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7161“…We also constrain the sum of neutrino masses, <math display="inline"><mrow><mo>∑</mo><msub><mrow><mi>m</mi></mrow><mrow><mi>ν</mi></mrow></msub><mo>≤</mo><mn>0.14</mn><mtext> </mtext><mtext> </mtext><mi>eV</mi></mrow></math> at 95% C.L., in the presence of relic axions and neutrinos. …”
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7162por Ladron De Guevara, P“…These data will also help to solve problems related to the ``atmospheric neutrino puzzle'' (prediction of the absolute number of upward going muons above 10 GeV to be observed underground).\\ \\Other fundamental issues of cosmic ray and astroparticle physics are being investigated : Burst signals of point sources or gamma ray bursts (GRB) may be detected and the associated muons analyzed. …”
Publicado 2002
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7163por Ammendola, R, Biagioni, A, Frezza, O, Lamanna, G, Lo Cicero, F, Lonardo, A, Martinelli, M, Paolucci, P S, Pastorelli, E, Pontisso, L, Rossetti, D, Simula, F, Sozzi, M, Tosoratto, L, Vicini, P“…We will provide performance results for the three NaNet implementations and describe their usage in the CERN NA62 and KM3NeT-IT underwater neutrino telescope experiments, showing that the architecture is very flexible and yet capable of matching the requirements of low-latency real-time applications with intensive I/O tasks involving the CPU and/or the GPU accelerators.…”
Publicado 2016
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7164por Escalante del Valle, Alberto“…However, it puts strong constrains to its potential cross section and decay to a muon and a neutrino, σW0B(W0 → µν) < 3 fb−1 for W0 masses larger than 2 TeV. …”
Publicado 2018
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7165por Dorrer, Holger, Chrysalidis, Katerina, Goodacre, Thomas Day, Düllmann, Christoph E, Eberhardt, Klaus, Enss, Christian, Gastaldo, Loredana, Haas, Raphael, Harding, Jonathan, Hassel, Clemens, Johnston, Karl, Kieck, Tom, Köster, Ulli, Marsh, Bruce, Mokry, Christoph, Rothe, Sebastian, Runke, Jörg, Schneider, Fabian, Stora, Thierry, Türler, Andreas, Wendt, Klaus“…Several experiments on the study of the electron neutrino mass are based on high-statistics measurements of the energy spectrum following electron capture of the radionuclide $^{163}$Ho. …”
Publicado 2018
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7166por Gataullin, Marat I“…The number of light neutrino species was measured to be 2.98±0.05(stat)±0.04(syst), and the first direct evidence for the pair-production of electron neutrinos was found. …”
Publicado 2006
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7167“…We consider the case of a [Formula: see text] boson with a mass of [Formula: see text] GeV and a gauge coupling [Formula: see text] , which is in reach of Belle-II, and a long-lived [Formula: see text] boson with a mass of [Formula: see text] which can be probed by searching for [Formula: see text] . Neutrino masses and mixing angles can also be accounted for if sterile neutrinos are added to the spectrum.…”
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7168por Broerman, B., Laubenstein, M., Nagorny, S. S., Nisi, S., Song, N., Vincent, A. C.“…The highest sensitivity of the measurement, greater than [Formula: see text] years, was achieved for the two neutrino and neutrinoless double beta decay modes of the isotope [Formula: see text] Pt. …”
Publicado 2023
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7169por Chen, Lin, Yang, Huizhen, Wang, Xingchao, Tian, Liping, Ding, Dongyan, Wang, Yunji, Ji, Ke, Zheng, Pengxiang, Luo, Ting, She, Chenye“…It is widely used in high energy detection experiments such as Jiangmen Underground Neutrino Observatory (JUNO), China JinPing underground Laboratory (CJPL) and Large High Altitude Air Shower Observatory (LHAASO). …”
Publicado 2023
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7170por Martini, Séverine, Al Ali, Badr, Garel, Marc, Nerini, David, Grossi, Vincent, Pacton, Muriel, Casalot, Laurence, Cuny, Philippe, Tamburini, Christian“…Photobacterium phosphoreum ANT-2200 has been isolated from the NW Mediterranean Sea at 2200-m depth (in situ temperature of 13°C) close to the ANTARES neutrino telescope. The effects of hydrostatic pressure on its growth and luminescence have been investigated under controlled laboratory conditions, using a specifically developed high-pressure bioluminescence system. …”
Publicado 2013
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7171por Artusa, D. R., Balzoni, A., Beeman, J. W., Bellini, F., Biassoni, M., Brofferio, C., Camacho, A., Capelli, S., Cardani, L., Carniti, P., Casali, N., Cassina, L., Clemenza, M., Cremonesi, O., Cruciani, A., D’Addabbo, A., Dafinei, I., Di Domizio, S., di Vacri, M. L., Ferroni, F., Gironi, L., Giuliani, A., Gotti, C., Keppel, G., Maino, M., Mancuso, M., Martinez, M., Morganti, S., Nagorny, S., Nastasi, M., Nisi, S., Nones, C., Orio, F., Orlandi, D., Pagnanini, L., Pallavicini, M., Palmieri, V., Pattavina, L., Pavan, M., Pessina, G., Pettinacci, V., Pirro, S., Pozzi, S., Previtali, E., Puiu, A., Rusconi, C., Schäffner, K., Tomei, C., Vignati, M., Zolotarova, A.“…The R&D activity performed during the last years proved the potential of ZnSe scintillating bolometers to the search for neutrino-less double beta decay, motivating the realization of the first large-mass experiment based on this technology: CUPID-0. …”
Publicado 2016
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7172“…The planned installation of a neutrino telescope also offers the potential for biological observatories. …”
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7173Publicado 2020“…High-brightness muon beams comparable to those produced by state-of-the-art electron, proton and ion accelerators could facilitate the study of lepton–antilepton collisions at extremely high energies and provide well characterized neutrino beams(1–6). Such muon beams could be realized using ionization cooling, which has been proposed to increase muon-beam brightness(7,8). …”
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7174por Rosati, P., Basa, S., Blain, A. W., Bozzo, E., Branchesi, M., Christensen, L., Ferrara, A., Gomboc, A., O’Brien, P. T., Osborne, J. P., Rossi, A., Schüssler, F., Spurio, M., Stergioulas, N., Stratta, G., Amati, L., Casewell, S., Ciolfi, R., Ghirlanda, G., Grimm, S., Guetta, D., Harms, J., Le Floc’h, E., Longo, F., Maggiore, M., Mereghetti, S., Oganesyan, G., Salvaterra, R., Tanvir, N. R., Turriziani, S., Vergani, S. D., Balman, S., Caruana, J., Erkut, M. H., Guidorzi, G., Frontera, F., Martin-Carrillo, A., Paltani, S., Porquet, D., Sergijenko, O.“…It will specifically exploit large samples of gamma-ray bursts to probe the early universe back to the first generation of stars, and to advance multi-messenger astrophysics by detecting and localizing the counterparts of gravitational waves and cosmic neutrino sources. The combination and coordination of these activities with multi-wavelength, multi-messenger facilities expected to be operating in the 2030s will open new avenues of exploration in many areas of astrophysics, cosmology and fundamental physics, thus adding considerable strength to the overall scientific impact of THESEUS and these facilities. …”
Publicado 2021
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7175Publicado 1970Tabla de Contenidos: “…The confirmation of continental drift / Hurley -- The lunar orbiter missions to the moon / Levin, Viele, and Eldrenkamp -- Radar observations of the planets / Shapiro -- The atmospheres of Mars and Venus / Eshleman -- The discover of Icarus / Richardson -- Jupiter's Great Red Spot / Hide -- The solar system beyond Neptune / Gingerich -- The solar chromosphere / Athay -- The solar wind / Parker -- Neutrinos from the sun / Bahcall -- Life outside the solar system / Huang -- The Crab Nebula / Oort -- The youngest stars / Herbig -- Dying stars / Greenstein -- Stellar populations / Burbidge and Burbidge -- The arms of the galaxy / Bok -- Interstellar grains / Greenberg -- Hydroxyl radicals in space / Robinson -- Pulsating stars and comic distances / Kraft -- Hydrogen in galaxies / Roberts -- The evolution of galaxies / Arp -- Exploding galaxies / Sandage -- Seyfert galaxies / Weymann -- X-Ray astronomy / Friedman -- The infrared sky / Neugebauer and Leighton -- Ultraviolet astronomy / Goldberg -- Pulsars / Hewish -- The Red-Shift / Sandage -- The evolutionary universe / Gamow -- The problme of the Quasi-stellar objects / Burbidge and Hoyle -- The primeval fireball / Peebles and Wilkinson -- Cosmology before and after quasars / Sciama -- The origin of galaxies / Rees and Silk.…”
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7176por Bogomilov, M., Karadzhov, Y., Kolev, D., Russinov, I., Tsenov, R., Vankova-Kirilova, G., Wang, L., Xu, F.Y., Zheng, S.X., Bertoni, R., Bonesini, M., Ferri, F., Lucchini, G., Mazza, R., Paleari, F., Strati, F., Palladino, V., Cecchet, G., de Bari, A., Capponi, M., Cirillo, A., Iaciofano, A., Manfredini, A., Parisi, M., Orestano, D., Pastore, F., Tonazzo, A., Tortora, L., Mori, Y., Kuno, Y., Sakamoto, H., Sato, A., Yano, T., Yoshida, M., Ishimoto, S., Suzuki, S., Yoshimura, K., Filthaut, F., Garoby, R., Gilardoni, S., Gruber, P., Hanke, K., Haseroth, H., Janot, P., Lombardi, A., Ramberger, S., Vretenar, M., Bene, P., Blondel, A., Cadoux, F., Graulich, J.S., Grichine, V., Gschwendtner, E., Masciocchi, F., Sandstrom, R., Verguilov, V., Wisting, H., Petitjean, C., Seviour, R., Alexander, J., Charnley, G., Collomb, N., Griffiths, S., Martlew, B., Moss, A., Mullacrane, I., Oates, A., Owens, P., White, C., York, S., Adams, D., Apsimon, R., Barclay, P., Baynham, D.E., Bradshaw, T.W., Courthold, M., Drumm, P., Edgecock, R., Hayler, T., Hills, M., Ivaniouchenkov, Y., Jones, A., Lintern, A., MacWaters, C., Nelson, C., Nichols, A., Preece, R., Ricciardi, S., Rochford, J.H., Rogers, C., Spensley, W., Tarrant, J., Tilley, K., Watson, S., Wilson, A., Forrest, D., Soler, F.J.P., Walaron, K., Cooke, P., Gamet, R., Alekou, A., Apollonio, M., Barber, G., Clark, D., Clark, I., Dobbs, A., Dornan, P., Fish, A., Hare, R., Greenwood, S., Jamdagni, A., Kasey, V., Khaleeq, M., Leaver, J., Long, K., McKigney, E., Matsushita, T., Pasternak, J., Sashalmi, T., Savidge, T., Takahashi, M., Blackmore, V., Carlisle, T., Cobb, J.H., Lau, W., Rayner, M., Tunnell, C.D., Witte, H., Yang, S., Booth, C.N., Hodgson, P., Howlett, L., Nicholson, R., Overton, E., Robinson, M., Smith, P., Adey, D., Back, J., Boyd, S., Harrison, P., Ellis, M., Kyberd, P., Littlefield, M., Nebrensky, J.J., Bross, A.D., Geer, S., Neuffer, D., Moretti, A., Popovic, M., Cummings, M.A.C., Roberts, T.J., DeMello, A., Green, M.A., Li, D., Virostek, S., Zisman, M.S., Freemire, B., Hanlet, P., Huang, D., Kafka, G., Kaplan, D.M., Snopok, P., Torun, Y., Blot, S., Kim, Y.K., Bravar, U., Onel, Y., Cline, D., Fukui, Y., Lee, K., Yang, X., Rimmer, R.A., Cremaldi, L.M., Gregoire, G., Hart, T.L., Sanders, D.A., Summers, D.J., Coney, L., Fletcher, R., Hanson, G.G., Heidt, C., Gallardo, J., Kahn, S., Kirk, H., Palmer, R.B.“…Ionization cooling channels are required for the Neutrino Factory and the Muon Collider. MICE will evaluate in detail the performance of a single lattice cell of the Feasibility Study 2 cooling channel. …”
Publicado 2012
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7177por Rybczynski, Maciej, Abgrall, N., Aduszkiewicz, A., Ali, Y., Anticic, T., Antoniou, N., Argyriades, J., Baatar, B., Blondel, A., Blumer, J., Bogomilov, M., Bravar, A., Brooks, W., Brzychczyk, J., Bubak, A., Bunyatov, S.A., Busygina, O., Christakoglou, P., Czopowicz, T., Davis, N., Debieux, S., Dembinski, H., Diakonos, F., Di Luise, S., Dominik, W., Drozhzhova, T., Dumarchez, J., Dynowski, K., Engel, R., Ereditato, A., Esposito, L.S., Feofilov, G.A., Fodor, Z., Ferrero, A., Fulop, A., Gazdzicki, M., Golubeva, M., Grabez, B., Grebieszkow, K., Grzeszczuk, A., Guber, F., Hakobyan, H., Hasegawa, T., Hierholzer, M., Idczak, R., Igolkin, S., Ivanov, Y., Ivashkin, A., Jakovic, D., Kadija, K., Kapoyannis, A., Katrynska, N., Kaptur, E., Kielczewska, D., Kikola, D., Kirejczyk, M., Kisiel, J., Kiss, T., Kleinfelder, S., Kobayashi, T., Kolesnikov, V.I., Kolev, D., Kondratiev, V.P., Korzenev, A., Kowalski, S., Krasnoperov, A., Kuleshov, S., Kurepin, A., Larsen, D., Laszlo, A., Lyubushkin, V.V., Mackowiak-Pawlowska, M., Majka, Z., Maksiak, B., Malakhov, A.I., Maletic, D., Marchionni, A., Marcinek, A., Marin, V., Marton, K., Mathes, H.J., Matulewicz, T., Matveev, V., Melkumov, G.L., Mrowczynski, St., Murphy, S., Nakadaira, T., Nirkko, M., Nishikawa, K., Palczewski, T., Palla, G., Panagiotou, A.D., Paul, T., Pistillo, C., Redij, A., Peryt, W., Petukhov, O., Planeta, R., Pluta, J., Popov, B.A., Posiadala, M., Pulawski, S., Puzovic, J., Rauch, W., Ravonel, M., Renfordt, R., Robert, A., Röhrich, D., Rondio, E., Roth, M., Rubbia, A., Rustamov, A., Rybczynski, M., Sadovsky, A., Sakashita, K., Savic, M., Sekiguchi, T., Seyboth, P., Shibata, M., Sipos, M., Skrzypczak, E., Slodkowski, M., Staszel, P., Stefanek, G., Stepaniak, J., Stroebele, H., Susa, T., Szuba, M., Tada, M., Tereshchenko, V., Tolyhi, T., Tsenov, R., Turko, L., Ulrich, R., Unger, M., Vassiliou, M., Veberic, D., Vechernin, V.V., Vesztergombi, G., Vinogradov, L., Wilczek, A., Wlodarczyk, Z., Wojtaszek, A., Wyszynski, O., Zambelli, L., Zipper, W.“…NA61/SHINE at the CERN SPS is a fixed-target experiment pursuing a rich physics program including measurements for heavy ion, neutrino and cosmic ray physics. The main goal of the ion program is to explore the most interesting $T, mu_{B}$ region of the phase diagram of strongly interacting matter. …”
Publicado 2013
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7178por Curtin, David, Drewes, Marco, McCullough, Matthew, Meade, Patrick, Mohapatra, Rabindra N., Shelton, Jessie, Shuve, Brian, Accomando, Elena, Alpigiani, Cristiano, Antusch, Stefan, Arteaga-Velázquez, Juan Carlos, Batell, Brian, Bauer, Martin, Blinov, Nikita, Caballero-Mora, Karen Salomé, Chang, Jae Hyeok, Chun, Eung Jin, Co, Raymond T., Cohen, Timothy, Cox, Peter, Craig, Nathaniel, Csáki, Csaba, Cui, Yanou, D'Eramo, Francesco, Delle Rose, Luigi, Bhupal Dev, P.S., Dienes, Keith R., Dror, Jeff A., Essig, Rouven, Evans, Jared A., Evans, Jason L., Tellez, Arturo Fernández, Fischer, Oliver, Flacke, Thomas, Fradette, Anthony, Frugiuele, Claudia, Fuchs, Elina, Gherghetta, Tony, Giudice, Gian F., Gorbunov, Dmitry, Gupta, Rick S., Hagedorn, Claudia, Hall, Lawrence J., Harris, Philip, Helo, Juan Carlos, Hirsch, Martin, Hochberg, Yonit, Hook, Anson, Ibarra, Alejandro, Ipek, Seyda, Jung, Sunghoon, Knapen, Simon, Kuflik, Eric, Liu, Zhen, Lombardo, Salvator, Lubatti, H.J., McKeen, David, Molinaro, Emiliano, Moretti, Stefano, Nagata, Natsumi, Neubert, Matthias, No, Jose Miguel, Olaiya, Emmanuel, Perez, Gilad, Peskin, Michael E., Pinner, David, Pospelov, Maxim, Reece, Matthew, Robinson, Dean J., Cahuantzi, Mario Rodríguez, Santonico, Rinaldo, Schlaffer, Matthias, Shepherd-Themistocleous, Claire H., Spray, Andrew, Stolarski, Daniel, Subieta Vasquez, Martin A., Sundrum, Raman, Thamm, Andrea, Thomas, Brooks, Tsai, Yuhsin, Tweedie, Brock, West, Stephen M., Young, Charles, Yu, Felix, Zaldivar, Bryan, Zhang, Yongchao, Zurek, Kathryn, Zurita, José“…LLPs are a common prediction of a wide range of theories that address unsolved fundamental mysteries such as naturalness, dark matter, baryogenesis and neutrino masses, and represent a natural and generic possibility for physics beyond the SM (BSM). …”
Publicado 2018
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7179por Feng, Jonathan L., Kling, Felix, Reno, Mary Hall, Rojo, Juan, Soldin, Dennis, Anchordoqui, Luis A., Boyd, Jamie, Ismail, Ahmed, Harland-Lang, Lucian, Kelly, Kevin J., Pandey, Vishvas, Trojanowski, Sebastian, Tsai, Yu-Dai, Alameddine, Jean-Marco, Araki, Takeshi, Ariga, Akitaka, Ariga, Tomoko, Asai, Kento, Bacchetta, Alessandro, Balazs, Kincso, Barr, Alan J., Battistin, Michele, Bian, Jianming, Bertone, Caterina, Bai, Weidong, Bakhti, Pouya, Balantekin, A. Baha, Barman, Basabendu, Batell, Brian, Bauer, Martin, Bauer, Brian, Becker, Mathias, Berlin, Asher, Bertuzzo, Enrico, Bhattacharya, Atri, Bonvini, Marco, Boogert, Stewart T., Boyarsky, Alexey, Bramante, Joseph, Brdar, Vedran, Carmona, Adrian, Casper, David W., Celiberto, Francesco Giovanni, Cerutti, Francesco, Chachamis, Grigorios, Chauhan, Garv, Citron, Matthew, Copello, Emanuele, Corso, Jean-Pierre, Darmé, Luc, D'Agnolo, Raffaele Tito, Darvishi, Neda, Das, Arindam, De Lellis, Giovanni, De Roeck, Albert, de Vries, Jordy, Dembinski, Hans P., Demidov, Sergey, deNiverville, Patrick, Denton, Peter B., Deppisch, Frank F., Dev, P.S. Bhupal, Di Crescenzo, Antonia, Dienes, Keith R., Diwan, Milind V., Dreiner, Herbi K., Du, Yong, Dutta, Bhaskar, Duwentäster, Pit, Elie, Lucie, Ellis, Sebastian A.R., Enberg, Rikard, Farzan, Yasaman, Fieg, Max, Foguel, Ana Luisa, Foldenauer, Patrick, Foroughi-Abari, Saeid, Fortin, Jean-François, Friedland, Alexander, Fuchs, Elina, Fucilla, Michael, Gallmeister, Kai, Garcia, Alfonso, García Canal, Carlos A., Garzelli, Maria Vittoria, Gauld, Rhorry, Ghosh, Sumit, Ghoshal, Anish, Gibson, Stephen, Giuli, Francesco, Gonçalves, Victor P., Gorbunov, Dmitry, Goswami, Srubabati, Grau, Silvia, Günther, Julian Y., Guzzi, Marco, Haas, Andrew, Hakulinen, Timo, Harris, Steven P., Harz, Julia, Herrera, Juan Carlos Helo, Hill, Christopher S., Hirsch, Martin, Hobbs, Timothy J., Höche, Stefan, Hryczuk, Andrzej, Huang, Fei, Inada, Tomohiro, Infantino, Angelo, Ismail, Ameen, Jacobsson, Richard, Jana, Sudip, Jeong, Yu Seon, Ježo, Tomas, Jho, Yongsoo, Jodłowski, Krzysztof, lowski, Krzysztof Jod, Kalashnikov, Dmitry, Kärkkäinen, Timo J., Keppel, Cynthia, Kim, Jongkuk, Klasen, Michael, Klein, Spencer R., Ko, Pyungwon, Köhler, Dominik, Komatsu, Masahiro, Kovaˇrík, Karol, Kulkarni, Suchita, Kumar, Jason, Kumar, Karan, Kuo, Jui-Lin, Krauss, Frank, Kusina, Aleksander, Laletin, Maxim, Le Roux, Chiara, Lee, Seung J., Lee, Hye-Sung, Lefebvre, Helena, Li, Jinmian, Li, Shuailong, Li, Yichen, Liu, Wei, Liu, Zhen, Lonjon, Mickael, Lyu, Kun-Feng, Maciula, Rafal, Mammen Abraham, Roshan, Masouminia, Mohammad R., McFayden, Josh, Mikulenko, Oleksii, Mohammed, Mohammed M.A., Mohan, Kirtimaan A., Morfín, Jorge G., Mosel, Ulrich, Mosny, Martin, Muzakka, Khoirul F., Nadolsky, Pavel, Nakano, Toshiyuki, Nangia, Saurabh, Cornago, Angel Navascues, Nevay, Laurence J., Ninin, Pierre, Nocera, Emanuele R., Nomura, Takaaki, Nunes, Rui, Okada, Nobuchika, Olness, Fred, Osborne, John, Otono, Hidetoshi, Ovchynnikov, Maksym, Papa, Alessandro, Pei, Junle, Peon, Guillermo, Perez, Gilad, Pickering, Luke, Plätzer, Simon, Plestid, Ryan, Poddar, Tanmay Kumar, Quílez, Pablo, Rai, Mudit, Rajaee, Meshkat, Raut, Digesh, Reimitz, Peter, Resnati, Filippo, Rhode, Wolfgang, Richardson, Peter, Ritz, Adam, Rokujo, Hiroki, Roszkowski, Leszek, Ruhe, Tim, Ruiz, Richard, Sabate-Gilarte, Marta, Sandrock, Alexander, Sarcevic, Ina, Sarkar, Subir, Sato, Osamu, Scherb, Christiane, Schienbein, Ingo, Schulz, Holger, Schwaller, Pedro, Sciutto, Sergio J., Sengupta, Dipan, Shchutska, Lesya, Shimomura, Takashi, Silvetti, Federico, Sinha, Kuver, Sjöstrand, Torbjörn, Sobczyk, Jan T., Song, Huayang, Soriano, Jorge F., Soreq, Yotam, Stasto, Anna, Stuart, David, Su, Shufang, Su, Wei, Szczurek, Antoni, Tabrizi, Zahra, Takubo, Yosuke, Taoso, Marco, Thomas, Brooks, Thonet, Pierre, Tuckler, Douglas, Sabio Vera, Agustin, Vincke, Heinz, Vishnudath, K.N., Wang, Zeren Simon, Winkler, Martin W., Wu, Wenjie, Xie, Keping, Xu, Xun-Jie, You, Tevong, Yu, Ji-Young, Yu, Jiang-Hao, Zapp, Korinna, Zhang, Yongchao, Zhang, Yue, Zhou, Guanghui, Funchal, Renata Zukanovich“…FPF experiments will be sensitive to a broad range of BSM physics through searches for new particle scattering or decay signatures and deviations from SM expectations in high statistics analyses with TeV neutrinos in this low-background environment. High statistics neutrino detection will also provide valuable data for fundamental topics in perturbative and non-perturbative QCD and in weak interactions. …”
Publicado 2022
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7180por Ade, P.A.R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A.J., Barreiro, R.B., Bartlett, J.G., Bartolo, N., Battaner, E., Battye, R., Benabed, K., Benoit, A., Benoit-Levy, A., Bernard, J.P., Bersanelli, M., Bielewicz, P., Bonaldi, A., Bonavera, L., Bond, J.R., Borrill, J., Bouchet, F.R., Boulanger, F., Bucher, M., Burigana, C., Butler, R.C., Calabrese, E., Cardoso, J.F., Catalano, A., Challinor, A., Chamballu, A., Chary, R.R., Chiang, H.C., Chluba, J., Christensen, P.R., Church, S., Clements, D.L., Colombi, S., Colombo, L.P.L., Combet, C., Coulais, A., Crill, B.P., Curto, A., Cuttaia, F., Danese, L., Davies, R.D., Davis, R.J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Desert, F.X., Di Valentino, E., Dickinson, C., Diego, J.M., Dolag, K., Dole, H., Donzelli, S., Dore, O., Douspis, M., Ducout, A., Dunkley, J., Dupac, X., Efstathiou, G., Elsner, F., Ensslin, T.A., Eriksen, H.K., Farhang, M., Fergusson, J., Finelli, F., Forni, O., Frailis, M., Fraisse, A.A., Franceschi, E., Frejsel, A., Galeotta, S., Galli, S., Ganga, K., Gauthier, C., Gerbino, M., Ghosh, T., Giard, M., Giraud-Heraud, Y., Giusarma, E., Gjerlow, E., Gonzalez-Nuevo, J., Gorski, K.M., Gratton, S., Gregorio, A., Gruppuso, A., Gudmundsson, J.E., Hamann, J., Hansen, F.K., Hanson, D., Harrison, D.L., Helou, G., Henrot-Versille, S., Hernandez-Monteagudo, C., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Huang, Z., Huffenberger, K.M., Hurier, G., Jaffe, A.H., Jaffe, T.R., Jones, W.C., Juvela, M., Keihanen, E., Keskitalo, R., Kisner, T.S., Kneissl, R., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lahteenmaki, A., Lamarre, J.M., Lasenby, A., Lattanzi, M., Lawrence, C.R., Leahy, J.P., Leonardi, R., Lesgourgues, J., Levrier, F., Lewis, A., Liguori, M., Lilje, P.B., Linden-Vornle, M., Lopez-Caniego, M., Lubin, P.M., Macias-Perez, J.F., Maggio, G., Mandolesi, N., Mangilli, A., Marchini, A., Martin, P.G., Martinelli, M., Martinez-Gonzalez, E., Masi, S., Matarrese, S., Mazzotta, P., McGehee, P., Meinhold, P.R., Melchiorri, A., Melin, J.B., Mendes, L., Mennella, A., Migliaccio, M., Millea, M., Mitra, S., Miville-Deschenes, M.A., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Murphy, J.A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C.B., Norgaard-Nielsen, H.U., Noviello, F., Novikov, D., Novikov, I., Oxborrow, C.A., Paci, F., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, T.J., Perdereau, O., Perotto, L., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Popa, L., Pratt, G.W., Prezeau, G., Prunet, S., Puget, J.L., Rachen, J.P., Reach, W.T., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., d'Orfeuil, B.Rouille, Rowan-Robinson, M., Rubino-Martin, J.A., Rusholme, B., Said, N., Salvatelli, V., Salvati, L., Sandri, M., Santos, D., Savelainen, M., Savini, G., Scott, D., Seiffert, M.D., Serra, P., Shellard, E.P.S., Spencer, L.D., Spinelli, M., Stolyarov, V., Stompor, R., Sudiwala, R., Sunyaev, R., Sutton, D., Suur-Uski, A.S., Sygnet, J.F., Tauber, J.A., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Trombetti, T., Tucci, M., Tuovinen, J., Turler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L.A., Wandelt, B.D., Wehus, I.K., White, M., White, S.D.M., Wilkinson, A., Yvon, D., Zacchei, A., Zonca, A.“…Combining Planck with other astrophysical data we find N_ eff = 3.15 +/- 0.23 for the effective number of relativistic degrees of freedom and the sum of neutrino masses is constrained to < 0.23 eV. Spatial curvature is found to be |Omega_K| < 0.005. …”
Publicado 2015
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