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Entropy changes due to delocalization and decoherence effects should modify the predictions for the cosmological neutrino background (C$\nu$B) temperature when one treats neutrino flavors in the framework of composite quantum systems.…

Cosmology and Nongalactic Astrophysics · Physics 2013-09-30 Alex E. Bernardini

Non-Standard neutrino Interactions (NSI) are vector contact interactions involving two neutrinos and two first generation fermions, which can affect neutrino propagation in matter. SU(2) gauge invariance suggests that NSI should be…

High Energy Physics - Phenomenology · Physics 2020-02-24 Sacha Davidson , Martin Gorbahn

It is generally expected that adding light sterile species would increase the effective number of neutrinos, $N_{eff}$. In this paper we discuss a scenario that $N_{eff}$ can actually decrease due to the neutrino oscillation effect if…

High Energy Physics - Phenomenology · Physics 2015-09-25 Yong Tang

The standard cosmological model predicts the existence of a cosmic neutrino background with a present density of about 110 cm^{-3} per flavour, which affects big-bang nucleosynthesis, cosmic microwave background anisotropies, and the…

Astrophysics · Physics 2009-11-11 P. D. Serpico

Precision cosmology enables to test fundamental physics, including neutrino properties, with unprecedented accuracy. In this work, I review the basics of neutrino cosmology. I briefly describe how neutrinos affect cosmological observables,…

Cosmology and Nongalactic Astrophysics · Physics 2018-04-02 Martina Gerbino

We perform a comprehensive study of cosmological constraints on non-standard neutrino self-interactions using cosmic microwave background (CMB) and baryon acoustic oscillation data. We consider different scenarios for neutrino…

Cosmology and Nongalactic Astrophysics · Physics 2021-09-22 Thejs Brinckmann , Jae Hyeok Chang , Marilena LoVerde

The presence of nonstandard neutrino interactions (NSI) has a large effect on the precision measurements at next generation neutrino oscillation experiments. Other type of experiments are needed to constrain the NSI parameter space. We…

High Energy Physics - Phenomenology · Physics 2021-09-08 Jiajun Liao , Yu Zhang

We investigate the effects of a Non-Standard Interaction (NSI) extension of the standard model of particle physics on solar neutrino flavour oscillations. This NSI model introduces a $U_{Z^\prime}(1)$ gauge symmetry through a $Z^\prime$…

High Energy Physics - Phenomenology · Physics 2023-08-31 Ilídio Lopes

We study the sensitivity of current and future long-baseline neutrino oscillation experiments to the effects of dimension six operators affecting neutrino propagation through Earth, commonly referred to as Non-Standard Interactions (NSI).…

High Energy Physics - Phenomenology · Physics 2016-03-23 Pilar Coloma

We report constraints on nonstandard neutrino interactions (NSI) from the observation of atmospheric neutrinos with IceCube, limiting all individual coupling strengths from a single dataset. Furthermore, IceCube is the first experiment to…

High Energy Physics - Experiment · Physics 2021-10-19 IceCube Collaboration , R. Abbasi , M. Ackermann , J. Adams , J. A. Aguilar , M. Ahlers , M. Ahrens , C. Alispach , A. A. Alves , N. M. Amin , R. An , K. Andeen , T. Anderson , I. Ansseau , G. Anton , C. Argüelles , Y. Ashida , S. Axani , X. Bai , A. Balagopal V. , A. Barbano , S. W. Barwick , B. Bastian , V. Basu , S. Baur , R. Bay , J. J. Beatty , K. -H. Becker , J. Becker Tjus , C. Bellenghi , S. BenZvi , D. Berley , E. Bernardini , D. Z. Besson , G. Binder , D. Bindig , E. Blaufuss , S. Blot , F. Bontempo , J. Borowka , S. Böser , O. Botner , J. Böttcher , E. Bourbeau , F. Bradascio , J. Braun , S. Bron , J. Brostean-Kaiser , S. Browne , A. Burgman , R. S. Busse , M. A. Campana , C. Chen , D. Chirkin , K. Choi , B. A. Clark , K. Clark , L. Classen , A. Coleman , G. H. Collin , J. M. Conrad , P. Coppin , P. Correa , D. F. Cowen , R. Cross , P. Dave , C. De Clercq , J. J. DeLaunay , H. Dembinski , K. Deoskar , S. De Ridder , A. Desai , P. Desiati , K. D. de Vries , G. de Wasseige , M. de With , T. DeYoung , S. Dharani , A. Diaz , J. C. Díaz-Vélez , H. Dujmovic , M. Dunkman , M. A. DuVernois , E. Dvorak , T. Ehrhardt , P. Eller , R. Engel , H. Erpenbeck , J. Evans , P. A. Evenson , A. R. Fazely , S. Fiedlschuster , A. T. Fienberg , K. Filimonov , C. Finley , L. Fischer , D. Fox , A. Franckowiak , E. Friedman , A. Fritz , P. Fürst , T. K. Gaisser , J. Gallagher , E. Ganster , A. Garcia , S. Garrappa , L. Gerhardt , A. Ghadimi , C. Glaser , T. Glauch , T. Glüsenkamp , A. Goldschmidt , J. G. Gonzalez , S. Goswami , D. Grant , T. Grégoire , S. Griswold , M. Gündüz , C. Günther , C. Haack , A. Hallgren , R. Halliday , L. Halve , F. Halzen , M. Ha Minh , K. Hanson , J. Hardin , A. A. Harnisch , A. Haungs , S. Hauser , D. Hebecker , K. Helbing , F. Henningsen , E. C. Hettinger , S. Hickford , J. Hignight , C. Hill , G. C. Hill , K. D. Hoffman , R. Hoffmann , T. Hoinka , B. Hokanson-Fasig , K. Hoshina , F. Huang , M. Huber , T. Huber , K. Hultqvist , M. Hünnefeld , R. Hussain , S. In , N. Iovine , A. Ishihara , M. Jansson , G. S. Japaridze , M. Jeong , B. J. P. Jones , R. Joppe , D. Kang , W. Kang , X. Kang , A. Kappes , D. Kappesser , T. Karg , M. Karl , A. Karle , U. Katz , M. Kauer , M. Kellermann , J. L. Kelley , A. Kheirandish , K. Kin , T. Kintscher , J. Kiryluk , S. R. Klein , R. Koirala , H. Kolanoski , T. Kontrimas , L. Köpke , C. Kopper , S. Kopper , D. J. Koskinen , P. Koundal , M. Kovacevich , M. Kowalski , N. Kurahashi , A. Kyriacou , N. Lad , C. Lagunas Gualda , J. L. Lanfranchi , M. J. Larson , F. Lauber , J. P. Lazar , J. W. Lee , K. Leonard , A. Leszczyńska , Y. Li , M. Lincetto , Q. R. Liu , M. Liubarska , E. Lohfink , C. J. Lozano Mariscal , L. Lu , F. Lucarelli , A. Ludwig , W. Luszczak , Y. Lyu , W. Y. Ma , J. Madsen , K. B. M. Mahn , Y. Makino , S. Mancina , I. C. Mariş , R. Maruyama , K. Mase , T. McElroy , F. McNally , K. Meagher , A. Medina , M. Meier , S. Meighen-Berger , J. Merz , J. Micallef , D. Mockler , T. Montaruli , R. W. Moore , R. Morse , M. Moulai , R. Naab , R. Nagai , U. Naumann , J. Necker , L. V. Nguyên , H. Niederhausen , M. U. Nisa , S. C. Nowicki , D. R. Nygren , A. Obertacke Pollmann , M. Oehler , A. Olivas , E. O'Sullivan , H. Pandya , D. V. Pankova , N. Park , G. K. Parker , E. N. Paudel , L. Paul , C. Pérez de los Heros , S. Philippen , D. Pieloth , S. Pieper , M. Pittermann , A. Pizzuto , M. Plum , Y. Popovych , A. Porcelli , M. Prado Rodriguez , P. B. Price , B. Pries , G. T. Przybylski , C. Raab , A. Raissi , M. Rameez , K. Rawlins , I. C. Rea , A. Rehman , R. Reimann , G. Renzi , E. Resconi , S. Reusch , W. Rhode , M. Richman , B. Riedel , S. Robertson , G. Roellinghoff , M. Rongen , C. Rott , T. Ruhe , D. Ryckbosch , D. Rysewyk Cantu , I. Safa , J. Saffer , S. E. Sanchez Herrera , A. Sandrock , J. Sandroos , M. Santander , S. Sarkar , S. Sarkar , K. Satalecka , M. Scharf , M. Schaufel , H. Schieler , P. Schlunder , T. Schmidt , A. Schneider , J. Schneider , F. G. Schröder , L. Schumacher , S. Sclafani , D. Seckel , S. Seunarine , A. Sharma , S. Shefali , M. Silva , B. Skrzypek , B. Smithers , R. Snihur , J. Soedingrekso , D. Soldin , C. Spannfellner , G. M. Spiczak , C. Spiering , J. Stachurska , M. Stamatikos , T. Stanev , R. Stein , J. Stettner , A. Steuer , T. Stezelberger , T. Stürwald , T. Stuttard , G. W. Sullivan , I. Taboada , F. Tenholt , S. Ter-Antonyan , A. Terliuk , S. Tilav , F. Tischbein , K. Tollefson , L. Tomankova , C. Tönnis , S. Toscano , D. Tosi , A. Trettin , M. Tselengidou , C. F. Tung , A. Turcati , R. Turcotte , C. F. Turley , J. P. Twagirayezu , B. Ty , M. A. Unland Elorrieta , N. Valtonen-Mattila , J. Vandenbroucke , N. van Eijndhoven , D. Vannerom , J. van Santen , S. Verpoest , M. Vraeghe , C. Walck , A. Wallace , T. B. Watson , C. Weaver , P. Weigel , A. Weindl , M. J. Weiss , J. Weldert , C. Wendt , J. Werthebach , M. Weyrauch , B. J. Whelan , N. Whitehorn , C. H. Wiebusch , D. R. Williams , M. Wolf , K. Woschnagg , G. Wrede , J. Wulff , X. W. Xu , Y. Xu , J. P. Yanez , S. Yoshida , S. Yu , T. Yuan , Z. Zhang

Neutrino-electron scatterings are purely leptonic processes with robust Standard Model (SM) predictions. Their measurements can therefore provide constraints to physics beyond SM. The $\nuebar$-e data taken at the Kuo-Sheng Reactor Neutrino…

High Energy Physics - Phenomenology · Physics 2014-11-21 M. Deniz er al. , TEXONO Collaboration

We consider the effect of non-standard neutrino interactions (NSI, for short) on the propagation of neutrinos through the supernova (SN) envelope within a three-neutrino framework and taking into account the presence of a neutrino…

High Energy Physics - Phenomenology · Physics 2010-04-06 A. Esteban-Pretel , R. Tomas , J. W. F. Valle

The neutral-current (NC) non-standard interactions (NSI) of neutrinos with fermions can modify the flavor oscillations of atmospheric neutrinos as they propagate through the Earth. We present constraints on the NC-NSI parameters…

High Energy Physics - Phenomenology · Physics 2025-12-30 J Krishnamoorthi , Anil Kumar , Sanjib Kumar Agarwalla

The number of relativistic species, $N_{\rm eff}$, has been precisely calculated in the standard model, and would be measured to the percent level by CMB-S4 in future. Neutral-current non-standard interactions would affect neutrino…

High Energy Physics - Phenomenology · Physics 2021-05-26 Yong Du , Jiang-Hao Yu

Elastic scattering between dark matter particles and a relativistic species such as photons or neutrinos leads to a transfer of energy from the latter due to their intrinsically different temperature scaling relations. In this work, we…

Cosmology and Nongalactic Astrophysics · Physics 2019-01-08 James A. D. Diacoumis , Yvonne Y. Y. Wong

Current neutrino experiments measure the neutrino mixing parameters with an unprecedented accuracy. The upcoming generation of experiments will be sensitive to subdominant effects that can give information on the unknown neutrino…

High Energy Physics - Phenomenology · Physics 2018-01-30 Y. Farzan , M. Tortola

In the presence of neutrino Non-Standard Interactions (NSI) with matter, the derivation of neutrino parameters from oscillation data must be reconsidered. In particular, along with the standard solution to neutrino oscillation, another…

High Energy Physics - Phenomenology · Physics 2018-04-12 Peter B. Denton , Yasaman Farzan , Ian M. Shoemaker

Flavor transitions of Neutrinos with a nonstandard interaction are studied. A scalar field is conformally coupled to matter and neutrinos. This interaction alters the neutrino effective mass and its wavefunction leading to a damping factor,…

High Energy Physics - Phenomenology · Physics 2021-05-25 H. Mohseni Sadjadi , H. Yazdani Ahmadabadi

The Neutrino oscillations have provided an excellent opportunity to study new-physics beyond the Standard Model, popularly known as BSM. The unknown couplings involving neutrinos, termed non-standard interactions (NSI), may appear as…

High Energy Physics - Phenomenology · Physics 2022-07-13 Abinash Medhi , Debajyoti Dutta , Moon Moon Devi

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