , M. V. Frohne , M. Gabrielyan , H. R. Gallagher , S. Germani , R. A. Gomes , M. C. Goodman , P. Gouffon , N. Graf , R. Gran , K. Grzelak , A. Habig , S. R. Hahn , J. Hartnell , R. Hatcher , A. Holin , J. Huang , J. Hylen , G. M. Irwin , Z. Isvan , C. James , D. Jensen , T. Kafka , S. M. S. Kasahara , G. Koizumi , M. Kordosky , A. Kreymer , K. Lang , J. Ling , P. J. Litchfield , P. Lucas , W. A. Mann , M. L. Marshak , N. Mayer , C. McGivern , M. M. Medeiros , R. Mehdiyev , J. R. Meier , M. D. Messier , W. H. Miller , S. R. Mishra , S. Moed Sher , C. D. Moore , L. Mualem , J. Musser , D. Naples , J. K. Nelson , H. B. Newman , R. J. Nichol , J. A. Nowak , J. O'Connor , M. Orchanian , R. B. Pahlka , J. Paley , R. B. Patterson , G. Pawloski , A. Perch , M. M. Pfützner , D. D. Phan , S. Phan-Budd , R. K. Plunkett , N. Poonthottathil , X. Qiu , A. Radovic , B. Rebel , C. Rosenfeld , H. A. Rubin , P. Sail , M. C. Sanchez , J. Schneps , A. Schreckenberger , P. Schreiner , R. Sharma , A. Sousa , N. Tagg , R. L. Talaga , J. Thomas , M. A. Thomson , X. Tian , A. Timmons , J. Todd , S. C. Tognini , R. Toner , D. Torretta , G. Tzanakos , J. Urheim , P. Vahle , B. Viren , A. Weber , R. C. Webb , C. White , L. Whitehead , L. H. Whitehead , S. G. Wojcicki , R. Zwaska

We study generalized neutrino interactions (GNI) for several neutrino processes, including neutrinos from electron-positron collisions, neutrino-electron scattering, and neutrino deep inelastic scattering. We constrain scalar, pseudoscalar,…

High Energy Physics - Phenomenology · Physics 2021-07-20 F. J. Escrihuela , L. J. Flores , O. G. Miranda , Javier Rendón

Atmospheric neutrinos provide a unique avenue to study neutrino interactions in matter. In this work, the prospects of constraining non-standard neutrino interactions with atmospheric neutrino oscillations are investigated for the proposed…

The low-energy threshold and the large detector size of Precision IceCube Next Generation Upgrade (PINGU) can make the study on neutrino oscillations with a planet-scale baseline possible. In this task, we consider the configuration that…

High Energy Physics - Phenomenology · Physics 2019-12-25 Wei-Jie Feng , Jian Tang , Tse-Chun Wang , Yi-Xing Zhou

We explore, for the first time, {\textit{neutral-current}} events at long-baseline experiments to constrain vector and axial-vector neutrino non-standard interactions (NSI) with quarks. We leverage the flavor dependence of NSIs to perform…

High Energy Physics - Phenomenology · Physics 2025-05-20 Julia Gehrlein , Pedro A. N. Machado , João Paulo Pinheiro

Neutrino flavour oscillation is one of the primary indication of the existence of new physics beyond standard model. The presence of small neutrino mass is indispensable to explicate the oscillation among different flavours of neutrino. By…

High Energy Physics - Phenomenology · Physics 2023-01-31 Trisha Sarkar

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

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

We discuss about effects of the non-standard interaction of neutrinos with matter on the nu_e appearance search in the MINOS experiment. We consider the effects of the complex phase of the interaction and of the uncertainty on theta_23…

High Energy Physics - Phenomenology · Physics 2008-11-26 Hiroaki Sugiyama

Neutrino oscillations in matter provide a unique probe of new physics. Leveraging the advent of neutrino appearance data from NOvA and T2K in recent years, we investigate the presence of CP-violating neutrino non-standard interactions in…

High Energy Physics - Phenomenology · Physics 2021-02-05 Peter B. Denton , Julia Gehrlein , Rebekah Pestes

The Standard Model Effective Field Theory (SMEFT) provides a systematic and model-independent framework to study neutrino non-standard interactions (NSIs). We study the constraining power of the on-going neutrino oscillation experiments…

High Energy Physics - Phenomenology · Physics 2021-03-17 Yong Du , Hao-Lin Li , Jian Tang , Sampsa Vihonen , Jiang-Hao Yu

Non-Standard Interactions (NSI) of neutrinos with matter has received renewed interest in recent years. In particular, it has been shown that NSI can reconcile the $3+1$ solution with IceCube atmospheric data with $E_\nu >500$ GeV, provided…

High Energy Physics - Phenomenology · Physics 2019-02-08 Peter B. Denton , Yasaman Farzan , Ian M. Shoemaker
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