Browsing by Author "Agarwalla, S. K."
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- Analytical approximation of the neutrino oscillation matter effects at large theta (13)Agarwalla, S. K.; Kao, Y.; Takeuchi, Tatsu (Springer, 2014-04-07)
- Constraining non-standard interactions of the neutrino with BorexinoAgarwalla, S. K.; Lombardi, Francesco; Takeuchi, Tatsu (Springer, 2012-12-01)We use the Borexino 153.6 ton·year data to place constraints on non-standard neutrino-electron interactions, taking into account the uncertainties in the 7Be solar neutrino flux and the mixing angle θ 23, and backgrounds due to 85Kr and 210Bi β-decay. We find that the bounds are comparable to existing bounds from all other experiments. Further improvement can be expected in Phase II of Borexino due to the reduction in the 85Kr background.
- Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-IIAgarwalla, S. K.; Agostini, Matteo; Altenmueller, Konrad; Appel, S.; Atroshchenko, Victor; Bagdasarian, Zara; Basilico, D.; Bellini, G.; Benziger, Jay; Bick, D.; Bonfini, G.; Bravo, D.; Caccianiga, B.; Calaprice, F.; Caminata, A.; Cappelli, L.; Cavalcante, P.; Cavanna, F.; Chepurnov, A.; Choi, K.; D'Angelo, D.; Davini, S.; Derbin, A. V.; Di Giacinto, A.; Di Marcello, V.; Ding, X. F.; Di Ludovico, Antonio; Di Noto, Lea; Drachnev, I.; Fomenko, K.; Formozov, A.; Franco, D.; Gabriele, Federico; Galbiati, C.; Gschwender, M.; Ghiano, C.; Giammarchi, Marco; Goretti, A.; Gromov, M.; Guffanti, D.; Hagner, C.; Hungerford, Ed V.; Ianni, Aldo; Ianni, Andrea; Jany, A.; Jeschke, D.; Kumaran, S.; Kobychev, V.; Korga, G.; Lachenmaier, Tobias; Laubenstein, Matthias; Litvinovich, E.; Lombardi, Paolo; Ludhova, L.; Lukyanchenko, G.; Lukyanchenko, L.; Machulin, I. N.; Manuzio; Marcocci, S.; Maricic, Jelena; Martyn, J.; Meroni, E.; Meyer, M.; Miramonti, L.; Misiaszek, M.; Muratova, V. N.; Neumair, B.; Nieslony, M.; Oberauer, L.; Orekhov, V.; Ortica, F.; Pallavicini, M.; Papp, L.; Penek, O.; Pietrofaccia, L.; Pilipenko, N.; Pocar, A.; Raikov, G.; Ranucci, G.; Razeto, A.; Re, A.; Redchuk, M.; Romani, A.; Rossi, Nicola; Rottenanger, Sebastian; Schoenert, S.; Semenov, D. A.; Skorokhvatov, Mikhail D.; Smirnov, O. Y.; Sotnikov, A.; Sun, C.; Suvorov, Yura; Takeuchi, Tatsu; Tartaglia, R.; Testera, G.; Thurn, J.; Unzhakov, E. V.; Vishneva, A.; Vogelaar, R. Bruce; von Feilitzsch, F.; Wojcik, M. M.; Wurm, M.; Zaimidoroga, O.; Zavatarelli, S.; Zuber, Kai; Zuzel, G. (2020-02-05)The Borexino detector measures solar neutrino fluxes via neutrino-electron elastic scattering. Observed spectra are determined by the solar-nu(e) survival probability P-ee(E), and the chiral couplings of the neutrino and electron. Some theories of physics beyond the Standard Model postulate the existence of Non-Standard Interactions (NSI's) which modify the chiral couplings and P-ee(E). In this paper, we search for such NSI's, in particular, flavor-diagonal neutral current interactions that modify the nu(e)e and nu(tau)e couplings using Borexino Phase II data. Standard Solar Model predictions of the solar neutrino fluxes for both high- and low-metallicity assumptions are considered. No indication of new physics is found at the level of sensitivity of the detector and constraints on the parameters of the NSI's are placed. In addition, with the same dataset the value of sin(2)theta(W) is obtained with a precision comparable to that achieved in reactor antineutrino experiments .
- Light Sterile Neutrinos: A White PaperAbazajian, Kevork N.; Acero, M. A.; Agarwalla, S. K.; Aguilar-Arevalo, A. A.; Albright, C. H.; Antusch, S.; Arguelles, C. A.; Balantekin, A. B.; Barenboim, G.; Barger, V.; Bernardini, P.; Bezrukov, F.; Bjaelde, O. E.; Bogacz, S. A.; Bowden, N. S.; Boyarsky, A.; Bravar, A.; Berguno, D. B.; Brice, S. J.; Bross, A. D.; Caccianiga, B.; Cavanna, F.; Chun, E. J.; Cleveland, B. T.; Collin, A. P.; Coloma, P.; Conrad, Janet M.; Cribier, M.; Cucoanes, A. S.; D'Olivo, J. C.; Das, S.; Gouvea, A. D.; Derbin, A. V.; Dharmapalan, R.; Diaz, J. S.; Ding, X. J.; Djurcic, Zelimir; Donini, A.; Duchesneau, D.; Ejiri, H.; Elliott, S. R.; Ernst, D. J.; Esmaili, A.; Evans, J. J.; Fernandez-Martinez, Enrique; Figueroa-Feliciano, E.; Fleming, B. T.; Formaggio, J. A.; Franco, D.; Gaffiot, J.; Gandhi, R.; Gao, Y.; Garvey, G. T.; Gavrin, V. N.; Ghoshal, P.; Gibin, D.; Giunti, C.; Gninenko, S. N.; Gorbachev, V. V.; Gorbunov, D. S.; Guenette, R.; Guglielmi, A.; Halzen, F.; Hamann, J.; Hannestad, S.; Haxton, W.; Heeger, K. M.; Henning, R.; Hernandez, P.; Huber, Patrick; Huelsnitz, W.; Ianni, A.; Ibragimova, T. V.; Karadzhov, Y.; Karagiorgi, Georgia S.; Keefer, G.; Kim, Y. D.; Kopp, J.; Kornoukhov, V. N.; Kusenko, A.; Kyberd, P.; Langacker, P.; Lasserre, T.; Laveder, M.; Letourneau, A.; Lhuillier, D.; Li, Y. F.; Lindner, M.; Link, Jonathan M.; Littlejohn, B. L.; Lombardi, Paolo; Long, K.; Lopez-Pavon, J.; Louis, W. C.; Ludhova, L.; Lykken, J. D.; Machado, P. A. N.; Maltoni, M.; Mann, W. A.; Marfatia, D.; Mariani, Camillo; Matveev, V. A.; Mavromatos, N. E.; Melchiorri, A.; Meloni, David; Mena, O.; Mention, G.; Merle, A.; Meroni, E.; Mezzetto, M.; Mills, G. B.; Minic, Djordje; Miramonti, L.; Mohapatra, D.; Mohapatra, R. N.; Montanari, C.; Mori, Y.; Mueller, T. A.; Mumm, H. P.; Muratova, V. N.; Nelson, A. E.; Nico, J. S.; Noah, E.; Nowak, J.; Smirnov, O. Y.; Obolensky, M.; Pakvasa, S.; Palamara, O.; Pallavicini, M.; Pascoli, S.; Patrizii, L.; Pavlovic, Z.; Peres, O. L. G.; Pessard, H.; Pietropaolo, F.; Pitt, M. L.; Popovic, M.; Pradler, J.; Ranucci, G.; Ray, H.; Razzaque, S.; Rebel, B.; Robertson, R. G. H.; Rodejohann, W.; Rountree, S. D.; Rubbia, C.; Ruchayskiy, O.; Sala, P. R.; Scholberg, K.; Schwetz, T.; Shaevitz, Marjorie Hansen; Shaposhnikov, M.; Shrock, R.; Simone, S.; Skorokhvatov, Mikhail D.; Sorel, M.; Sousa, A.; Spergel, D. N.; Spitz, Joshua; Stanco, L.; Stancu, Ion; Suzuki, A.; Takeuchi, Tatsu; Tamborra, Irene; Tang, J.; Testera, G.; Tian, X. C.; Tonazzo, A.; Tunnell, C. D.; Water, R. G. V. D.; Verde, L.; Veretenkin, E. P.; Vignoli, C.; Vivier, M.; Vogelaar, R. Bruce; Wascko, M. O.; Wilkerson, J. F.; Winter, W.; Wong, Y. Y. Y.; Yanagida, T. T.; Yasuda, O.; Yeh, M.; Yermia, F.; Yokley, Z. W.; Zeller, Geralyn P.; Zhan, L.; Zhang, H. (2012-04)This white paper addresses the hypothesis of light sterile neutrinos based on recent anomalies observed in neutrino experiments and the latest astrophysical data.
- Neutrinos from Stored Muons nuSTORM: Expression of InterestAdey, D.; Agarwalla, S. K.; Ankenbrandt, C. M.; Asfandiyarov, R.; Back, J. J.; Barker, G.; Baussan, E.; Bayes, R.; Bhadra, S.; Blackmore, V.; Blondel, A.; Bogacz, S. A.; Booth, C.; Boyd, S. B.; Bravar, A.; Brice, S. J.; Bross, A. D.; Cadoux, F.; Cease, H.; Cervera, A.; Cobb, J.; Colling, D.; Coney, L.; Dobbs, A.; Dobson, J.; Donini, A.; Dornan, P. J.; Dracos, M.; Dufour, F.; Edgecock, R.; Evans, J.; George, M. A.; Ghosh, T.; deGouvea, A.; Gomez-Cadenas, J. J.; Haesler, A.; Hanson, G.; Geelhoed, M.; Harrison, P. F.; Hartz, M.; Hernandez, P.; Hernando-Morata, J. A.; Hodgson, P. J.; Huber, Patrick; Izmaylov, A.; Karadhzov, Y.; Kobilarcik, T.; Kopp, J.; Kormos, L.; Korzenev, A.; Kurup, A.; Kuno, Y.; Kyberd, P.; Lagrange, J. P.; Laing, A. M.; Link, Jonathan M.; Liu, A.; Long, K. R.; McCauley, N.; McDonald, K. T.; Mahn, K.; Martin, C.; Martin, J.; Mena, O.; Mishra, S. R.; Mokhov, N.; Morfin, J.; Mori, Y.; Murray, W.; Neuffer, D.; Nichol, R.; Noah, E.; Palmer, M. A.; Parke, S.; Pascoli, S.; Pasternak, J.; Popovic, M.; Ratoff, P.; Ravonel, M.; Rayner, M.; Ricciardi, S.; Rogers, C.; Rubinov, P.; Santos, E.; Sato, A.; Scantamburlo, E.; Sedgbeer, J. K.; Smith, D. R.; Smith, P. J.; Sobczyk, J. T.; Söldner-Rembold, S.; Soler, F. J. P.; Sorel, M.; Stahl, A.; Stanco, L.; Stamoulis, P.; Striganov, S.; Tanaka, H.; Taylor, I. J.; Touramanis, C.; Tunnell, C. D.; Uchida, Y.; Vassilopoulos, N.; Wascko, M. O.; Weber, A.; Wildner, E.; Wilking, M. J.; Winter, W.; Yang, U. K. (2013-05)The nuSTORM facility has been designed to deliver beams of electron and muon neutrinos from the decay of a stored muon beam with a central momentum of 3.8 GeV/c and a momentum spread of 10%. The facility is unique in that it will: serve the future long- and short-baseline neutrino-oscillation programmes by providing definitive measurements of electron-neutrino- and muon-neutrino-nucleus cross sections with percent-level precision; allow searches for sterile neutrinos of exquisite sensitivity to be carried out; and constitute the essential first step in the incremental development of muon accelerators as a powerful new technique for particle physics. Of the world's proton-accelerator laboratories, only CERN and FNAL have the infrastructure required to mount nuSTORM. Since no siting decision has yet been taken, the purpose of this Expression of Interest (EoI) is to request the resources required to: investigate in detail how nuSTORM could be implemented at CERN; and develop options for decisive European contributions to the nuSTORM facility and experimental programme wherever the facility is sited. The EoI defines a two-year programme culminating in the delivery of a Technical Design Report.
- Running of oscillation parameters in matter with flavor-diagonal non-standard interactions of the neutrinoAgarwalla, S. K.; Kao, Y.; Saha, D.; Takeuchi, Tatsu (Springer, 2015-11-05)