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Related papers: Atmospheric Sterile Neutrinos

200 papers

We consider the upscattering of atmospheric neutrinos in the interior of the Earth producing heavy neutral leptons (HNLs) which subsequently decay inside large volume detectors (e.g. Super-Kamiokande or DUNE). We compute the flux of…

High Energy Physics - Phenomenology · Physics 2024-09-04 R. Andrew Gustafson , Ryan Plestid , Ian M. Shoemaker

A high-density calorimeter, consisting of magnetized iron planes interleaved by RPCs, as tracking and timing devices, is a good candidate for a next generation experiment on atmospheric neutrinos. With 34 kt of mass and in four years of…

Sterile neutrinos with mass in the eV-scale and large mixings of order $\theta_0\simeq 0.1$ could explain some anomalies found in short-baseline neutrino oscillation data. Here, we revisit a neutrino portal scenario in which eV-scale…

High Energy Physics - Phenomenology · Physics 2018-06-27 Yu Seon Jeong , Sergio Palomares-Ruiz , Mary Hall Reno , Ina Sarcevic

It is commonly assumed that the cosmological and astrophysical bounds on the mixings of sterile with active neutrinos are much more stringent than those obtained from laboratory measurements. We point out that in scenarios with a very low…

Astrophysics · Physics 2009-06-23 Graciela Gelmini , Efunwande Osoba , Sergio Palomares-Ruiz , Silvia Pascoli

A supernova event in our own galaxy will result in a large number of neutrinos detected on Earth within the time-frame of a few seconds. These neutrinos will have been produced thermally with, in principle, three distinct temperatures for…

High Energy Physics - Phenomenology · Physics 2016-05-04 Jonathan H. Davis

Sterile neutrinos can be produced in the early universe via interactions with their active counterparts. For small active-sterile mixing angles, thermal equilibrium with the standard model plasma is not reached and sterile neutrinos are…

High Energy Physics - Phenomenology · Physics 2022-07-06 Gonzalo Alonso-Álvarez , James M. Cline

Solar neutrino experiments are highly sensitive to sources of $\nu\to\overline{\nu}$ conversions in the $^8$B neutrino flux. In this work we adapt these searches to non-minimal sterile neutrino models recently proposed to explain the LSND,…

High Energy Physics - Phenomenology · Physics 2021-09-29 Matheus Hostert , Maxim Pospelov

Sterile neutrinos are among the most attractive extensions of the SM to generate the light neutrino masses observed in neutrino oscillation experiments. When the sterile neutrinos are subject to a protective symmetry, they can have masses…

High Energy Physics - Phenomenology · Physics 2017-06-07 Stefan Antusch , Eros Cazzato , Oliver Fischer

If massive sterile neutrinos exist, their decays into photons and/or electron-positron pairs may give rise to observable consequences. We consider the possibility that MeV sterile neutrino decays lead to the diffuse positron annihilation…

High Energy Astrophysical Phenomena · Physics 2015-06-03 M. H. Chan , M. -C. Chu

Low-scale models of neutrino mass generation often feature sterile neutrinos with masses in the GeV-TeV range, which can be produced at colliders through their mixing with the Standard Model neutrinos. We consider an alternative scenario in…

High Energy Physics - Phenomenology · Physics 2021-02-24 Stéphane Lavignac , Anibal D. Medina

A measurement of the flux of neutrino-induced muons using the MACRO detector is presented. Different event topologies, corresponding to different neutrino parent energies can be detected. The upward throughgoing muon sample is the larger…

High Energy Physics - Experiment · Physics 2008-11-26 F. Ronga

Seesaw mechanism constrains from below mixing between active and sterile neutrinos for fixed sterile neutrino masses. Signal events associated with sterile neutrino decays inside a detector at fixed target experiment are suppressed by the…

High Energy Physics - Phenomenology · Physics 2018-10-09 Igor Krasnov , Timofey Grigorin-Ryabov

Young, rapidly rotating neutron stars could accelerate protons to energies of $\sim 1$ PeV close to the stellar surface, which scatter with x-rays from the stellar surface through the $\Delta$ resonance and produce pions. The pions…

Astrophysics · Physics 2008-11-26 G. F. Burgio , B. Link

The signal produced in neutrino observatories by the pair-annihilation neutrinos emitted from a 20 $M_{\odot}$ pre-supernova star at the silicon burning phase is estimated. The spectrum of the neutrinos with an average energy $\sim$2 MeV is…

Astrophysics · Physics 2007-05-23 A. Odrzywolek , M. Misiaszek , M. Kutschera

In the standard model extended with a seesaw mass matrix, we study the production of sterile neutrinos from the decay of vector bosons at $T\simeq M_{W,Z}$. We derive a general quantum kinetic equation for the production of sterile…

High Energy Physics - Phenomenology · Physics 2017-03-01 Louis Lello , Daniel Boyanovsky , Robert D. Pisarski

A global analysis of all the available atmospheric neutrino data is presented in terms of neutrino oscillations in the nu_mu -> nu_tau and nu_mu -> nu_s channels, where nu_s denotes a sterile neutrino. We perform our analysis of the…

High Energy Physics - Phenomenology · Physics 2009-09-17 N. Fornengo , M. C. Gonzalez-Garcia , J. W. F. Valle

We show that study of the atmospheric neutrinos in the 10--100 GeV energy range by DeepCore sub-array of the IceCube Neutrino Observatory can substantially constrain the mixing of sterile neutrinos of mass $\sim 1$ eV with active neutrinos.…

High Energy Physics - Phenomenology · Physics 2012-05-22 Soebur Razzaque , A. Yu. Smirnov

Recent results show that atmospheric $\nu_\mu$ oscillate with $\delta m^2 \simeq 3 \times 10^{-3}$ eV$^2$ and $\sin^2{2\theta_{atm}} \simeq 1$, and that conversion into $\nu_e$ is strongly disfavored. The Super-Kamiokande (SK)…

High Energy Physics - Phenomenology · Physics 2009-11-10 John F. Beacom , Sergio Palomares-Ruiz

Searches for a light sterile neutrino have been performed independently by the MINOS and the Daya Bay experiments using the muon (anti)neutrino and electron antineutrino disappearance channels, respectively. In this Letter, results from…

High Energy Physics - Experiment · Physics 2016-10-18 Daya Bay , MINOS Collaborations , : , P. Adamson , F. P. An , I. Anghel , A. Aurisano , A. B. Balantekin , H. R. Band , G. Barr , M. Bishai , A. Blake , S. Blyth G. J. Bock , D. Bogert , D. Cao , G. F. Cao , J. Cao , S. V. Cao , T. J. Carroll , C. M. Castromonte , W. R. Cen , Y. L. Chan , J. F. Chang , L. C. Chang , Y. Chang , H. S. Chen , Q. Y. Chen , R. Chen , S. M. Chen , Y. Chen , Y. X. Chen , J. Cheng , J. -H. Cheng , Y. P. Chen , Z. K. Cheng , J. J. Cherwinka , S. Childress , M. C. Chu , A. Chukanov , J. A. B. Coelho , L. Corwin , D. Cronin-Hennessy , J. P. Cummings , J. de Arcos , S. De Rijck , Z. Y. Deng , A. V. Devan , N. E. Devenish , X. F. Ding , Y. Y. Ding , M. V. Diwan , M. Dolgareva , J. Dove , D. A. Dwyer , W. R. Edwards , C. O. Escobar , J. J. Evans , E. Falk , G. J. Feldman , W. Flanagan , M. V. Frohne , M. Gabrielyan , H. R. Gallagher , S. Germani , R. Gill , R. A. Gomes , M. Gonchar , G. H. Gong , H. Gong , M. C. Goodman , P. Gouffon , N. Graf , R. Gran , M. Grassi , K. Grzelak , W. Q. Gu , M. Y. Guan , L. Guo , R. P. Guo , X. H. Guo , Z. Guo , A. Habig , R. W. Hackenburg , S. R. Hahn , R. Han , S. Hans , J. Hartnell , R. Hatcher , M. He , K. M. Heeger , Y. K. Heng , A. Higuera , A. Holin , Y. K. Hor , Y. B. Hsiung , B. Z. Hu , T. Hu , W. Hu , E. C. Huang , H. X. Huang , J. Huang , X. T. Huang , P. Huber , W. Huo , G. Hussain , J. Hylen , G. M. Irwin , Z. Isvan , D. E. Jaffe , P. Jaffke , C. James , K. L. Jen , D. Jensen , S. Jetter , X. L. Ji , X. P. Ji , J. B. Jiao , R. A. Johnson , J. K. de Jong , J. Joshi , T. Kafka , L. Kang , S. M. S. Kasahara , S. H. Kettell , S. Kohn , G. Koizumi , M. Kordosky , M. Kramer , A. Kreymer , 1 K. K. Kwan , M. W. Kwok , T. Kwok , K. Lang , T. J. Langford , K. Lau , L. Lebanowski , J. Lee , J. H. C. Lee , R. T. Lei , R. Leitner , J. K. C. Leung , C. Li , D. J. Li , F. Li , G. S. Li , Q. J. Li , S. Li , S. C. Li , W. D. Li , X. N. Li , Y. F. Li , Z. B. Li , H. Liang , C. J. Lin , G. L. Lin , S. Lin , S. K. Lin , Y. -C. Lin , J. J. Ling J. M. Link , P. J. Litchfield , L. Littenberg , B. R. Littlejohn , D. W. Liu , J. C. Liu , J. L. Liu , C. W. Loh , C. Lu , H. Q. Lu , J. S. Lu , P. Lucas , K. B. Luk , Z. Lv , Q. M. Ma , X. B. Ma , X. Y. Ma , Y. Q. Ma , Y. Malyshkin , W. A. Mann , M. L. Marshak , D. A. Martinez Caicedo , N. Mayer , K. T. McDonald , C. McGivern , R. D. McKeown , M. M. Medeiros , R. Mehdiyev , J. R. Meier , M. D. Messier , W. H. Miller , S. R. Mishra , I. Mitchell , M. Mooney , C. D. Moore , L. Mualem , J. Musser , Y. Nakajima , D. Naples , J. Napolitano , D. Naumov , E. Naumova , J. K. Nelson , H. B. Newman , H. Y. Ngai , R. J. Nichol , Z. Ning , A. Nowak , J. O'Connor , J. P. Ochoa-Ricoux , A. Olshevskiy , M. Orchanian , R. , R. B. Pahlka , J. Paley , H. -R. Pan , J. Park , R. B. Patterson , S. Patton , G. Pawloski , V. Pec , J. C. Peng , A. Perch , M. M. Pfutzner , D. D. Phan , S. Phan-Budd , L. Pinsky , R. K. Plunkett , N. Poonthottathil , C. S. J. Pun , F. Z. Qi , M. Qi , X. Qian , X. Qiu , A. Radovic , N. Raper , B. Rebel , J. Ren , C. Rosenfeld , R. Rosero , B. Roskovec , X. C. Ruan , H. A. Rubin , P. Sail , M. C. Sanchez , J. Schneps , A. Schreckenberger , P. Schreiner , R. Sharma , S. Moed Sher , A. Sousa , H. Steiner , G. X. Sun , J. L. Sun , N. Tagg , R. L. Talaga , W. Tang , D. Taychenachev , J. Thomas , M. A. Thomson , X. Tian A. Timmons , J. Todd , S. C. Tognini , R. Toner , D. Torretta , K. Treskov , K. V. Tsang , C. E. Tull , G. Tzanakos , J. Urheim , P. Vahle , N. Viaux , B. Viren , V. Vorobel , C. H. Wang , M. Wang , N. Y. Wang , R. G. Wang , W. Wang , X. Wang , Y. F. Wang , Z. Wang , Z. M. Wang , R. C. Webb , A. Weber , H. Y. Wei , L. J. Wen , K. Whisnant , C. White , L. Whitehead L. H. Whitehead , T. Wise , S. G. Wojcicki , H. L. H. Wong , S. C. F. Wong , E. Worcester , C. -H. Wu , Q. Wu , W. J. Wu , D. M. Xia , J. K. Xia , Z. Z. Xing , J. L. Xu , J. Y. Xu , Y. Xu , T. Xue , C. G. Yang , H. Yang , L. Yang , M. S. Yang , M. T. Yang , M. Ye. , Z. Ye , M. Yeh , B. L. Young , Z. Y. Yu , S. Zeng , L. ZhanC. Zhang , H. H. Zhang , J. W. Zhang , Q. M. Zhang , X. T. Zhang , Y. M. Zhang , Y. X. Zhang , Z. J. Zhang , Z. P. Zhang , Z. Y. Zhang , J. Zhao , Q. W. Zhao , Y. B. Zhao , W. L. Zhong , L. Zhou , N. Zhou , H. L. Zhuang , J. H. Zou

The down-going atmospheric \nu_{\mu} and {\bar{\nu_{\mu}}} fluxes can be significantly altered due to the presence of eV^2-scale active-sterile oscillations. We study the sensitivity of a large Liquid Argon detector and a large magnetized…

High Energy Physics - Phenomenology · Physics 2013-05-30 Raj Gandhi , Pomita Ghoshal