Zobrazeno 1 - 10
of 22
pro vyhledávání: '"Tur, Clarisse"'
Publikováno v:
Phys.Rev.Lett.106:152501,2011
We have studied the sensitivity to variations in the triple alpha and 12C(alpha, gamma)16O reaction rates, of the yield of the neutrino process isotopes 7Li,11B, 19F, 138La, and 180Ta in core collapse supernovae. Compared to solar abundances, less th
Externí odkaz:
http://arxiv.org/abs/1102.4858
We have studied the sensitivity of supernova production of the gamma emitting nuclei 26Al, 44Ti and 60Fe to variations of the rates of the triple alpha and 12C(alpha, gamma) reactions. Over a range of twice their experimental uncertainties we find va
Externí odkaz:
http://arxiv.org/abs/1012.4732
Publikováno v:
Nucl.Instrum.Meth.A620:351-358,2010
We have characterized two state-of-the-art solid-state photomultipliers, one by SensL, the other by Hamamatsu, coupled to scintillators by Saint-Gobain Crystals in the -25 to 50 degrees C temperature range. At room temperature, the energy resolution
Externí odkaz:
http://arxiv.org/abs/0911.2429
Publikováno v:
Astrophys.J.718:357-367,2010
We have studied the sensitivity to variations in the the triple alpha and 12C(a,g)16O reaction rates of the production of 26Al, 44Ti, and 60Fe in core-collapse supernovae. We used the KEPLER code to model the evolution of 15, 20, and 25 solar mass st
Externí odkaz:
http://arxiv.org/abs/0908.4283
Publikováno v:
Astrophys.J.702:1068-1077,2009
We have studied the sensitivity of s-process nucleosynthesis in massive stars to +/- 2 sigma variations in the rates of the triple alpha and 12C(a,g)16O reactions. We simulated the evolution of massive stars from H-burning through Fe-core collapse, f
Externí odkaz:
http://arxiv.org/abs/0809.0291
We explore the dependence of pre-supernova evolution and supernova nucleosynthesis yields on the uncertainties in helium burning reaction rates. Using the revised solar abundances of Lodders (2003) for the initial stellar composition, instead of thos
Externí odkaz:
http://arxiv.org/abs/0705.4404
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 2010 620(2):351-358
Autor:
Masi, Rita, Garcon, Michel, Zhao, Bo, Amaryan, Moscov, Amaryan, Moskov, Ambrozewicz, Pawel, Anghinolfi, Marco, Asryan, Gegham, Avagyan, Harutyun, Baghdasaryan, Hovhannes, Baillie, Nathan, Ball, J. P., Ball, Jacques, Ball, James, Baltzell, Nathan, Baturin, Vitaly, Battaglieri, Marco, Bedlinskiy, Ivan, Bellis, Matthew, Benmouna, Nawal, Berman, Barry, Bertin, Pierre, Biselli, Angela, Blaszczyk, Lukasz, Bouchigny, Sylvain, Boyarinov, Sergey, Bradford, Robert, Branford, Derek, Briscoe, William, Brooks, William, Bultmann, S., Bueltmann, Stephen, Burkert, Volker, Butuceanu, Cornel, Calarco, John, Careccia, Sharon, Carman, Daniel, Casey, Liam, Chen, Shifeng, Cheng, Lu, Cole, Philip, Collins, Patrick, Coltharp, Philip, Crabb, Donald, Crede, Volker, Dashyan, Natalya, Sanctis, Enzo, Vita, Raffaella, Degtiarenko, Pavel, Deur, Alexandre, Dharmawardane, Kahanawita, Dickson, Richard, Djalali, Chaden, Dodge, Gail, Donnelly, Joseph, Doughty, David, Dugger, Michael, Dzyubak, Oleksandr, Egiyan, Hovanes, Egiyan, Kim, Elfassi, Lamiaa, Elouadrhiri, Latifa, Eugenio, Paul, Fedotov, Gleb, Feldman, Gerald, Fradi, Ahmed, Funsten, Herbert, Gavalian, Gagik, Gilfoyle, Gerard, Giovanetti, Kevin, Girod, Francois-Xavier, Goetz, John, Gonenc, Atilla, Gothe, Ralf, Griffioen, Keith, Guidal, Michel, Guler, Nevzat, Guo, Lei, Gyurjyan, Vardan, Hafidi, Kawtar, Hakobyan, Hayk, Hanretty, Charles, Hersman, F., Hicks, Kenneth, Hleiqawi, Ishaq, Holtrop, Maurik, Hyde, Charles, Ilieva, Yordanka, Ireland, David, Ishkhanov, Boris, Isupov, Evgeny, Ito, Mark, Jenkins, David, Jo, Hyon-Suk, Johnstone, John, Joo, Kyungseon, Juengst, Henry, Kalantarians, Narbe, Kellie, James, Khandaker, Mahbubul, Kim, Wooyoung, Klein, Andreas, Klein, Franz, Klimenko, Alexei, Kossov, Mikhail, Krahn, Zebulun, Kramer, Laird, Kubarovsky, Valery, Kuhn, Joachim, Kuhn, Sebastian, Kuleshov, Sergey, Lachniet, Jeff, Laget, Jean, Langheinrich, Jorn, Lawrence, David, Lee, Tsung-Shung, Livingston, Kenneth, Lu, Haiyun, Maccormick, Marion, Markov, Nikolai, Mattione, Paul, Mazouz, Malek, Mckinnon, Bryan, Mecking, Bernhard, Mestayer, Mac, Meyer, Curtis, Mibe, Tsutomu, Michel, Bernard, Mikhaylov, Konstantin, Mirazita, Marco, Miskimen, Rory, Mokeev, Viktor, Moreno, Brahim, Moriya, Kei, Morrow, Steven, Moteabbed, Maryam, Munevar Espitia, Edwin, Mutchler, Gordon, Nadel-Turonski, Pawel, Nasseripour, Rakhsha, Niccolai, Silvia, Niculescu, Gabriel, Niculescu, Maria-Ioana, Niczyporuk, Bogdan, Niroula, Megh, Niyazov, Rustam, Nozar, Mina, Osipenko, Mikhail, Ostrovidov, Alexander, Park, Kijun, Pasyuk, Evgueni, Paterson, Craig, Pereira, Sergio, Pierce, Joshua, Pivnyuk, Nikolay, Pocanic, Dinko, Pogorelko, Oleg, Pozdnyakov, Sergey, Price, John, Procureur, Sebastien, Prok, Yelena, Protopopescu, Dan, Raue, Brian, Ricco, Giovanni, Ripani, Marco, Ritchie, Barry, Ronchetti, Federico, Rosner, Guenther, Rossi, Patrizia, Sabatie, Franck, Salamanca, Julian, Salgado, Carlos, Santoro, Joseph, Sapunenko, Vladimir, Schumacher, Reinhard, Serov, Vladimir, Sharabian, Youri, Sharov, Dmitri, Shvedunov, Nikolay, Smith, Elton, Smith, Lee, Sober, Daniel, Sokhan, Daria, Stavinsky, Aleksey, Stepanyan, Samuel, Stepanyan, Stepan, Stokes, Burnham, Stoler, Paul, Strakovski, Igor, Strauch, Steffen, Taiuti, Mauro, Tedeschi, David, Tkabladze, Avtandil, Tkachenko, Svyatoslav, Tur, Clarisse, Ungaro, Maurizio, Vineyard, Michael, Vlassov, Alexander, Voutier, Eric, Watts, Daniel, Weinstein, Lawrence, Weygand, Dennis, Williams, Michael, Wolin, Elliott, Wood, Michael, Yegneswaran, Amrit, Zana, Lorenzo, Zhang, Jixie, Zhiwen Zhao
Publikováno v:
Physical Review C
Physical Review C, 2008, 77, pp.042201. ⟨10.1103/PhysRevC.77.042201⟩
Physical Review C, American Physical Society, 2008, 77, pp.042201. ⟨10.1103/PhysRevC.77.042201⟩
DOE / OSTI
Physical Review C, 2008, 77, pp.042201. ⟨10.1103/PhysRevC.77.042201⟩
Physical Review C, American Physical Society, 2008, 77, pp.042201. ⟨10.1103/PhysRevC.77.042201⟩
DOE / OSTI
5 pages, 6 figures; The beam spin asymmetry (BSA) in the exclusive reaction ep->ep pi0 was measured with the CEBAF 5.77 GeV polarized electron beam and Large Acceptance Spectrometer(CLAS). The xB, Q2, t and phi dependences of the pi0 BSA are presente
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::daefad2585f421ea54929ec777546caf
https://hal.in2p3.fr/in2p3-00192985
https://hal.in2p3.fr/in2p3-00192985
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Akademický článek
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