Mostrando 7,161 - 7,180 Resultados de 8,091 Para Buscar '"Neutrino"', tiempo de consulta: 0.21s Limitar resultados
  1. 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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  2. 7162
    por Ladron De Guevara, P
    Publicado 2002
    “…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. …”
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  3. 7163
    “…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.…”
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  4. 7164
    por Escalante del Valle, Alberto
    Publicado 2018
    “…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. …”
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  5. 7165
  6. 7166
    por Gataullin, Marat I
    Publicado 2006
    “…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. …”
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  7. 7167
    por Ardu, Marco, Kirk, Fiona
    Publicado 2023
    “…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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  8. 7168
    “…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. …”
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  9. 7169
    “…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). …”
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  10. 7170
    “…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. …”
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  11. 7171
  12. 7172
    “…The planned installation of a neutrino telescope also offers the potential for biological observatories. …”
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  13. 7173
    Publicado 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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  14. 7174
    “…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. …”
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  15. 7175
    Publicado 1970
    Tabla 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.…”
    Libro
  16. 7176
    por 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.
    Publicado 2012
    “…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. …”
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  17. 7177
    por 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.
    Publicado 2013
    “…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. …”
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  18. 7178
    por 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
    Publicado 2018
    “…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). …”
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  19. 7179
    por 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
    Publicado 2022
    “…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. …”
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  20. 7180
    por 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.
    Publicado 2015
    “…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. …”
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