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    Wyświetlanie 1-4 z 4
    Tytuł:
    Measurement of the electron structure function $F_{2}^{e}$ at LEP energies
    Autorzy:
    Fuster, J.
    Zalewska, A.
    Veloso, F.
    Benvenuti, A.
    Cavallo, F.
    Pukhaeva, N.
    Todorovova, S.
    Petrolini, A.
    Benekos, N.
    Mazzucato, F.
    Moenig, K.
    Treille, D.
    Begalli, M.
    Rovelli, T.
    Meroni, C.
    Sokolov, A.
    Abdallah, J.
    Wicke, D.
    Siebel, M.
    Van Vulpen, I.
    Spassov, T.
    Zavrtanik, D.
    Ferrer, A.
    Szumlak, T.
    Wickens, J.
    Sander, C.
    Jarry, P.
    Muryn, B.
    Borisov, G.
    Crennell, D.
    De Maria, N.
    Tonazzo, A.
    Barker, G. J.
    Garcia, C.
    Berat, C.
    Mandl, F.
    Amato, S.
    Nikolenko, M.
    Ferro, F.
    Ruhlmann-Kleider, V.
    Asman, B.
    Lesiak, T.
    Adzic, P.
    Liebig, W.
    Tobin, M.
    Matorras, F.
    Mazzucato, M.
    Lyons, L.
    Fernandez, J.
    van Remortel, N.
    Andreazza, A.
    Tzamarias, S.
    Katsoufis, E.
    Ballestrero, A.
    Flagmeyer, U.
    Stugu, B.
    Zupan, M.
    Di Ciaccio, L.
    Rivero, M.
    Behrmann, A.
    De Boer, W.
    Contri, R.
    Mulders, M.
    Myklebust, T.
    Bertrand, D.
    Blom, M.
    Augustin, J. E.
    Jonsson, P.
    Brenner, R.
    Myatt, G.
    Romero, A.
    Ouraou, A.
    Tortosa, P.
    Della Ricca, G.
    Oyanguren, A.
    Kapusta, F.
    da Silva, T.
    Parkes, C.
    Ellert, M.
    Ryabtchikov, D.
    Abreu, P.
    Piotto, E.
    Orava, R.
    Vitale, L.
    Zimin, N. I.
    Drees, J.
    Vrba, V.
    Winter, M.
    Lutz, P.
    Kouznetsov, O.
    Jackson, J. N.
    Sosnowski, R.
    Szczekowski, M.
    Moa, T.
    Arnoud, Y.
    Mueller, U.
    Smadja, G.
    Krumstein, Z.
    Bonesini, M.
    Augustinus, A.
    Camporesi, T.
    Ben-Haim, E.
    Johansson, E. K.
    Jungermann, L.
    Grosdidier, G.
    Muenich, K.
    Besancon, M.
    Mariotti, C.
    Ask, S.
    Pimenta, M.
    Salmi, L.
    Anjos, N.
    Boyko, I.
    Renton, P.
    Belous, K.
    Chudoba, J.
    Palacios, J. P.
    Castro, N.
    Allport, P. P.
    Trochimczuk, M.
    Moreno, S.
    Sisakian, A.
    Eigen, G.
    Liko, D.
    Bowcock, T. J. W.
    Cuevas, J.
    Haug, S.
    Rodriguez, D.
    Apel, W-D.
    MacNaughton, J.
    Ledroit, F.
    Moraes, D.
    Baroncelli, A.
    De Clercq, C.
    Buschmann, P.
    Martinez-Rivero, C.
    Tome, B.
    Bambade, P.
    Di Simone, A.
    Polok, G.
    Leinonen, L.
    Carena, F.
    Bouquet, B.
    Booth, P. S. L.
    Leder, G.
    Elsing, M.
    Holmgren, S-O.
    Podobnik, T.
    Yushchenko, O.
    Stanitzki, M.
    Kerzel, U.
    Antilogus, P.
    Uvarov, V.
    Gavillet, Ph.
    Cossutti, F.
    Vilanova, D.
    Lepeltier, V.
    Poireau, V.
    Pozdniakov, V.
    Olshevski, A.
    Botner, O.
    Gomez-Ceballos, G.
    Reid, D.
    Mundim, L.
    Albrecht, T.
    Van Eldik, J.
    Battaglia, M.
    Haag, C.
    de Paula, L.
    Smirnova, O.
    Margoni, M.
    Papadopoulou, Th. D.
    Chierici, R.
    Marin, J-C.
    Migliore, E.
    Brunet, J. M.
    Tkatchev, L.
    Cieslik, K.
    Mastroyiannopoulos, N.
    Fokitis, E.
    Maltezos, S.
    Costa, M. J.
    Katsanevas, S.
    Pierre, F.
    Bluj, M.
    Malek, A.
    Berggren, M.
    Barbier, R.
    D'Hondt, J.
    Nawrocki, K.
    Brodet, E.
    Hedberg, V.
    King, B. T.
    Zintchenko, A.
    Passon, O.
    Buschbeck, B.
    Nicolaidou, R.
    Hauler, F.
    Turluer, M-L.
    Verzi, V.
    Marechal, B.
    Sopczak, A.
    Richard, F.
    Hallgren, A.
    Fanourakis, G.
    Pape, L.
    Hennecke, M.
    Radojicic, D.
    Guy, J.
    Parodi, F.
    Washbrook, A. J.
    Onofre, A.
    Salt, J.
    Adam, W.
    Paganoni, M.
    Baillon, P.
    Loukas, D.
    Tabarelli, T.
    Marco, J.
    Doroba, K.
    Wilkinson, G.
    Kucharczyk, M.
    Gokieli, R.
    Ronchese, P.
    Nemecek, S.
    Oblakowska-Mucha, A.
    Verdier, P.
    Nassiakou, M.
    Valenti, G.
    Kluit, P.
    Passeri, A.
    Markou, A.
    Chapkin, M.
    Foeth, H.
    Gazis, E.
    De Lotto, B.
    Vegni, G.
    Fulda-Quenzer, F.
    Leitner, R.
    Matteuzzi, C.
    Hamilton, K.
    Hamacher, K.
    Weiser, C.
    Jeans, D.
    Cosme, G.
    Bloch, D.
    Pieri, L.
    Ridky, M.
    Amapane, N.
    Murray, W.
    Baubillier, M.
    Kernel, G.
    Szwed, Jerzy
    Allmendinger, T.
    Bruckman, P.
    Perrotta, A.
    Jarlskog, G.
    Zhuravlov, V.
    Mjoernmark, U.
    Montenegro, J.
    Ekelof, T.
    Checchia, P.
    Witek, M.
    Sekulin, R.
    Stocchi, A.
    Tyapkin, I. A.
    Piedra, J.
    Mitaroff, W.
    Chung, S. U.
    Bracko, M.
    Obraztsov, V.
    Schwickerath, U.
    Goncalves, P.
    Parzefall, U.
    Chliapnikov, P.
    Marco, R.
    Mc Nulty, R.
    Espirito Santo, M. C.
    Troncon, C.
    Becks, K-H.
    Osterberg, K.
    Fassouliotis, D.
    Collins, P.
    Lamsa, J.
    Pol, M. E.
    Rebecchi, P.
    Zalewski, P.
    Roudeau, P.
    Venus, W.
    Da Silva, W.
    Palka, H.
    Savoy-Navarro, A.
    Graziani, E.
    Morettini, P.
    Perepelitsa, V.
    Grzelak, K.
    Wahlen, H.
    Bardin, D.
    Kourkoumelis, C.
    Moch, M.
    Feindt, M.
    Kjaer,N. J.
    Lipniacka, A.
    Golob, B.
    Sadovsky, A.
    Rehn, J.
    Andringa, S.
    Navarria, F.
    De Min, A.
    Strauss, J.
    Besson, N.
    VanDam, P.
    Timmermans, J.
    Charpentier, Ph.
    Szeptycka, M.
    Alemany-Fernandez, R.
    Peralta, L.
    Tegenfeldt, F.
    Houlden, M. A.
    Masik, J.
    Hoffman, J.
    Lopes, J. H.
    Lemonne, J.
    Travnicek, P.
    Joram, C.
    Monge, R.
    Kersevan, B. P.
    Tristram, G.
    Boonekamp, M.
    Gandelman, M.
    Holt, P. J.
    Amaldi, U.
    Kokkinias, P.
    Pullia, A.
    Anashkin, E.
    Lopez, J. M.
    Reinhardt, R.
    Canale, V.
    Paiano, S.
    Słomiński, Wojciech
    De Angelis, A.
    Calvi, M.
    Opis:
    The hadronic part of the electron structure function $F_{2}^{e}$ has been measured for the first time, using $e^{+}e^{-} $ data collected by the DELPHI experiment at LEP, at centre-of-mass energies of $\sqrt{s}$=91.2-209.5 GeV. The data analysis is simpler than that of the measurement of the photon structure function. The electron structure function $F_{2}^{e}$ data are compared to predictions of phenomenological models based on the photon structure function. It is shown that the contribution of large target photon virtualities is significant. The data presented can serve as a cross-check of the photon structure function $F_{2}^{\gamma}$ analyses and help in refining existing parameterisations.
    Dostawca treści:
    Repozytorium Uniwersytetu Jagiellońskiego
    Artykuł
    Tytuł:
    Prospects for dark matter observations in dwarf spheroidal galaxies with the Cherenkov Telescope Array Observatory
    Autorzy:
    Pandey, A.
    Cristofari, P.
    Siejkowski, H.
    Karas, V.
    Cicciari, G. M.
    Saturni, F. G.
    Jarnot, C.
    Chadwick, P. M.
    Kubo, H.
    Roache, E.
    Meyer, D. M.-A.
    Burmistrov, L.
    Nosek, D.
    Simongini, A.
    Lindfors, E.
    Escarate, P.
    Komin, N.
    de Gouveia Dal Pino, E. M.
    Gallozzi, S.
    Leone, F.
    Hadasch, D.
    Yao, Y.
    Zhang, W.
    Mereghetti, S.
    Pech, M.
    Bottacini, E.
    Kluźniak, W.
    Hara, S.
    Okumura, A.
    Laadim, F. De Frondat
    García-Lago, F. Frías
    Biland, A.
    Galanti, G.
    Ponti, G.
    Abhishek, A.
    Green, D.
    Silvestri, G.
    Takahashi, M.
    Zech, A.
    Stamerra, A.
    Živec, M.
    Zavrtanik, M.
    Paredes, J. M.
    Vigorito, C F.
    Lombardi, S.
    Nieto, D.
    Nishijima, K.
    Stuani, L. Augusto
    Romano, P.
    Sáez, J. Buces
    Bosnjak, Z.
    Gradetzke, T.
    Rando, R.
    Ferrarotto, F.
    Sano, H.
    Brose, R.
    Doro, M.
    Zamanillo, V. Moya
    Chiavassa, A.
    Balazs, C.
    Chen, Y.
    Bringmann, T.
    Sánchez-Conde, M.
    Spinello, S.
    Antonelli, L. A.
    Giordano, F.
    Vandenbroucke, J.
    Gianotti, F.
    Rodríguez-Fernández, G.
    Tanaka, S. J.
    Berge, D.
    Vacula, M.
    Goldoni, P.
    Ricci, C.
    Miener, T.
    Bahilo, J. Lozano
    Aguasca-Cabot, A.
    Batista, P. I.
    Caraveo, P.
    Barrio, J. A.
    Contreras, J. L.
    Burton, M.
    Cotter, G.
    Fedorova, E.
    Prouza, M.
    Voutsinas, G.
    Berti, A.
    Mackey, J.
    Calisse, P. G.
    Germani, S.
    Cascone, E.
    Cerasole, D.
    Kowal, G.
    Lamastra, A.
    Rowell, G.
    Travnicek, P.
    Kushida, J.
    Hussain, S.
    Vercellone, S.
    Romeo, G.
    Dazzi, F.
    Amans, J.-P.
    Del Burgo, R.
    Paoletti, R.
    Tejedor, L. A.
    Larriva, A. Baquero
    Torres, D. F.
    Blanch, O.
    Djuvsland, J.
    Testa, V.
    Linhoff, M.
    Chernyakova, M.
    Eckner, C.
    Chon, G.
    Xotta, F.
    Pantaleo, F. R.
    Leonora, E.
    Majumdar, P.
    Otero-Santos, J.
    Orito, R.
    Falceta-Goncalves, D.
    Gaug, M.
    Castro-Tirado, A. J.
    Alfaro, R.
    Kaufmann, S.
    Cerruti, M.
    Hnatyk, R.
    Beck, G.
    Mello, A. J. T. S.
    Jaroschewski, I.
    Martínez, I. Jiménez
    Pirola, G.
    Paiva, J. G. Giesbrecht Formiga
    Ducci, L.
    Pintore, F.
    Sergijenko, O.
    Tothill, N.
    Kerszberg, D.
    Beshley, V.
    Persic, M.
    Sapienza, V.
    Ruina, A.
    Depaoli, D.
    Gasbarra, C.
    Viaux, N.
    Tutone, A.
    Glicenstein, J.-F.
    Malyshev, D.
    Pumo, M. L.
    Furniss, A.
    Elsässer, D.
    Parmiggiani, N.
    Sangiorgi, P.
    Stanič, S.
    Esposito, P.
    Fukui, Y.
    Castignani, G.
    Yamazaki, R.
    Kazanas, D.
    Mariotti, M.
    Bonollo, A.
    Kataoka, J.
    Girolamo, T. Di
    Wierzcholska, A.
    Principe, G.
    Batzofin, R.
    Fiasson, A.
    Longo, F.
    Aguirre-Santaella, A.
    Ramos, A. Moreno
    Murach, T.
    Emery, G.
    Schiavone, F.
    Novotny, V.
    de Leon, A. Rosales
    Gasparrini, D.
    de Souza, V.
    Dwarkadas, V. V.
    Martínez, M.
    Fukazawa, Y.
    Acero, F.
    Verna, G.
    Reis, I.
    Zuriaga-Puig, J.
    Lacave, B.
    Viana, A.
    Morselli, A.
    Podobnik, F.
    Pagliaro, A.
    de Lavergne, M. de Bony
    Recchia, S.
    Barrios-Jiménez, L.
    Cornejo, B.
    Coelho, J. Goulart
    Hoffmann, D.
    Mitchell, A.
    Salzmann, H.
    Pfeifle, F.
    Rodríguez-Vázquez, J. J.
    Fegan, S.
    Gammaldi, V.
    Hofmann, W.
    Olive, J.-F.
    Hassan, T.
    D’Amico, G.
    Piano, A. Di
    Keita, T.
    Savchenko, V.
    Perrotta, F.
    Pecimotika, M.
    López-Moya, M.
    Mazin, D.
    Molfese, C.
    Carosi, R.
    Gallego, J. Méndez
    Panebianco, G.
    Takeishi, R.
    Volpe, D. della
    Fiandrini, E.
    Torradeflot, F.
    Kieda, D. B.
    Neto, J. P.
    Galaz, G.
    López-Coto, R.
    Hanlon, W.
    Oya, I.
    Incardona, F.
    Janecek, P.
    Martínez, G. A.
    Dinesh, A.
    Siqueira, C.
    Montaruli, T.
    Arcaro, C.
    Grolleron, G.
    Queiroz, F. S.
    Luciani, H.
    Heckmann, L.
    Caroff, S.
    Inada, T.
    Lazarević, S.
    Sol, H.
    Acosta, M. Vázquez
    Kornecki, P.
    Tibaldo, L.
    Hayashi, K.
    Garczarczyk, M.
    Heller, M.
    Orlando, E.
    Capasso, G.
    Hrupec, D.
    Tonev, D.
    Starecki, T.
    Brunelli, G.
    Carquin, E.
    Vassiliev, V.
    Blazek, J.
    Palatiello, M.
    De Angelis, A.
    Horvath, P.
    Moralejo, A.
    Yoshikoshi, T.
    Batković, I.
    Fontaine, G.
    Alfaro, J.
    Rhode, W.
    Costantini, H.
    Gréaux, L.
    de Naurois, M.
    Lenain, J.-P.
    Pinchbeck, L.
    Orlando, S.
    Moulin, E.
    Sarkar, S.
    Marsella, G.
    Inoue, Y.
    Miranda, J. M.
    Abe, S.
    Bunse, M.
    Barbera, A. La
    Aguilera, A. Pérez
    Böttcher, M.
    Ong, R. A.
    Rizi, V.
    Meyer, M.
    Pierro, F. Di
    Amato, E.
    Miceli, M.
    Inoue, S.
    Cortina, J.
    Pohl, M.
    Prandini, E.
    Macias, O.
    Nemmen, R.
    Truzzi, S.
    Orlandini, M.
    Molina, E.
    Abhir, J.
    Pietropaolo, E.
    Roy, A.
    White, M.
    del Peral, L.
    Tjus, J. Becker
    Lyard, E.
    Sadeh, I.
    Menon, S.
    Curtis-Ginsberg, Z.
    Donini, A.
    Ambrosino, D.
    Kolar, D.
    Márquez, I.
    Cifuentes, A.
    Green, J. G.
    Diebold, S.
    Niemiec, J.
    Bonnoli, G.
    González, C. Pozo
    Tian, W. W.
    Vorobiov, S.
    Granot, J.
    Peresano, M.
    Feng, Q.
    Chai, Y.
    De Palma, G.
    Sofia, I.
    Delgado, C.
    Duangchan, C.
    Paneque, D.
    Jahanvi, -
    Saha, L.
    Tramacere, A.
    Acharyya, A.
    Hnatyk, B.
    Stolarczyk, T.
    Reimer, O.
    Voitsekhovskyi, V.
    Guedes, L. M. V.
    Mandat, D.
    Bigongiari, C.
    Pollet, V.
    Dörner, J.
    Vecchi, M.
    Visentin, E.
    Ríos, C.
    Nikołajuk, M.
    Quirrenbach, A.
    Schipani, P.
    Foffano, L.
    Domínguez, D. Martín
    Backes, M.
    Miceli, D.
    Conforti, V.
    Soto, S. García
    Marchetti, A.
    Campoy-Ordaz, A.
    Fioretti, V.
    Araujo, C. H. Coimbra
    Giglietto, N.
    Muraishi, H.
    Cuevas, O.
    D’Ammando, F.
    Walter, R.
    Richtler, T.
    Martinez, O.
    Teshima, M.
    Sengupta, D.
    Agudo, I.
    Batista, R. Alves
    Capuzzo-Dolcetta, R.
    Rosillo, M. Nievas
    Balbo, M.
    Tingay, S. J.
    Loporchio, S.
    Ruiz-Velasco, E.
    Ambrosino, F.
    Molero, M.
    Bernardini, E.
    Bissaldi, E.
    Ebr, J.
    Noda, K.
    Zhdanov, V. I.
    Reimer, A.
    Vigliano, A.
    Adam, R.
    Egberts, K.
    Wechakama, M.
    Ferrand, G.
    Bronzini, E.
    Tajima, H.
    Manicò, G.
    González, J. M.
    Alispach, C.
    Asano, K.
    Chudoba, J.
    del Valle, M. V.
    Tibolla, O.
    Viale, I.
    Glombitza, J.
    Munari, K.
    Nakamori, T.
    Rico, J.
    Hiroshima, N.
    Frías, M. D. Rodríguez
    Savarese, S.
    Jean, P.
    Petruk, O.
    Reisenegger, A.
    Pittori, C.
    Giuffrida, R.
    Cantlay, B. K.
    Kohri, K.
    Jamrozy, Marek
    Iocco, F.
    Pueschel, E.
    Michailidis, M.
    Ambrosi, G.
    Iarlori, M.
    Jin, W.
    Ventura, S.
    Moghadam, M. Ozlati
    Iuliano, A.
    Harvey, V. M.
    Carrasco, M.-S.
    Sguera, V.
    Ghalumyan, A.
    Heß, B.
    Regeard, M.
    Ascasibar, Y.
    Tria, R. Di
    Scherer, A.
    Pérez-Romero, J.
    van Eldik, C.
    Bhattacharyya, S.
    Rainò, S.
    Jurysek, J.
    Cortínez, A. Cerviño
    De Lotto, B.
    Nozaki, S.
    Peron, G.
    Luque-Escamilla, P. L.
    Lapington, J.
    Mangano, S.
    Schussler, F.
    Ribó, M.
    Benbow, W.
    Li, Y.
    Delicado, M. Molina
    Wohlleben, F.
    Santos-Lima, R.
    Kissmann, R.
    Láinez, M.
    Riitano, L.
    Trois, A.
    Rudak, B.
    David, L.
    Zavrtanik, D.
    Starling, R.
    Hamal, P.
    Filipovic, M.
    Costa, A.
    Palombara, N. La
    Gueta, O.
    Sliusar, V.
    González, J. Becerra
    Abe, K.
    Godoy, M. Escobar
    Venere, L. Di
    Aramo, C.
    Martins, V. Barbosa
    Kalekin, O.
    Bernete, J.
    Spiga, D.
    Bhattacharjee, P.
    Patricelli, B.
    Chen, A. W.
    Pühlhofer, G.
    Nieves, C. Escañuela
    Colapietro, M.
    Vitale, V.
    Vignatti, J.
    López-Oramas, A.
    Ettori, S.
    Jankowsky, F.
    Bartolini, C.
    Horan, D.
    Chaty, S.
    Muraczewski, A.
    Suda, Y.
    Rieger, F.
    Angel, L.
    Tombesi, F.
    Bertucci, B.
    Caproni, A.
    Poireau, V.
    Rosado, J.
    Opis:
    The dwarf spheroidal galaxies (dSphs) orbiting the Milky Way are widely regarded as systems supported by velocity dispersion against self-gravity, and as prime targets for the search for indirect dark matter (DM) signatures in the GeV-to-TeV $\gamma$-ray range owing to their lack of astrophysical $\gamma$-ray background. We present forecasts of the sensitivity of the forthcoming Cherenkov Telescope Array Observatory (CTAO) to annihilating or decaying DM signals in these targets. An original selection of candidates is performed from the current catalogue of known objects, including both classical and ultrafaint dSphs. For each, the expected DM content is derived using the most comprehensive photometric and spectroscopic data available, within a consistent framework of analysis. This approach enables the derivation of novel astrophysical factor profiles for indirect DM searches, which are compared with results from the literature. From an initial sample of 64 dSphs, eight promising targets are identified – Draco I, Coma Berenices, Ursa Major II, Ursa Minor, and Willman 1 in the North, Reticulum II, Sculptor, and Sagittarius II in the South – for which different DM density models yield consistent expectations, leading to robust predictions. CTAO is expected to provide the strongest limits above ∼ 10 TeV, reaching velocity-averaged annihilation cross sections of $\sim 5 \times 10^{-25} cm^{3} s^{-1}$ and decay lifetimes up to $\sim 10^{26}$ s for combined limits. The dominant uncertainties arise from the imprecise determination of the DM content, particularly for ultrafaint dSphs. Observation strategies are proposed that optimize either deep exposures of the best candidates or diversified target selections.
    Dostawca treści:
    Repozytorium Uniwersytetu Jagiellońskiego
    Artykuł
    Tytuł:
    PRISM (Polarized Radiation Imaging and Spectroscopy Mission) : an extended white paper
    Autorzy:
    Negrello, Mattia
    Tartari, Andrea
    Naselsky, Pavel
    Comis, Barbara
    Silva, Antonio Da
    Piacentini, Francesco
    Rosset, Cyrille
    Nati, Federico
    Fosalba, Pablo
    Perrotta, Francesca
    Petris, Marco de
    Cuttaia, Francesco
    Battye, Richard
    Ghribi, Adnan
    Chluba, Jens
    Trombetti, Tiziana
    Lattanzi, Massimiliano
    Verde, Licia
    Maino, Davide
    Avillez, Miguel de
    Bouchet, François
    Mangilli, Anna
    Macias-Perez, Juan
    Bucher, Martin
    Stompor, Radek
    Fuller, Gary
    Enßlin, Torsten
    Bendo, George
    Boulanger, François
    Davis, Richard
    Liguori, Michele
    Bartolo, Nicola
    Grainge, Keith
    Béthermin, Matthieu
    Barreiro, Belen
    Falgarone, Edith
    Martinez-Gonzalez, Enrique
    Errard, Josquin
    André, Philippe
    Ponthieu, Nicolas
    Banday, Anthony
    Bonaldi, Anna
    Lesgourgues, Julien
    Natoli, Paolo
    Tristram, Matthieu
    Castex, Guillaume
    Pollo, Agnieszka
    Wandelt, Ben
    Zotti, Gianfranco de
    Watson, Robert
    Liuzzo, Elisabetta
    Trappe, Neil
    Challinor, Anthony
    Hamilton, Jean-Christophe
    Schillaci, Alessandro
    Bernard, Jean-Philippe
    Noviello, Fabio
    Paladino, Rosita
    Rubino-Martin, Jose-Alberto
    Delabrouille, Jacques
    Ganga, Ken
    Lopez-Caniego, Marcos
    Burigana, Carlo
    Massardi, Marcella
    Casasola, Viviana
    Mennella, Aniello
    Rosa, Adriano de
    Ferrière, Katia
    Camus, Philippe
    Miville-Deschênes, Marc-Antoine
    Silk, Joseph
    Murphy, Anthony
    Shellard, Paul
    Cai, Zhen-Yi
    Palanque-Delabrouille, Nathalie
    Jackson, Mark
    Khatri, Rishi
    Bartlett, James
    Martins, Carlos J. A. P.
    Paoletti, Daniela
    Casas, Francisco
    Piccirillo, Lucio
    Giard, Martin
    Herranz, Diego
    Melchiorri, Alessandro
    Bersanelli, Marco
    Hernandez-Monteagudo, Carlos
    Chon, Gayoung
    Hall, Alex
    Dunkley, Joanna
    Barbosa, Domingos
    Galli, Silvia
    Ferreira, Pedro
    Colafrancesco, Sergio
    Monfardini, Alessandro
    Bernardis, Paolo de
    Maffei, Bruno
    Matarrese, Sabino
    Polenta, Gianluca
    Lamagna, Luca
    Jaffe, Andrew
    Benoȋt, Alain
    García-Bellido, Juan
    Masi, Silvia
    Dickinson, Clive
    Toffolatti, Luigi
    Tucci, Marco
    Weijgaert, Rien Van de
    Paci, Francesco
    Ricciardi, Sara
    Finelli, Fabio
    Gonzalez-Nuevo, Joaquin
    Gruppuso, Alessandro
    Kunz, Martin
    Fletcher, Andrew
    Giraud-Héraud, Yannick
    Roman, Matthieu
    Baccigalupi, Carlo
    Désert, François-Xavier
    Peiris, Hiranya
    Vielva, Patricio
    Terenzi, Luca
    Salatino, Maria
    Bielewicz, Pawel
    O'Sullivan, Créidhe
    Tent, Bartjan Van
    Leahy, Paddy
    Brand, Jan
    Remazeilles, Mathieu
    Pisano, Giampaolo
    Sunyaev, Rashid
    Withington, Stafford
    Starobinsky, Alexei
    Melin, Jean-Baptiste
    Tomasi, Maurizio
    Pagano, Luca
    Haverkorn, Marijke
    D'Alessandro, Giuseppe
    Piat, Michel
    Battistelli, Elia
    Diego, Jose Maria
    Mignano, Arturo
    Opis:
    PRISM (Polarized Radiation Imaging and Spectroscopy Mission) was proposed to ESA in May 2013 as a large-class mission for investigating within the framework of the ESA Cosmic Vision program a set of important scientific questions that require high resolution, high sensitivity, full-sky observations of the sky emission at wavelengths ranging from millimeter-wave to the far-infrared. PRISM's main objective is to explore the distant universe, probing cosmic history from very early times until now as well as the structures, distribution of matter, and velocity flows throughout our Hubble volume. PRISM will survey the full sky in a large number of frequency bands in both intensity and polarization and will measure the absolute spectrum of sky emission more than three orders of magnitude better than COBE FIRAS. The data obtained will allow us to precisely measure the absolute sky brightness and polarization of all the components of the sky emission in the observed frequency range, separating the primordial and extragalactic components cleanly from the galactic and zodiacal light emissions. The aim of this Extended White Paper is to provide a more detailed overview of the highlights of the new science that will be made possible by PRISM, which include: (1) the ultimate galaxy cluster survey using the Sunyaev-Zeldovich (SZ) effect, detecting approximately 10^{6} clusters extending to large redshift, including a characterization of the gas temperature of the brightest ones (through the relativistic corrections to the classic SZ template) as well as a peculiar velocity survey using the kinetic SZ effect that comprises our entire Hubble volume; (2) a detailed characterization of the properties and evolution of dusty galaxies, where the most of the star formation in the universe took place, the faintest population of which constitute the diffuse CIB (Cosmic Infrared Background); (3) a characterization of the B modes from primordial gravity waves generated during inflation and from gravitational lensing, as well as the ultimate search for primordial non-Gaussianity using CMB polarization, which is less contaminated by foregrounds on small scales than the temperature anisotropies; (4) a search for distortions from a perfect blackbody spectrum, which include some nearly certain signals and others that are more speculative but more informative; and (5) a study of the role of the magnetic field in star formation and its interaction with other components of the interstellar medium of our Galaxy. These are but a few of the highlights presented here along with a description of the proposed instrument.
    Dostawca treści:
    Repozytorium Uniwersytetu Jagiellońskiego
    Artykuł
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